Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_A/661/A5 into FORTRAN code for loading all data files into arrays.
Note that special values are assigned to unknown or unspecified
numbers (also called NULL numbers);
when necessary, the coordinate components making up the right ascension
and declination are converted into floating-point numbers
representing these angles in degrees.
program load_ReadMe
C=============================================================================
C F77-compliant program generated by readme2f_1.81 (2015-09-23), on 2026-May-18
C=============================================================================
* This code was generated from the ReadMe file documenting a catalogue
* according to the "Standard for Documentation of Astronomical Catalogues"
* currently in use by the Astronomical Data Centers (CDS, ADC, A&A)
* (see full documentation at URL http://vizier.u-strasbg.fr/doc/catstd.htx)
* Please report problems or questions to
C=============================================================================
implicit none
* Unspecified or NULL values, generally corresponding to blank columns,
* are assigned one of the following special values:
* rNULL__ for unknown or NULL floating-point values
* iNULL__ for unknown or NULL integer values
real*4 rNULL__
integer*4 iNULL__
parameter (rNULL__=--2147483648.) ! NULL real number
parameter (iNULL__=(-2147483647-1)) ! NULL int number
integer idig ! testing NULL number
C=============================================================================
Cat. J/A+A/661/A5 The eFEDS AGN catalog (Liu+, 2022)
*================================================================================
*The eROSITA Final Equatorial-Depth Survey (eFEDS).
*The AGN catalog and its X-ray spectral properties.
* Liu T., Buchner J., Nandra K., Merloni A., Dwelly T., Sanders J.S.,
* Salvato M., Arcodia R., Brusa M., Wolf J., Georgakakis A., Boller T.,
* Krumpe M., Lamer G., Waddell S., Urrutia T., Schwope A., Robrade J.,
* Wilms J., Dauser T., Comparat J., Toba Y., Ichikawa K., Iwasawa K.,
* Shen Y., Medel H.I.
* <Astron. Astrophys. 661, A5 (2022)>
* =2022A&A...661A...5L
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! The eFEDS AGN catalog
integer*4 nr__
parameter (nr__=22079) ! Number of records
character*736 ar__ ! Full-size record
C J2000 position composed of: RAcdeg DEcdeg
integer*4 ID_SRC (nr__) ! [1/32683] ID of the sources in the eFEDS
* main X-ray catalog (Paper I) (ID_SRC)
real*8 RAcdeg (nr__) ! (deg) [126.24/145.59] Right ascension (J2000),
* astrometric corrected (Paper I)
* (RA_CORR)
real*4 DEcdeg (nr__) ! (deg) [-2.91/5.97] Declination (J2000),
* astrometric corrected (Paper I)
* (DEC_CORR)
real*8 DetLike (nr__) ! 0.2-2.3 keV source detection likelihood
* (Paper I) (DET_LIKE)
real*4 inArea90 (nr__) ! Whether located inside the inner
* 90%-area region of eFEDS (Paper I)
* (inArea90)
character*11 CTPLS8 (nr__) ! ID of the best LS8 counterpart
* (Paper II) (CTP_LS8_UNIQUE_OBJID)
real*8 RALdeg (nr__) ! (deg) [126.23/145.59] Right ascension (J2000)
* of the best LS8 counterpart (Paper II)
* (CTP_LS8_RA)
real*4 DELdeg (nr__) ! (deg) [-2.91/5.97] Declination (J2000) of the
* best LS8 counterpart (Paper II)
* (CTP_LS8_DEC)
integer*4 CTPqual (nr__) ! [2/4] Counterpart quality (Paper II)
* A value >=2 is recommended
* (CTP_quality)
integer*4 CTPClass (nr__) ! [2/3] Classification of the optical
* counterpart (Paper II) (CTP_CLASS) (1)
real*8 CTPz (nr__) ! [0.0/8.0] Redshift of the optical
* counterpart (Paper II) (CTP_REDSHIFT)
integer*4 CTPzgrade (nr__) ! [2/5] Redshift Grade (Paper II)
* A value >=3 is recommended
* (CTP_REDSHIFT_GRADE)
integer*4 inKiDSFlag (nr__) ! [0/1] Whether located inside the region
* of the KiDS survey (Paper II)
* (in_KiDS_flag)
integer*4 LxModel (nr__) ! [1/5] Index of selected model for
* luminosity measurement (LxModel) (2)
integer*4 NHclass (nr__) ! [1/4] Class of AGN NH measurement with
* model 1 (single-powerlaw) (NHclass) (3)
integer*4 FSModel (nr__) ! [3/6] Index of selected model for
* 0.5-2keV flux (FSModel) (4)
integer*4 FHModel (nr__) ! [5/7] Index of selected model for
* 2.3-5keV flux (FHModel) (5)
real*4 galNH (nr__) ! (cm-2) Total column density of Galactic
* absorption (galNH)
real*4 galNHI (nr__) ! (cm-2) HI column density from HI4PI (galNHI)
real*8 SrcCts (nr__) ! (ct) Source net counts in the 0.2-5 keV band
* (SrcCts)
real*4 FluxcMedS (nr__) ! (mW/m2) Absorption corrected flux in observed
* 0.5-2 keV, posterior median
* (FluxCorr_Med_s)
real*4 b_FluxcS (nr__) ! (mW/m2) Absorption corrected flux in observed
* 0.5-2 keV, 1sigma lower limit
* (FluxCorr_Lo1_s)
real*4 B_FluxcS_1 (nr__) ! (mW/m2) Absorption corrected flux in observed
* 0.5-2 keV, 1sigma upper limit
* (FluxCorr_Up1_s)
real*4 FluxcMedT (nr__) ! (mW/m2) Absorption corrected flux in observed
* 2.3-5 keV, posterior median
* (FluxCorr_Med_t)
real*4 b_FluxcT (nr__) ! (mW/m2) Absorption corrected flux in observed
* 2.3-5 keV, 1sigma lower limit
* (FluxCorr_Lo1_t)
real*4 B_FluxcT_1 (nr__) ! (mW/m2) Absorption corrected flux in observed
* 2.3-5 keV, 1sigma upper limit
* (FluxCorr_Up1_t)
real*4 FluxIMedS (nr__) ! (mW/m2) Absorption corrected flux in rest-frame
* 0.5-2 keV, posterior median
* (FluxIntr_Med_s)
real*4 b_FluxIS (nr__) ! (mW/m2) Absorption corrected flux in rest-frame
* 0.5-2keV, 1sigma lower limit
* (FluxIntr_Lo1_s)
real*4 B_FluxIS_1 (nr__) ! (mW/m2) Absorption corrected flux in rest-frame
* 0.5-2keV, 1sigma upper limit
* (FluxIntr_Up1_s)
real*4 FluxIMed2keV(nr__) ! (mW/m2/eV) Absorption corrected flux at rest-frame
* 2keV, median (FluxIntr_Med_2keV)
real*4 b_FluxI2keV(nr__) ! (mW/m2/eV) Absorption corrected flux at rest-frame
* 2keV, 1sigma lower limit
* (FluxIntr_Lo1_2keV)
real*4 B_FluxI2keV_1(nr__) ! (mW/m2/eV) Absorption corrected flux at rest-frame
* 2keV, 1sigma upper limit
* (FluxIntr_Up1_2keV)
real*8 LumIMedS (nr__) ! (10-7W) Intrinsic luminosity in rest-frame
* 0.5-2 keV, posterior median
* (LumiIntr_Med_s)
real*8 b_LumIS (nr__) ! (10-7W) Intrinsic luminosity in rest-frame
* 0.5-2 keV, 1sigma lower limit
* (LumiIntr_Lo1_s)
real*8 B_LumIS_1 (nr__) ! (10-7W) Intrinsic luminosity in rest-frame
* 0.5-2 keV, 1sigma upper limit
* (LumiIntr_Up1_s)
real*8 LumIMed2keV(nr__) ! (10-7W/eV) Intrinsic luminosity at rest-frame 2keV,
* posterior median in erg/s/eV
* (LumiIntr_Med_2keV)
real*8 b_LumI2keV (nr__) ! (10-7W/eV) Intrinsic luminosity at rest-frame 2keV,
* 1sigma lower limit in erg/s/eV
* (LumiIntr_Lo1_2keV)
real*8 B_LumI2keV_1(nr__) ! (10-7W/eV) Intrinsic luminosity at rest-frame 2keV,
* 1sigma upper limit in erg/s/eV
* (LumiIntr_Up1_2keV)
real*4 FluxObsMedS(nr__) ! (mW/m2) Observed flux in observed 0.5-2 keV,
* posterior median (FluxObsv_Med_s)
real*4 b_FluxObsS (nr__) ! (mW/m2) Observed flux in observed 0.5-2 keV,
* 1sigma lower limit (FluxObsv_Lo1_s)
real*4 B_FluxObsS_1(nr__) ! (mW/m2) Observed flux in observed 0.5-2 keV,
* 1sigma upper limit (FluxObsv_Up1_s)
real*4 FluxObsMedT(nr__) ! (mW/m2) Observed flux in observed 2.3-5 keV,
* posterior median (FluxObsv_Med_t)
real*4 b_FluxObsT (nr__) ! (mW/m2) Observed flux in observed 2.3-5 keV,
* 1sigma lower limit (FluxObsv_Lo1_t)
real*4 B_FluxObsT_1(nr__) ! (mW/m2) Observed flux in observed 2.3-5 keV,
* 1sigma upper limit (FluxObsv_Up1_t)
real*8 lognHKLm1 (nr__) ! log AGN column density, KL divergence
* (in nats units) (lognH_KL_m1)
real*8 b_lognHm1 (nr__) ! ([cm-2]) log AGN column density, HDI lower limit
* (lognH_HLo_m1)
real*8 B_lognHm1_1(nr__) ! ([cm-2]) log AGN column density, HDI upper limit
* (lognH_HUp_m1)
real*8 lognHMedm1 (nr__) ! ([cm-2]) log AGN column density, posterior median
* (lognH_Med_m1)
real*8 GammaKLm3 (nr__) ! primary power-law slope in model 3,
* KL divergence (in nats units)
* (Gamma_KL_m3)
real*8 b_GammaHm3 (nr__) ! primary power-law slope in model 3,
* HDI lower limit (Gamma_HLo_m3)
real*8 B_GammaHm3_1(nr__) ! primary power-law slope in model 3,
* HDI upper limit (Gamma_HUp_m3)
real*8 GammaMedm3 (nr__) ! primary power-law slope in model 3,
* posterior median (Gamma_Med_m3)
real*8 logZm0 (nr__) ! ([-]) log Bayesian evidence with model 0:
* APEC (logZ_m0)
real*8 logZm1 (nr__) ! ([-]) log Bayesian evidence with model 1:
* single powerlaw (logZ_m1)
real*8 logZm2 (nr__) ! ([-]) log Bayesian evidence with model 2:
* double powerlaw (logZ_m2)
real*8 logZm3 (nr__) ! ([-]) log Bayesian evidence with model 3:
* powerlaw + blackbody (logZ_m3)
real*8 logZm4 (nr__) ! ([-]) log Bayesian evidence with model 4:
* powerlaw with Gamma fixed at 2.0
* (logZ_m4)
real*8 logZm5 (nr__) ! ([-]) log Bayesian evidence with model 5:
* shape-fixed powerlaw (logZ_m5)
real*8 L2500 (nr__) ! (10-7W/Hz) ?=-99.0 The rest-frame 2500 luminosity
* in erg/s/Hz (L2500)
real*8 L5100 (nr__) ! (10-7W/Hz) ?=-99.0 The rest-frame 5100 luminosity
* in erg/s/Hz (L5100)
real*8 W1mag (nr__) ! (mag) ? LS8-WISE W1 AB magnitude (Paper II)
* (W1)
real*4 e_W1mag (nr__) ! (mag) ? LS8-WISE W1 magnitude error (Paper II)
* (W1_ERR)
real*8 W2mag (nr__) ! (mag) ? LS8-WISE W2 AB magnitude (Paper II)
* (W2)
real*4 e_W2mag (nr__) ! (mag) ? LS8-WISE W2 magnitude error (Paper II)
* (W2_ERR)
*Note (1): Classification of the optical counterpart as follows:
* 0 = likely Galactic
* 1 = secure Galactic
* 2 = likely extraGalactic
* 3 = secure extraGalactic
*Note (2): Index of selected model for luminosity measurement as follows:
* 1 = single-powerlaw
* 3 = powerlaw+bb
* 4 = powerlaw with Gamma
*Note (3): Class of AGN NH measurement with model 1 (single-powerlaw) as follows:
* 1 = uninformative
* 2 = unobscured
* 3 = mildly-measured
* 4 = well-measured
*Note (4): Index of selected model for 0.5-2keV flux as follows:
* 5 = counts-based measurement for faint sources
* 0 = robust spectra-based measurement
* 3 = robust spectra-based measurement
* 6 = robust spectra-based measurement
*Note (5): Index of selected model for 2.3-5keV flux as follows:
* 5 = counts-based measurement for faint sources
* 7 = robust spectra-based measurement
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Spectral properties
integer*4 nr__1
parameter (nr__1=27910) ! Number of records
character*645 ar__1 ! Full-size record
C J2000 position composed of: RAdeg DEdeg
integer*4 ID_SRC_1 (nr__1) ! [1/32683] ID of the sources in the eFEDS
* main X-ray catalog (Paper I) (ID_SRC)
real*8 RAcdeg_1 (nr__1) ! (deg) [126.24/145.66] Right ascension (J2000),
* astrometric corrected (Paper I) (RA_CORR)
real*4 DEcdeg_1 (nr__1) ! (deg) [-2.91/5.97] Declination (J2000),
* astrometric corrected (Paper I)
* (DEC_CORR)
real*8 DetLike_1 (nr__1) ! [6.0/33254.59] 0.2-2.3 keV source
* detection likelihood (Paper I) (DET_LIKE)
real*8 ExtLike (nr__1) ! X-ray source extent likelihood (Paper I)
* (EXT_LIKE)
real*4 inArea90_1 (nr__1) ! Whether located inside the inner 90%-area
* region of eFEDS (Paper I) (inArea90)
real*4 galNH_1 (nr__1) ! (cm-2) Total column density of Galactic
* absorption (galNH)
real*4 galNHI_1 (nr__1) ! (cm-2) HI column density from HI4PI (galNHI)
real*8 ExpTime (nr__1) ! (s) Spectra exposure time (Exposure)
real*8 SrcCts_1 (nr__1) ! (ct) Source net counts in the 0.2-5 keV band
* (SrcCts)
real*8 RAdeg (nr__1) ! (deg) [126.24/145.66] Right ascension (J2000)
* before astrometric correction (Paper I)
* (RA)
real*4 DEdeg (nr__1) ! (deg) [-2.91/5.97] Declination (J2000) before
* astrometric correction (Paper I) (DEC)
integer*4 Rad (nr__1) ! (arcsec) [12/259] Source extraction radius (Rad)
integer*4 Ann1 (nr__1) ! (arcsec) [22/515] Inner radius of background
* extraction region (Ann1)
integer*4 Ann2 (nr__1) ! (arcsec) [171/900] Outer radius of background
* extraction region (Ann2)
real*4 RegArea (nr__1) ! (deg2) Geometry area of source extraction region
* (REGAREA_s)
real*4 Backscal (nr__1) ! (deg2) Source BACKSCAL (Backscal_s)
real*8 BackscalBkg(nr__1) ! (deg2) Background BACKSCAL (Backscal_b)
integer*4 FSModel_1 (nr__1) ! [0/6] Index of selected model for
* 0.5-2keV flux (FSModel) (1)
integer*4 FHModel_1 (nr__1) ! [5/7] Index of selected model for
* 2.3-5keV flux (FHModel) (2)
real*4 Rate0_2_2_3(nr__1) ! (ct/s) Net count rate in 0.2-2.3 keV
* (Rate_d2_2d3)
real*8 e_Rate0_2_2_3(nr__1) ! (ct/s) Net count rate error in 0.2-2.3 keV
* (RateErr_d2_2d3)
real*4 Rate0_2_0_5(nr__1) ! (ct/s) Net count rate in 0.2-0.5 keV (Rate_d2_d5)
real*4 e_Rate0_2_0_5(nr__1) ! (ct/s) Net count rate error in 0.2-0.5 keV
* (RateErr_d2_d5)
real*4 Rate0_5_1 (nr__1) ! (ct/s) Net count rate in 0.5-1 keV (Rate_d5_1)
real*4 e_Rate0_5_1(nr__1) ! (ct/s) Net count rate error in 0.5-1 keV
* (RateErr_d5_1)
real*4 Rate1_2 (nr__1) ! (ct/s) Net count rate in 1-2 keV (Rate_1_2)
real*4 e_Rate1_2 (nr__1) ! (ct/s) Net count rate error in 1-2 keV
* (RateErr_1_2)
real*4 Rate2_4_5 (nr__1) ! (ct/s) Net count rate in 2-4.5 keV (Rate_2_4d5)
real*4 e_Rate2_4_5(nr__1) ! (ct/s) Net count rate error in 2-4.5 keV
* (RateErr_2_4d5)
real*4 Rate2_3_5 (nr__1) ! (ct/s) Net count rate in 2.3-5 keV (Rate_2d3_5)
real*4 e_Rate2_3_5(nr__1) ! (ct/s) Net count rate error in 2.3-5 keV
* (RateErr_2d3_5)
real*4 Rate5_8 (nr__1) ! (ct/s) Net count rate in 5-8 keV (Rate_5_8)
real*4 e_Rate5_8 (nr__1) ! (ct/s) Net count rate error in 5-8 keV
* (RateErr_5_8)
real*4 BkgCts0_2_0_6(nr__1) ! (ct) Background counts in 0.2-0.6 keV
* (BkgCts_d2_d6)
real*8 e_BkgCts0_2_0_6(nr__1) ! (ct) Background counts error in 0.2-0.6 keV
* (BkgCtsErr_d2_d6)
real*4 BkgCts0_6_2_3(nr__1) ! (ct) Background counts in 0.6-2.3 keV
* (BkgCts_d6_2d3)
real*8 e_BkgCts0_6_2_3(nr__1) ! (ct) Background counts error in 0.6-2.3 keV
* (BkgCtsErr_d6_2d3)
real*4 BkgCts2_3_5(nr__1) ! (ct) Background counts in 2.3-5 keV
* (BkgCts_2d3_5)
real*8 e_BkgCts2_3_5(nr__1) ! (ct) Background counts error in 2.3-5 keV
* (BkgCtsErr_2d3_5)
real*4 BkgCts5_8 (nr__1) ! (ct) Background counts in 5-8 keV (BkgCts_5_8)
real*8 e_BkgCts5_8(nr__1) ! (ct) Background counts error in 5-8 keV
* (BkgCtsErr_5_8)
real*8 PSFCor0_2_0_5(nr__1) ! PSF-loss correction (ARF CORRPSF) averaged
* in 0.2-0.5 keV (PSFCor_d2_d5)
real*8 PSFCor0_5_1(nr__1) ! PSF-loss correction (ARF CORRPSF) averaged
* in 0.5-1 keV (PSFCor_d5_1)
real*8 PSFCor1_2 (nr__1) ! PSF-loss correction (ARF CORRPSF) averaged
* in 1-2 keV (PSFCor_1_2)
real*8 PSFCor2_3_5(nr__1) ! PSF-loss correction (ARF CORRPSF) averaged
* in 2.3-5 keV (PSFCor_2d3_5)
integer*4 Nempty (nr__1) ! [35/771] Number of empty channels between
* channel 20 and 900 (Nempty)
real*4 FluxObsMedS_1(nr__1) ! (mW/m2) Observed flux in observed 0.5-2 keV,
* posterior median (FluxObsv_Med_s)
real*4 b_FluxObsS_2(nr__1) ! (mW/m2) Observed flux in observed 0.5-2 keV,
* 1sigma lower limit (FluxObsv_Lo1_s)
real*4 B_FluxObsS_3(nr__1) ! (mW/m2) Observed flux in observed 0.5-2 keV,
* 1sigma upper limit (FluxObsv_Up1_s)
real*4 FluxObsMedT_1(nr__1) ! (mW/m2) Observed flux in observed 2.3-5 keV,
* posterior median (FluxObsv_Med_t)
real*4 b_FluxObsT_2(nr__1) ! (mW/m2) Observed flux in observed 2.3-5 keV,
* 1sigma lower limit (FluxObsv_Lo1_t)
real*4 B_FluxObsT_3(nr__1) ! (mW/m2) Observed flux in observed 2.3-5 keV,
* 1sigma upper limit (FluxObsv_Up1_t)
*Note (1): Index of selected model for 0.5-2keV flux as follows:
* 5 = counts-based measurement for faint sources
* 0 = robust spectra-based measurement
* 3 = robust spectra-based measurement
* 6 = robust spectra-based measurement
*Note (2): Index of selected model for 2.3-5keV flux as follows:
* 5 = counts-based measurement for faint sources
* 7 = robust spectra-based measurement
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! APEC fitting results
integer*4 nr__2
parameter (nr__2=27910) ! Number of records
character*715 ar__2 ! Full-size record
integer*4 ID_SRC_2 (nr__2) ! [1/32683] ID of the sources in the eFEDS
* main X-ray catalog (Paper I) (ID_SRC)
real*4 z (nr__2) ! The redshift adopted for the spectral
* model (Redshift)
real*8 lognHKL (nr__2) ! log AGN column density, KL divergence
* (in nats units) (lognH_KL)
real*8 b_lognHH (nr__2) ! ([cm-2]) log AGN column density, HDI lower limit
* (lognH_HLo)
real*8 B_lognHH_1 (nr__2) ! ([cm-2]) log AGN column density, HDI upper limit
* (lognH_HUp)
real*8 logkTKL (nr__2) ! log temperature, KL divergence
* (in nats units) (logkT_KL)
real*4 b_logkTH (nr__2) ! ([keV]) log temperature, HDI lower limit
* (logkT_HLo)
real*4 B_logkTH_1 (nr__2) ! ([keV]) log temperature, HDI upper limit
* (logkT_HUp)
real*8 logAbundKL (nr__2) ! log abundance, KL divergence
* (in nats units) (logAbundanc_KL)
real*8 b_logAbunH (nr__2) ! log abundance, HDI lower limit
* (logAbundanc_HLo)
real*4 B_logAbunH_1(nr__2) ! log abundance, HDI upper limit
* (logAbundanc_HUp)
real*8 logApecNormKL(nr__2) ! log APEC normalization, KL divergence
* (in nats units) (logApecNorm_KL)
real*8 b_logApecNormH(nr__2) ! ([cm-5]) log APEC normalization, HDI lower limit
* (logApecNorm_HLo)
real*8 B_logApecNormH_1(nr__2) ! ([cm-5]) log APEC normalization, HDI upper limit
* (logApecNorm_HUp)
real*8 lognHBF (nr__2) ! ([cm-2]) log AGN column density, best-fit model
* (lognH_BF)
real*4 logkTBF (nr__2) ! ([keV]) log temperature, best-fit model
* (logkT_BF)
real*4 logAbundBF (nr__2) ! log abundance, best-fit model
* (logAbundanc_BF)
real*8 logApecNBF (nr__2) ! ([cm-5]) log APEC normalization, best-fit model
* (logApecNorm_BF)
real*4 FluxObsBFS (nr__2) ! (mW/m2) Observed flux in observed 0.5-2 keV,
* best-fit model (FluxObsv_BF_s)
real*4 FluxObsMedS_2(nr__2) ! (mW/m2) Observed flux in observed 0.5-2 keV,
* posterior median (FluxObsv_Med_s)
real*4 b_FluxObsS_4(nr__2) ! (mW/m2) Observed flux in observed 0.5-2 keV,
* 1sigma lower limit (FluxObsv_Lo1_s)
real*4 B_FluxObsS_5(nr__2) ! (mW/m2) Observed flux in observed 0.5-2 keV,
* 1sigma upper limit (FluxObsv_Up1_s)
real*4 b2_FluxObsS(nr__2) ! (mW/m2) Observed flux in observed 0.5-2 keV,
* 2sigma lower limit (FluxObsv_Lo2_s)
real*4 B2_FluxObsS_1(nr__2) ! (mW/m2) Observed flux in observed 0.5-2 keV,
* 2sigma upper limit (FluxObsv_Up2_s)
real*4 FluxObsBFT (nr__2) ! (mW/m2) Observed flux in observed 2.3-5 keV,
* best-fit model (FluxObsv_BF_t)
real*4 FluxObsMedT_2(nr__2) ! (mW/m2) Observed flux in observed 2.3-5 keV,
* posterior median (FluxObsv_Med_t)
real*4 b_FluxObsT_4(nr__2) ! (mW/m2) Observed flux in observed 2.3-5 keV,
* 1sigma lower limit (FluxObsv_Lo1_t)
real*4 B_FluxObsT_5(nr__2) ! (mW/m2) Observed flux in observed 2.3-5 keV,
* 1sigma upper limit (FluxObsv_Up1_t)
real*4 b2_FluxObsT(nr__2) ! (mW/m2) Observed flux in observed 2.3-5 keV,
* 2sigma lower limit (FluxObsv_Lo2_t)
real*4 B2_FluxObsT_1(nr__2) ! (mW/m2) Observed flux in observed 2.3-5 keV,
* 2sigma upper limit (FluxObsv_Up2_t)
real*8 lognHMed (nr__2) ! ([cm-2]) log AGN column density, posterior median
* (lognH_Med)
real*8 b_lognH (nr__2) ! ([cm-2]) log AGN column density, percentile
* lower limit (lognH_Lo)
real*8 B_lognH_1 (nr__2) ! ([cm-2]) log AGN column density, percentile
* upper limit (lognH_Up)
real*8 lognHMean (nr__2) ! ([cm-2]) log AGN column density, mean (lognH_Mean)
real*8 s_lognH (nr__2) ! ([cm-2]) log AGN column density,
* standard deviation (lognH_Std)
real*4 logkTMed (nr__2) ! ([keV]) log temperature, posterior median
* (logkT_Med)
real*4 b_logkT (nr__2) ! ([keV]) log temperature, percentile lower limit
* (logkT_Lo)
real*4 B_logkT_1 (nr__2) ! ([keV]) log temperature, percentile upper limit
* (logkT_Up)
real*4 logkTMean (nr__2) ! ([keV]) log temperature, mean (logkT_Mean)
real*8 s_logkT (nr__2) ! ([keV]) log temperature, standard deviation
* (logkT_Std)
real*8 logAbundMed(nr__2) ! log abundance, posterior median
* (logAbundanc_Med)
real*8 b_logAbund (nr__2) ! log abundance, percentile lower limit
* (logAbundanc_Lo)
real*8 B_logAbund_1(nr__2) ! log abundance, percentile upper limit
* (logAbundanc_Up)
real*8 logAbundMean(nr__2) ! log abundance, mean (logAbundanc_Mean)
real*8 s_logAbund (nr__2) ! log abundance, standard deviation
* (logAbundanc_Std)
real*8 logApecNMed(nr__2) ! ([cm-5]) log APEC normalization, posterior median
* (logApecNorm_Med)
real*8 b_logApecN (nr__2) ! ([cm-5]) log APEC normalization, percentile
* lower limit (logApecNorm_Lo)
real*8 B_logApecN_1(nr__2) ! ([cm-5]) log APEC normalization, percentile
* upper limit (logApecNorm_Up)
real*8 logApecNMean(nr__2) ! ([cm-5]) log APEC normalization, mean
* (logApecNorm_Mean)
real*8 s_logApecN (nr__2) ! ([cm-5]) log APEC normalization,
* standard deviation (logApecNorm_Std)
real*4 logBkgNMed (nr__2) ! log background normalization,
* posterior median (logBkgNorm_Med)
real*4 b_logBkgN (nr__2) ! log background normalization,
* percentile lower limit (logBkgNorm_Lo)
real*4 B_logBkgN_1(nr__2) ! log background normalization,
* percentile upper limit (logBkgNorm_Up)
real*4 logBkgNMean(nr__2) ! log background normalization,
* mean (logBkgNorm_Mean)
real*8 s_logBkgN (nr__2) ! log background normalization,
* standard deviation (logBkgNorm_Std)
real*8 chi25 (nr__2) ! ?=-99 Chi^2 of the best-fit model against
* the rebinned data (>=25 cts/bin) (chi25)
integer*4 dof25 (nr__2) ! ?=-99 DOF of the rebinned data, which
* has at least 25 counts per bin (dof25)
real*8 logZ (nr__2) ! log10 Bayesian evidence (logZ)
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table4.dat' ! Single-powerlaw results
integer*4 nr__3
parameter (nr__3=27910) ! Number of records
character*990 ar__3 ! Full-size record
integer*4 ID_SRC_3 (nr__3) ! [1/32683] ID of the sources in the
* eFEDS main X-ray catalog (Paper I)
* (ID_SRC)
real*4 z_1 (nr__3) ! [-0.01/8.0] The redshift adopted for
* the spectral model (Redshift)
real*8 GammaKL (nr__3) ! power-law slope, KL divergence
* (in nats units) (Gamma_KL)
real*8 b_GammaH (nr__3) ! power-law slope, HDI lower limit
* (Gamma_HLo)
real*8 B_GammaH_1 (nr__3) ! power-law slope, HDI upper limit
* (Gamma_HUp)
real*8 lognHKL_1 (nr__3) ! log AGN column density,
* KL divergence (in nats units)
* (lognH_KL)
real*8 b_lognHH_2 (nr__3) ! ([cm-2]) log AGN column density,
* HDI lower limit (lognH_HLo)
real*8 B_lognHH_3 (nr__3) ! ([cm-2]) log AGN column density,
* HDI upper limit (lognH_HUp)
real*8 logPowNKL (nr__3) ! log power-law normalization,
* KL divergence (in nats units)
* (logPowNorm_KL)
real*8 b_logPowNH (nr__3) ! (ph/keV/cm2/s) log power-law normalization,
* HDI lower limit (logPowNorm_HLo)
real*8 B_logPowNH_1(nr__3) ! (ph/keV/cm2/s) log power-law normalization,
* HDI upper limit (logPowNorm_HUp)
real*8 GammaBF (nr__3) ! power-law slope, best-fit model
* (Gamma_BF)
real*8 lognHBF_1 (nr__3) ! ([cm-2]) log AGN column density,
* best-fit model (lognH_BF)
real*8 logPowNBF (nr__3) ! (ph/keV/cm2/s) log power-law normalization,
* best-fit model (logPowNorm_BF)
real*4 FluxObsBFS_1(nr__3) ! (mW/m2) Observed flux in observed 0.5-2 keV,
* best-fit model (FluxObsv_BF_s)
real*4 FluxObsMedS_3(nr__3) ! (mW/m2) Observed flux in observed 0.5-2 keV,
* posterior median (FluxObsv_Med_s)
real*4 b_FluxObsS_6(nr__3) ! (mW/m2) Observed flux in observed 0.5-2 keV,
* 1sigma lower limit (FluxObsv_Lo1_s)
real*4 B_FluxObsS_7(nr__3) ! (mW/m2) Observed flux in observed 0.5-2 keV,
* 1sigma upper limit (FluxObsv_Up1_s)
real*4 b2_FluxObsS_2(nr__3) ! (mW/m2) Observed flux in observed 0.5-2 keV,
* 2sigma lower limit (FluxObsv_Lo2_s)
real*4 B2_FluxObsS_3(nr__3) ! (mW/m2) Observed flux in observed 0.5-2 keV,
* 2sigma upper limit (FluxObsv_Up2_s)
real*4 FluxObsBFT_1(nr__3) ! (mW/m2) Observed flux in observed 2.3-5 keV,
* best-fit model (FluxObsv_BF_t)
real*4 FluxObsMedT_3(nr__3) ! (mW/m2) Observed flux in observed 2.3-5 keV,
* posterior median (FluxObsv_Med_t)
real*4 b_FluxObsT_6(nr__3) ! (mW/m2) Observed flux in observed 2.3-5 keV,
* 1sigma lower limit (FluxObsv_Lo1_t)
real*4 B_FluxObsT_7(nr__3) ! (mW/m2) Observed flux in observed 2.3-5 keV,
* 1sigma upper limit (FluxObsv_Up1_t)
real*4 b2_FluxObsT_2(nr__3) ! (mW/m2) Observed flux in observed 2.3-5 keV,
* 2sigma lower limit (FluxObsv_Lo2_t)
real*4 B2_FluxObsT_3(nr__3) ! (mW/m2) Observed flux in observed 2.3-5 keV,
* 2sigma upper limit (FluxObsv_Up2_t)
real*4 FluxcBFS (nr__3) ! (mW/m2) Absorption corrected flux in
* observed 0.5-2 keV,
* best-fit model (FluxCorr_BF_s)
real*4 FluxcMedS_1(nr__3) ! (mW/m2) Absorption corrected flux in
* observed 0.5-2 keV,
* posterior median (FluxCorr_Med_s)
real*4 b_FluxcS_2 (nr__3) ! (mW/m2) Absorption corrected flux in
* observed 0.5-2 keV,
* 1sigma lower limit (FluxCorr_Lo1_s)
real*4 B_FluxcS_3 (nr__3) ! (mW/m2) Absorption corrected flux in
* observed 0.5-2 keV,
* 1sigma upper limit (FluxCorr_Up1_s)
real*4 b2_FluxcS (nr__3) ! (mW/m2) Absorption corrected flux in
* observed 0.5-2 keV,
* 2sigma lower limit (FluxCorr_Lo2_s)
real*4 B2_FluxcS_1(nr__3) ! (mW/m2) Absorption corrected flux in
* observed 0.5-2 keV,
* 2sigma upper limit (FluxCorr_Up2_s)
real*4 FluxcBFT (nr__3) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV, best-fit model
* (FluxCorr_BF_t)
real*4 FluxcMedT_1(nr__3) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV,
* posterior median (FluxCorr_Med_t)
real*4 b_FluxcT_2 (nr__3) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV,
* 1sigma lower limit (FluxCorr_Lo1_t)
real*4 B_FluxcT_3 (nr__3) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV,
* 1sigma upper limit (FluxCorr_Up1_t)
real*4 b2_FluxcT (nr__3) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV,
* 2sigma lower limit (FluxCorr_Lo2_t)
real*4 B2_FluxcT_1(nr__3) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV,
* 2sigma upper limit (FluxCorr_Up2_t)
real*4 FluxIBFS (nr__3) ! (mW/m2) Absorption corrected flux in
* rest-frame 0.5-2 keV,
* best-fit model (FluxIntr_BF_s)
real*4 FluxIMedS_1(nr__3) ! (mW/m2) Absorption corrected flux in
* rest-frame 0.5-2 keV,
* posterior median (FluxIntr_Med_s)
real*4 b_FluxIS_2 (nr__3) ! (mW/m2) Absorption corrected flux in
* rest-frame 0.5-2keV,
* 1sigma lower limit (FluxIntr_Lo1_s)
real*4 B_FluxIS_3 (nr__3) ! (mW/m2) Absorption corrected flux in
* rest-frame 0.5-2keV,
* 1sigma upper limit (FluxIntr_Up1_s)
real*4 b2_FluxIS (nr__3) ! (mW/m2) Absorption corrected flux in
* rest-frame 0.5-2 keV,
* 2sigma lower limit (FluxIntr_Lo2_s)
real*4 B2_FluxIS_1(nr__3) ! (mW/m2) Absorption corrected flux in
* rest-frame 0.5-2 keV,
* 2sigma upper limit (FluxIntr_Up2_s)
real*4 FluxIBF2keV(nr__3) ! (mW/m2/eV) Absorption corrected flux at
* rest-frame 2keV, best- fit
* (FluxIntr_BF_2keV)
real*4 FluxIMed2keV_1(nr__3) ! (mW/m2/eV) Absorption corrected flux at
* rest-frame 2keV, median
* (FluxIntr_Med_2keV)
real*4 b_FluxI2keV_2(nr__3) ! (mW/m2/eV) Absorption corrected flux at
* rest-frame 2keV, 1sigma
* lower limit (FluxIntr_Lo1_2keV)
real*4 B_FluxI2keV_3(nr__3) ! (mW/m2/eV) Absorption corrected flux at
* rest-frame 2keV, 1sigma
* upper limit (FluxIntr_Up1_2keV)
real*4 b2_FluxI2keV(nr__3) ! (mW/m2/eV) Absorption corrected flux at
* rest-frame 2keV, 2sigma
* lower limit (FluxIntr_Lo2_2keV)
real*4 B2_FluxI2keV_1(nr__3) ! (mW/m2/eV) Absorption corrected flux at
* rest-frame 2keV, 2sigma
* upper limit (FluxIntr_Up2_2keV)
real*8 LumIBFS (nr__3) ! (10-7W) ?=-99 Intrinsic luminosity in
* rest-frame 0.5-2 keV,
* best-fit model (LumiIntr_BF_s)
real*8 LumIMedS_1 (nr__3) ! (10-7W) ?=-99 Intrinsic luminosity in
* rest-frame 0.5-2 keV,
* posterior median (LumiIntr_Med_s)
real*8 b_LumIS_2 (nr__3) ! (10-7W) ?=-99 Intrinsic luminosity in
* rest-frame 0.5-2 keV,
* 1sigma lower limit (LumiIntr_Lo1_s)
real*8 B_LumIS_3 (nr__3) ! (10-7W) ?=-99 Intrinsic luminosity in
* rest-frame 0.5-2 keV,
* 1sigma upper limit (LumiIntr_Up1_s)
real*8 b2_LumIS (nr__3) ! (10-7W) ?=-99 Intrinsic luminosity in
* rest-frame 0.5-2 keV,
* 2sigma lower limit (LumiIntr_Lo2_s)
real*8 B2_LumIS_1 (nr__3) ! (10-7W) ?=-99 Intrinsic luminosity in
* rest-frame 0.5-2 keV,
* 2sigma upper limit (LumiIntr_Up2_s)
real*8 LumIBF2keV (nr__3) ! (10-7W/eV) ?=-99 Intrinsic luminosity at
* rest-frame 2keV, best-fit model
* (LumiIntr_BF_2keV)
real*8 LumIMed2keV_1(nr__3) ! (10-7W/eV) ?=-99 Intrinsic luminosity at
* rest-frame 2keV, posterior median
* (LumiIntr_Med_2keV)
real*8 b_LumI2keV_2(nr__3) ! (10-7W/eV) ?=-99 Intrinsic luminosity at
* rest-frame 2keV, 1sigma lower limit
* (LumiIntr_Lo1_2keV)
real*8 B_LumI2keV_3(nr__3) ! (10-7W/eV) ?=-99 Intrinsic luminosity at
* rest-frame 2keV, 1sigma upper limit
* (LumiIntr_Up1_2keV)
real*8 b2_LumI2keV(nr__3) ! (10-7W/eV) ?=-99 Intrinsic luminosity at
* rest-frame 2keV, 2sigma lower limit
* (LumiIntr_Lo2_2keV)
real*8 B2_LumI2keV_1(nr__3) ! (10-7W/eV) ?=-99 Intrinsic luminosity at
* rest-frame 2keV, 2sigma upper limit
* (LumiIntr_Up2_2keV)
real*8 GammaMed (nr__3) ! power-law slope, posterior median
* (Gamma_Med)
real*8 b_Gamma (nr__3) ! power-law slope, percentile
* lower limit (Gamma_Lo)
real*8 B_Gamma_1 (nr__3) ! power-law slope, percentile
* upper limit (Gamma_Up)
real*8 GammaMean (nr__3) ! power-law slope, mean (Gamma_Mean)
real*8 s_Gamma (nr__3) ! power-law slope, standard deviation
* (Gamma_Std)
real*8 lognHMed_1 (nr__3) ! ([cm-2]) log AGN column density,
* posterior median (lognH_Med)
real*8 b_lognH_2 (nr__3) ! ([cm-2]) log AGN column density,
* percentile lower limit (lognH_Lo)
real*8 B_lognH_3 (nr__3) ! ([cm-2]) log AGN column density,
* percentile upper limit (lognH_Up)
real*8 lognHMean_1(nr__3) ! ([cm-2]) log AGN column density,
* mean (lognH_Mean)
real*8 s_lognH_1 (nr__3) ! ([cm-2]) log AGN column density,
* standard deviation (lognH_Std)
real*8 logPowNMed (nr__3) ! (ph/keV/cm2/s) log power-law normalization,
* posterior median (logPowNorm_Med)
real*8 b_logPowN (nr__3) ! (ph/keV/cm2/s) log power-law normalization,
* percentile lower limit
* (logPowNorm_Lo)
real*8 B_logPowN_1(nr__3) ! (ph/keV/cm2/s) log power-law normalization,
* percentile upper limit
* (logPowNorm_Up)
real*8 logPowNMean(nr__3) ! (ph/keV/cm2/s) log power-law normalization,
* mean (logPowNorm_Mean)
real*8 s_logPowN (nr__3) ! (ph/keV/cm2/s) log power-law normalization,
* standard deviation (logPowNorm_Std)
real*4 logBkgNMed_1(nr__3) ! log background normalization,
* posterior median (logBkgNorm_Med)
real*8 b_logBkgN_2(nr__3) ! log background normalization,
* percentile lower limit
* (logBkgNorm_Lo)
real*4 B_logBkgN_3(nr__3) ! log background normalization,
* percentile upper limit
* (logBkgNorm_Up)
real*4 logBkgNMean_1(nr__3) ! log background normalization,
* mean (logBkgNorm_Mean)
real*8 s_logBkgN_1(nr__3) ! log background normalization,
* standard deviation (logBkgNorm_Std)
real*8 chi25_1 (nr__3) ! ?=-99 Chi^2 of the best-fit model
* against the rebinned data
* (>=25 cts/bin) (chi25)
integer*4 dof25_1 (nr__3) ! ?=-99 DOF of the rebinned data,
* which has at least 25 counts per
* bin (dof25)
real*8 logZ_1 (nr__3) ! log10 Bayesian evidence (logZ)
integer*4 NHclass_1 (nr__3) ! [1/4] Class of AGN NH measurement
* with model 1 (single-powerlaw)
* (NHclass) (1)
*Note (1): Class of AGN NH measurement with model 1 (single-powerlaw)
* as follows:
* 1 = uninformative
* 2 = unobscured
* 3 = mildly-measured
* 4 = well-measured
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table5.dat' ! Double-powerlaw results
integer*4 nr__4
parameter (nr__4=27910) ! Number of records
character*1175 ar__4 ! Full-size record
integer*4 ID_SRC_4 (nr__4) ! [1/32683] ID of the sources in
* the eFEDS main X-ray catalog
* (Paper I) (ID_SRC)
real*4 z_2 (nr__4) ! [-0.01/8.0] The redshift adopted
* for the spectral model
* (Redshift)
real*8 dGmKL (nr__4) ! Soft-powerlaw slope minus
* primary-powerlaw slope,
* KL divergence (in nats units)
* (dGm_KL)
real*8 b_dGmH (nr__4) ! Soft-powerlaw slope minus
* primary-powerlaw slope,
* HDI lower limit (dGm_HLo)
real*8 B_dGmH_1 (nr__4) ! Soft-powerlaw slope minus
* primary-powerlaw slope,
* HDI upper limit (dGm_HUp)
real*8 GammaKL_1 (nr__4) ! ? power-law slope,
* KL divergence (in nats units)
* (Gamma_KL)
real*8 b_GammaH_2 (nr__4) ! power-law slope, HDI lower limit
* (Gamma_HLo)
real*8 B_GammaH_3 (nr__4) ! power-law slope, HDI upper limit
* (Gamma_HUp)
real*8 lognHKL_2 (nr__4) ! log AGN column density,
* KL divergence (in nats units)
* (lognH_KL)
real*8 b_lognHH_4 (nr__4) ! ([cm-2]) log AGN column density,
* HDI lower limit (lognH_HLo)
real*8 B_lognHH_5 (nr__4) ! ([cm-2]) log AGN column density,
* HDI upper limit (lognH_HUp)
real*8 logPowNKL_1(nr__4) ! log power-law normalization,
* KL divergence (in nats units)
* (logPowNorm_KL)
real*8 b_logPowNH_2(nr__4) ! ([ph/keV/cm2/s]) log power-law normalization,
* HDI lower limit
* (logPowNorm_HLo)
real*8 B_logPowNH_3(nr__4) ! ([ph/keV/cm2/s]) log power-law normalization,
* HDI upper limit
* (logPowNorm_HUp)
real*8 logFracKL (nr__4) ! ? Constant factor multiplied to
* the soft power-law,
* KL divergence (in nats units)
* (logFrac_KL)
real*8 b_logFracH (nr__4) ! Constant factor multiplied to
* the soft power-law,
* HDI lower limit (logFrac_HLo)
real*4 B_logFracH_1(nr__4) ! Constant factor multiplied to
* the soft power-law,
* HDI upper limit (logFrac_HUp)
real*8 dGmBF (nr__4) ! Soft-powerlaw slope minus
* primary-powerlaw slope,
* best-fit model (dGm_BF)
real*8 GammaBF_1 (nr__4) ! power-law slope, best-fit model
* (Gamma_BF)
real*8 lognHBF_2 (nr__4) ! ([cm-2]) log AGN column density,
* best-fit model (lognH_BF)
real*8 logPowNBF_1(nr__4) ! ([ph/keV/cm2/s]) log power-law normalization,
* best-fit model (logPowNorm_BF)
real*4 logFracBF (nr__4) ! Constant factor multiplied to
* the soft power-law, best-fit
* model (logFrac_BF)
real*4 FluxObsBFS_2(nr__4) ! (mW/m2) Observed flux in observed
* 0.5-2 keV, best-fit model
* (FluxObsv_BF_s)
real*4 FluxObsMedS_4(nr__4) ! (mW/m2) Observed flux in observed
* 0.5-2 keV, posterior median
* (FluxObsv_Med_s)
real*4 b_FluxObsS_8(nr__4) ! (mW/m2) Observed flux in observed
* 0.5-2 keV, 1sigma lower limit
* (FluxObsv_Lo1_s)
real*4 B_FluxObsS_9(nr__4) ! (mW/m2) Observed flux in observed
* 0.5-2 keV, 1sigma upper limit
* (FluxObsv_Up1_s)
real*4 b2_FluxObsS_4(nr__4) ! (mW/m2) Observed flux in observed
* 0.5-2 keV, 2sigma lower limit
* (FluxObsv_Lo2_s)
real*4 B2_FluxObsS_5(nr__4) ! (mW/m2) Observed flux in observed
* 0.5-2 keV, 2sigma upper limit
* (FluxObsv_Up2_s)
real*4 FluxObsBFT_2(nr__4) ! (mW/m2) Observed flux in observed
* 2.3-5 keV, best-fit model
* (FluxObsv_BF_t)
real*4 FluxObsMedT_4(nr__4) ! (mW/m2) Observed flux in observed
* 2.3-5 keV, posterior median
* (FluxObsv_Med_t)
real*4 b_FluxObsT_8(nr__4) ! (mW/m2) Observed flux in observed
* 2.3-5 keV, 1sigma lower limit
* (FluxObsv_Lo1_t)
real*4 B_FluxObsT_9(nr__4) ! (mW/m2) Observed flux in observed
* 2.3-5 keV, 1sigma upper limit
* (FluxObsv_Up1_t)
real*4 b2_FluxObsT_4(nr__4) ! (mW/m2) Observed flux in observed
* 2.3-5 keV, 2sigma lower limit
* (FluxObsv_Lo2_t)
real*4 B2_FluxObsT_5(nr__4) ! (mW/m2) Observed flux in observed
* 2.3-5 keV, 2sigma upper limit
* (FluxObsv_Up2_t)
real*4 FluxCBFS_1 (nr__4) ! (mW/m2) Absorption corrected flux in
* observed 0.5-2 keV,
* best-fit model (FluxCorr_BF_s)
real*4 FluxCMedS_2(nr__4) ! (mW/m2) Absorption corrected flux in
* observed 0.5-2 keV, posterior
* median (FluxCorr_Med_s)
real*4 b_FluxCS_4 (nr__4) ! (mW/m2) Absorption corrected flux in
* observed 0.5-2 keV, 1sigma
* lower limit (FluxCorr_Lo1_s)
real*4 B_FluxCS_5 (nr__4) ! (mW/m2) Absorption corrected flux in
* observed 0.5-2 keV, 1sigma
* upper limit (FluxCorr_Up1_s)
real*4 b2_FluxCS_2(nr__4) ! (mW/m2) Absorption corrected flux in
* observed 0.5-2 keV, 2sigma
* lower limit (FluxCorr_Lo2_s)
real*4 B2_FluxCS_3(nr__4) ! (mW/m2) Absorption corrected flux in
* observed 0.5-2 keV, 2sigma
* upper limit (FluxCorr_Up2_s)
real*4 FluxCBFT_1 (nr__4) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV,
* best-fit model (FluxCorr_BF_t)
real*4 FluxCMedT_2(nr__4) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV, posterior
* median (FluxCorr_Med_t)
real*4 b_FluxCT_4 (nr__4) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV, 1sigma
* lower limit (FluxCorr_Lo1_t)
real*4 B_FluxCT_5 (nr__4) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV, 1sigma
* upper limit (FluxCorr_Up1_t)
real*4 b2_FluxCT_2(nr__4) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV, 2sigma
* lower limit (FluxCorr_Lo2_t)
real*4 B2_FluxCT_3(nr__4) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV, 2sigma
* upper limit (FluxCorr_Up2_t)
real*4 FluxIBFS_1 (nr__4) ! (mW/m2) Absorption corrected flux in
* rest-frame 0.5-2 keV,
* best-fit model (FluxIntr_BF_s)
real*4 FluxIMedS_2(nr__4) ! (mW/m2) Absorption corrected flux in
* rest-frame 0.5-2 keV,
* posterior median
* (FluxIntr_Med_s)
real*4 b_FluxIS_4 (nr__4) ! (mW/m2) Absorption corrected flux in
* rest-frame 0.5-2keV, 1sigma
* lower limit (FluxIntr_Lo1_s)
real*4 B_FluxIS_5 (nr__4) ! (mW/m2) Absorption corrected flux in
* rest-frame 0.5-2keV, 1sigma
* upper limit (FluxIntr_Up1_s)
real*4 b2_FluxIS_2(nr__4) ! (mW/m2) Absorption corrected flux in
* rest-frame 0.5-2 keV, 2sigma
* lower limit (FluxIntr_Lo2_s)
real*4 B2_FluxIS_3(nr__4) ! (mW/m2) Absorption corrected flux in
* rest-frame 0.5-2 keV, 2sigma
* upper limit (FluxIntr_Up2_s)
real*4 FluxIBF2keV_1(nr__4) ! (mW/m2/eV) Absorption corrected flux at
* rest-frame 2keV, best-fit
* (FluxIntr_BF_2keV)
real*4 FluxIMed2keV_2(nr__4) ! (mW/m2/eV) Absorption corrected flux at
* rest-frame 2keV, median
* (FluxIntr_Med_2keV)
real*4 b_FluxI2keV_4(nr__4) ! (mW/m2/eV) Absorption corrected flux at
* rest-frame 2keV, 1sigma
* lower limit (FluxIntr_Lo1_2keV)
real*4 B_FluxI2keV_5(nr__4) ! (mW/m2/eV) Absorption corrected flux at
* rest-frame 2keV, 1sigma
* upper limit (FluxIntr_Up1_2keV)
real*4 b2_FluxI2keV_2(nr__4) ! (mW/m2/eV) Absorption corrected flux at
* rest-frame 2keV, 2sigma
* lower limit (FluxIntr_Lo2_2keV)
real*4 B2_FluxI2keV_3(nr__4) ! (mW/m2/eV) Absorption corrected flux at
* rest-frame 2keV, 2sigma
* upper limit (FluxIntr_Up2_2keV)
real*8 LumIBFS_1 (nr__4) ! (10-7W) ?=-99 Intrinsic luminosity in
* rest-frame 0.5-2 keV,
* best-fit model (LumiIntr_BF_s)
real*8 LumIMedS_2 (nr__4) ! (10-7W) ?=-99 Intrinsic luminosity in
* rest-frame 0.5-2 keV, posterior
* median (LumiIntr_Med_s)
real*8 b_LumIS_4 (nr__4) ! (10-7W) ?=-99 Intrinsic luminosity in
* rest-frame 0.5-2 keV,
* 1sigma lower limit
* (LumiIntr_Lo1_s)
real*8 B_LumIS_5 (nr__4) ! (10-7W) ?=-99 Intrinsic luminosity in
* rest-frame 0.5-2 keV,
* 1sigma upper limit
* (LumiIntr_Up1_s)
real*8 b2_LumIS_2 (nr__4) ! (10-7W) ?=-99 Intrinsic luminosity in
* rest-frame 0.5-2 keV,
* 2sigma lower limit
* (LumiIntr_Lo2_s)
real*8 B2_LumIS_3 (nr__4) ! (10-7W) ?=-99 Intrinsic luminosity in
* rest-frame 0.5-2 keV,
* 2sigma upper limit
* (LumiIntr_Up2_s)
real*8 LumIBF2keV_1(nr__4) ! (10-7W/eV) ?=-99 Intrinsic luminosity at
* rest-frame 2keV, best-fit
* model (LumiIntr_BF_2keV)
real*8 LumIMed2keV_2(nr__4) ! (10-7W/eV) ?=-99 Intrinsic luminosity at
* rest-frame 2keV, posterior
* median (LumiIntr_Med_2keV)
real*8 b_LumI2keV_4(nr__4) ! (10-7W/eV) ?=-99 Intrinsic luminosity at
* rest-frame 2keV, 1sigma
* lower limit (LumiIntr_Lo1_2keV)
real*8 B_LumI2keV_5(nr__4) ! (10-7W/eV) ?=-99 Intrinsic luminosity at
* rest-frame 2keV, 1sigma
* upper limit (LumiIntr_Up1_2keV)
real*8 b2_LumI2keV_2(nr__4) ! (10-7W/eV) ?=-99 Intrinsic luminosity at
* rest-frame 2keV, 2sigma
* lower limit (LumiIntr_Lo2_2keV)
real*8 B2_LumI2keV_3(nr__4) ! (10-7W/eV) ?=-99 Intrinsic luminosity at
* rest-frame 2keV, 2sigma
* upper limit (LumiIntr_Up2_2keV)
real*8 dGmMed (nr__4) ! Soft-powerlaw slope minus
* primary-powerlaw slope,
* posterior median (dGm_Med)
real*8 b_dGm (nr__4) ! Soft-powerlaw slope minus
* primary-powerlaw slope,
* 1sigma lower limit (dGm_Lo)
real*8 B_dGm_1 (nr__4) ! Soft-powerlaw slope minus
* primary-powerlaw slope,
* 1sigma upper limit (dGm_Up)
real*8 dGmMean (nr__4) ! Soft-powerlaw slope minus
* primary-powerlaw slope,
* mean (dGm_Mean)
real*8 s_dGm (nr__4) ! Soft-powerlaw slope minus
* primary-powerlaw slope,
* standard deviation (dGm_Std)
real*8 GammaMed_1 (nr__4) ! power-law slope, posterior
* median (Gamma_Med)
real*8 b_Gamma_2 (nr__4) ! power-law slope, percentile
* lower limit (Gamma_Lo)
real*8 B_Gamma_3 (nr__4) ! power-law slope, percentile
* upper limit (Gamma_Up)
real*8 GammaMean_1(nr__4) ! power-law slope, mean
* (Gamma_Mean)
real*4 s_Gamma_1 (nr__4) ! power-law slope,
* standard deviation (Gamma_Std)
real*8 lognHMed_2 (nr__4) ! ([cm-2]) log AGN column density,
* posterior median (lognH_Med)
real*8 b_lognH_4 (nr__4) ! ([cm-2]) log AGN column density,
* percentile lower limit
* (lognH_Lo)
real*8 B_lognH_5 (nr__4) ! ([cm-2]) log AGN column density,
* percentile upper limit
* (lognH_Up)
real*8 lognHMean_2(nr__4) ! ([cm-2]) log AGN column density,
* mean (lognH_Mean)
real*8 s_lognH_2 (nr__4) ! ([cm-2]) log AGN column density,
* standard deviation (lognH_Std)
real*8 logPowNMed_1(nr__4) ! ([ph/keV/cm2/s]) log power-law normalization,
* posterior median
* (logPowNorm_Med)
real*8 b_logPowN_2(nr__4) ! ([ph/keV/cm2/s]) log power-law normalization,
* percentile lower limit
* (logPowNorm_Lo)
real*8 B_logPowN_3(nr__4) ! ([ph/keV/cm2/s]) log power-law normalization,
* percentile upper limit
* (logPowNorm_Up)
real*8 logPowNMean_1(nr__4) ! ([ph/keV/cm2/s]) log power-law normalization,
* mean (logPowNorm_Mean)
real*8 s_logPowN_1(nr__4) ! ([ph/keV/cm2/s]) log power-law normalization,
* standard deviation
* (logPowNorm_Std)
real*8 logFracMed (nr__4) ! Constant factor multiplied to
* the soft power-law,
* posterior median (logFrac_Med)
real*8 b_logFrac (nr__4) ! Constant factor multiplied to
* the soft power-law,
* 1sigma lower limit (logFrac_Lo)
real*8 B_logFrac_1(nr__4) ! Constant factor multiplied to
* the soft power-law,
* 1sigma upper limit (logFrac_Up)
real*8 logFracMean(nr__4) ! Constant factor multiplied to
* the soft power-law,
* mean (logFrac_Mean)
real*8 s_logFrac (nr__4) ! Constant factor multiplied to
* the soft power-law,
* standard deviation
* (logFrac_Std)
real*4 logBkgNMed_2(nr__4) ! log background normalization,
* posterior median
* (logBkgNorm_Med)
real*8 b_logBkgN_4(nr__4) ! log background normalization,
* percentile lower limit
* (logBkgNorm_Lo)
real*4 B_logBkgN_5(nr__4) ! log background normalization,
* percentile upper limit
* (logBkgNorm_Up)
real*4 logBkgNMean_2(nr__4) ! log background normalization,
* mean (logBkgNorm_Mean)
real*8 s_logBkgN_2(nr__4) ! log background normalization,
* standard deviation
* (logBkgNorm_Std)
real*8 chi25_2 (nr__4) ! ?=-99 Chi^2 of the best-fit
* model against the rebinned
* data (>=25 cts/bin) (chi25)
integer*4 dof25_2 (nr__4) ! ?=-99 DOF of the rebinned data,
* which has at least 25 counts
* per bin (dof25)
real*8 logZ_2 (nr__4) ! log10 Bayesian evidence (logZ)
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table6.dat' ! Powerlaw+blackbody results
integer*4 nr__5
parameter (nr__5=27910) ! Number of records
character*1217 ar__5 ! Full-size record
integer*4 ID_SRC_5 (nr__5) ! [1/32683] ID of the sources in
* the eFEDS main X-ray catalog
* (Paper I) (ID_SRC)
real*4 z_3 (nr__5) ! [-0.01/8.0] The redshift adopted
* for the spectral model
* (Redshift)
real*8 GammaKL_2 (nr__5) ! power-law slope, KL divergence
* (in nats units) (Gamma_KL)
real*8 b_GammaH_4 (nr__5) ! power-law slope, HDI lower limit
* (Gamma_HLo)
real*8 B_GammaH_5 (nr__5) ! power-law slope, HDI upper limit
* (Gamma_HUp)
real*8 lognHKL_3 (nr__5) ! log AGN column density,
* KL divergence (in nats units)
* (lognH_KL)
real*8 b_lognHH_6 (nr__5) ! ([cm-2]) log AGN column density,
* HDI lower limit (lognH_HLo)
real*8 B_lognHH_7 (nr__5) ! ([cm-2]) log AGN column density,
* HDI upper limit (lognH_HUp)
real*8 logPowNKL_2(nr__5) ! log power-law normalization,
* KL divergence (in nats units)
* (logPowNorm_KL)
real*8 b_logPowNH_4(nr__5) ! ([ph/keV/cm2/s]) log power-law normalization,
* HDI lower limit
* (logPowNorm_HLo)
real*8 B_logPowNH_5(nr__5) ! ([ph/keV/cm2/s]) log power-law normalization,
* HDI upper limit (logPowNorm_HUp)
real*8 logkTKL_1 (nr__5) ! log temperature,
* KL divergence (in nats units)
* (logkT_KL)
real*8 b_logkTH_2 (nr__5) ! ([keV]) log temperature, HDI lower limit
* (logkT_HLo)
real*8 B_logkTH_3 (nr__5) ! ([keV]) log temperature, HDI upper limit
* (logkT_HUp)
real*8 logBBNKL (nr__5) ! log blackbody normalization,
* KL divergence (in nats units)
* (logBBNorm_KL)
real*8 b_logBBNH (nr__5) ! ([10+24W/pc2]) log blackbody normalization in
* 10^+31^erg/pc^2^, HDI
* lower limit (logBBNorm_HLo)
real*8 B_logBBNH_1(nr__5) ! ([10+24W/pc2]) log blackbody normalization in
* 10^+31^erg/pc^2^, HDI
* upper limit (logBBNorm_HUp)
real*8 GammaBF_2 (nr__5) ! power-law slope, best-fit model
* (Gamma_BF)
real*8 lognHBF_3 (nr__5) ! ([cm-2]) log AGN column density,
* best-fit model (lognH_BF)
real*8 logPowNBF_2(nr__5) ! ([ph/keV/cm2/s]) log power- law normalization,
* best-fit model (logPowNorm_BF)
real*8 logkTBF_1 (nr__5) ! ([keV]) log temperature, best- fit model
* (logkT_BF)
real*8 logBBNBF (nr__5) ! ([10+24W/pc2]) log blackbody normalization in
* 10^+31^erg/pc^2^, best-fit
* model (logBBNorm_BF)
real*4 FluxObsBFS_3(nr__5) ! (mW/m2) Observed flux in observed
* 0.5-2 keV, best-fit model
* (FluxObsv_BF_s)
real*4 FluxObsMedS_5(nr__5) ! (mW/m2) Observed flux in observed
* 0.5-2 keV, posterior median
* (FluxObsv_Med_s)
real*4 b_FluxObsS_10(nr__5) ! (mW/m2) Observed flux in observed
* 0.5-2 keV, 1sigma lower limit
* (FluxObsv_Lo1_s)
real*4 B_FluxObsS_11(nr__5) ! (mW/m2) Observed flux in observed
* 0.5-2 keV, 1sigma upper limit
* (FluxObsv_Up1_s)
real*4 b2_FluxObsS_6(nr__5) ! (mW/m2) Observed flux in observed
* 0.5-2 keV, 2sigma lower limit
* (FluxObsv_Lo2_s)
real*4 B2_FluxObsS_7(nr__5) ! (mW/m2) Observed flux in observed
* 0.5-2 keV, 2sigma upper limit
* (FluxObsv_Up2_s)
real*4 FluxObsBFT_3(nr__5) ! (mW/m2) Observed flux in observed
* 2.3-5 keV, best-fit model
* (FluxObsv_BF_t)
real*4 FluxObsMedT_5(nr__5) ! (mW/m2) Observed flux in observed
* 2.3-5 keV, posterior median
* (FluxObsv_Med_t)
real*4 b_FluxObsT_10(nr__5) ! (mW/m2) Observed flux in observed
* 2.3-5 keV, 1sigma lower limit
* (FluxObsv_Lo1_t)
real*4 B_FluxObsT_11(nr__5) ! (mW/m2) Observed flux in observed
* 2.3-5 keV, 1sigma upper limit
* (FluxObsv_Up1_t)
real*4 b2_FluxObsT_6(nr__5) ! (mW/m2) Observed flux in observed
* 2.3-5 keV, 2sigma lower limit
* (FluxObsv_Lo2_t)
real*4 B2_FluxObsT_7(nr__5) ! (mW/m2) Observed flux in observed
* 2.3-5 keV, 2sigma upper limit
* (FluxObsv_Up2_t)
real*4 FluxCBFS_2 (nr__5) ! (mW/m2) Absorption corrected flux in
* observed 0.5-2 keV, best-fit
* model (FluxCorr_BF_s)
real*4 FluxCMedS_3(nr__5) ! (mW/m2) Absorption corrected flux in
* observed 0.5-2 keV, posterior
* median (FluxCorr_Med_s)
real*4 b_FluxCS_6 (nr__5) ! (mW/m2) Absorption corrected flux in
* observed 0.5-2 keV, 1sigma
* lower limit (FluxCorr_Lo1_s)
real*4 B_FluxCS_7 (nr__5) ! (mW/m2) Absorption corrected flux in
* observed 0.5-2 keV, 1sigma
* upper limit (FluxCorr_Up1_s)
real*4 b2_FluxCS_4(nr__5) ! (mW/m2) Absorption corrected flux in
* observed 0.5-2 keV, 2sigma
* lower limit (FluxCorr_Lo2_s)
real*4 B2_FluxCS_5(nr__5) ! (mW/m2) Absorption corrected flux in
* observed 0.5-2 keV, 2sigma
* upper limit (FluxCorr_Up2_s)
real*4 FluxCBFT_2 (nr__5) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV, best-fit
* model (FluxCorr_BF_t)
real*4 FluxCMedT_3(nr__5) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV, posterior
* median (FluxCorr_Med_t)
real*4 b_FluxCT_6 (nr__5) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV, 1sigma
* lower limit (FluxCorr_Lo1_t)
real*4 B_FluxCT_7 (nr__5) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV, 1sigma
* upper limit (FluxCorr_Up1_t)
real*4 b2_FluxCT_4(nr__5) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV, 2sigma
* lower limit (FluxCorr_Lo2_t)
real*4 B2_FluxCT_5(nr__5) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV, 2sigma
* upper limit (FluxCorr_Up2_t)
real*4 FluxIBFS_2 (nr__5) ! (mW/m2) Absorption corrected flux in
* rest-frame 0.5-2 keV,
* best-fit model (FluxIntr_BF_s)
real*4 FluxIMedS_3(nr__5) ! (mW/m2) Absorption corrected flux in
* rest-frame 0.5-2 keV, posterior
* median (FluxIntr_Med_s)
real*4 b_FluxIS_6 (nr__5) ! (mW/m2) Absorption corrected flux in
* rest-frame 0.5-2keV, 1sigma
* lower limit (FluxIntr_Lo1_s)
real*4 B_FluxIS_7 (nr__5) ! (mW/m2) Absorption corrected flux in
* rest-frame 0.5-2keV, 1sigma
* upper limit (FluxIntr_Up1_s)
real*4 b2_FluxIS_4(nr__5) ! (mW/m2) Absorption corrected flux in
* rest-frame 0.5-2 keV, 2sigma
* lower limit (FluxIntr_Lo2_s)
real*4 B2_FluxIS_5(nr__5) ! (mW/m2) Absorption corrected flux in
* rest-frame 0.5-2 keV, 2sigma
* upper limit (FluxIntr_Up2_s)
real*4 FluxIBF2keV_2(nr__5) ! (mW/m2/eV) Absorption corrected flux at
* rest-frame 2keV, best-fit
* (FluxIntr_BF_2keV)
real*4 FluxIMed2keV_3(nr__5) ! (mW/m2/eV) Absorption corrected flux at
* rest-frame 2keV, median
* (FluxIntr_Med_2keV)
real*4 b_FluxI2keV_6(nr__5) ! (mW/m2/eV) Absorption corrected flux at
* rest-frame 2keV, 1sigma
* lower limit (FluxIntr_Lo1_2keV)
real*4 B_FluxI2keV_7(nr__5) ! (mW/m2/eV) Absorption corrected flux at
* rest-frame 2keV, 1sigma
* upper limit (FluxIntr_Up1_2keV)
real*4 b2_FluxI2keV_4(nr__5) ! (mW/m2/eV) Absorption corrected flux at
* rest-frame 2keV, 2sigma
* lower limit (FluxIntr_Lo2_2keV)
real*4 B2_FluxI2keV_5(nr__5) ! (mW/m2/eV) Absorption corrected flux at
* rest-frame 2keV, 2sigma
* upper limit (FluxIntr_Up2_2keV)
real*8 LumIBFS_2 (nr__5) ! (10-7W) ?=-99 Intrinsic luminosity in
* rest-frame 0.5-2 keV, best-fit
* model (LumiIntr_BF_s)
real*8 LumIMedS_3 (nr__5) ! (10-7W) ?=-99 Intrinsic luminosity in
* rest-frame 0.5-2 keV, posterior
* median (LumiIntr_Med_s)
real*8 b_LumIS_6 (nr__5) ! (10-7W) ?=-99 Intrinsic luminosity in
* rest-frame 0.5-2 keV, 1sigma
* lower limit (LumiIntr_Lo1_s)
real*8 B_LumIS_7 (nr__5) ! (10-7W) ?=-99 Intrinsic luminosity in
* rest-frame 0.5-2 keV, 1sigma
* upper limit (LumiIntr_Up1_s)
real*8 b2_LumIS_4 (nr__5) ! (10-7W) ?=-99 Intrinsic luminosity in
* rest-frame 0.5-2 keV, 2sigma
* lower limit (LumiIntr_Lo2_s)
real*8 B2_LumIS_5 (nr__5) ! (10-7W) ?=-99 Intrinsic luminosity in
* rest-frame 0.5-2 keV, 2sigma
* upper limit (LumiIntr_Up2_s)
real*8 LumIBF2keV_2(nr__5) ! (10-7W/eV) ?=-99 Intrinsic luminosity at
* rest-frame 2keV, best-fit
* model (LumiIntr_BF_2keV)
real*8 LumIMed2keV_3(nr__5) ! (10-7W/eV) ?=-99 Intrinsic luminosity at
* rest-frame 2keV, posterior
* median (LumiIntr_Med_2keV)
real*8 b_LumI2keV_6(nr__5) ! (10-7W/eV) ?=-99 Intrinsic luminosity at
* rest-frame 2keV, 1sigma
* lower limit (LumiIntr_Lo1_2keV)
real*8 B_LumI2keV_7(nr__5) ! (10-7W/eV) ?=-99 Intrinsic luminosity at
* rest-frame 2keV, 1sigma
* upper limit (LumiIntr_Up1_2keV)
real*8 b2_LumI2keV_4(nr__5) ! (10-7W/eV) ?=-99 Intrinsic luminosity at
* rest-frame 2keV, 2sigma
* lower limit (LumiIntr_Lo2_2keV)
real*8 B2_LumI2keV_5(nr__5) ! (10-7W/eV) ?=-99 Intrinsic luminosity at
* rest-frame 2keV, 2sigma
* upper limit (LumiIntr_Up2_2keV)
real*8 GammaMed_2 (nr__5) ! power-law slope, posterior
* median (Gamma_Med)
real*8 b_Gamma_4 (nr__5) ! power-law slope, percentile
* lower limit (Gamma_Lo)
real*8 B_Gamma_5 (nr__5) ! power-law slope, percentile
* upper limit (Gamma_Up)
real*8 GammaMean_2(nr__5) ! power-law slope, mean
* (Gamma_Mean)
real*8 s_Gamma_2 (nr__5) ! power-law slope,
* standard deviation (Gamma_Std)
real*8 lognHMed_3 (nr__5) ! ([cm-2]) log AGN column density,
* posterior median (lognH_Med)
real*8 b_lognH_6 (nr__5) ! ([cm-2]) log AGN column density,
* percentile lower limit
* (lognH_Lo)
real*8 B_lognH_7 (nr__5) ! ([cm-2]) log AGN column density,
* percentile upper limit
* (lognH_Up)
real*8 lognHMean_3(nr__5) ! ([cm-2]) log AGN column density,
* mean (lognH_Mean)
real*8 s_lognH_3 (nr__5) ! ([cm-2]) log AGN column density,
* standard deviation (lognH_Std)
real*8 logPowNMed_2(nr__5) ! ([ph/keV/cm2/s]) log power-law normalization,
* posterior median
* (logPowNorm_Med)
real*8 b_logPowN_4(nr__5) ! ([ph/keV/cm2/s]) log power-law normalization,
* percentile lower limit
* (logPowNorm_Lo)
real*8 B_logPowN_5(nr__5) ! ([ph/keV/cm2/s]) log power-law normalization,
* percentile upper limit
* (logPowNorm_Up)
real*8 logPowNMean_2(nr__5) ! ([ph/keV/cm2/s]) log power-law normalization,
* mean (logPowNorm_Mean)
real*8 s_logPowN_2(nr__5) ! ([ph/keV/cm2/s]) log power-law normalization,
* standard deviation
* (logPowNorm_Std)
real*8 logkTMed_1 (nr__5) ! ([keV]) log temperature, posterior
* median (logkT_Med)
real*8 b_logkT_2 (nr__5) ! ([keV]) log temperature, percentile
* lower limit (logkT_Lo)
real*8 B_logkT_3 (nr__5) ! ([keV]) log temperature, percentile
* upper limit (logkT_Up)
real*8 logkTMean_1(nr__5) ! ([keV]) log temperature, mean
* (logkT_Mean)
real*8 s_logkT_1 (nr__5) ! ([keV]) log temperature, standard
* deviation (logkT_Std)
real*8 logBBNMed (nr__5) ! ([10+24W/pc2]) log blackbody normalization in
* 10^+31^erg/s/pc^2^, posterior
* median (logBBNorm_Med)
real*8 b_logBBN (nr__5) ! ([10+24W/pc2]) log blackbody normalization in
* 10^+31^erg/s/pc^2^, percentile
* lower limit (logBBNorm_Lo)
real*8 B_logBBN_1 (nr__5) ! ([10+24W/pc2]) log blackbody normalization in
* 10^+31^erg/s/pc^2^, percentile
* upper limit (logBBNorm_Up)
real*8 logBBNMean (nr__5) ! ([10+24W/pc2]) log blackbody normalization in
* 10^+31^erg/s/pc^2^,
* mean (logBBNorm_Mean)
real*8 s_logBBN (nr__5) ! ([10+24W/pc2]) log blackbody normalization in
* 10^+31^erg/s/pc^2^, standard
* deviation (logBBNorm_Std)
real*4 logBkgNMed_3(nr__5) ! log background normalization,
* posterior median
* (logBkgNorm_Med)
real*8 b_logBkgN_6(nr__5) ! log background normalization,
* percentile lower limit
* (logBkgNorm_Lo)
real*4 B_logBkgN_7(nr__5) ! log background normalization,
* percentile upper limit
* (logBkgNorm_Up)
real*4 logBkgNMean_3(nr__5) ! log background normalization,
* mean (logBkgNorm_Mean)
real*8 s_logBkgN_3(nr__5) ! log background normalization,
* standard deviation
* (logBkgNorm_Std)
real*8 chi25_3 (nr__5) ! ?=-99 Chi^2 of the best-fit
* model against the rebinned
* data (>=25 cts/bin) (chi25)
integer*4 dof25_3 (nr__5) ! ?=-99 DOF of the rebinned data,
* which has at least
* 25 counts per bin (dof25)
real*8 logZ_3 (nr__5) ! log10 Bayesian evidence (logZ)
real*8 logRbb (nr__5) ! log blackbody relative strength
* at 1keV (logRbb)
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table7.dat' ! Gamma-fixed-powerlaw results
integer*4 nr__6
parameter (nr__6=27910) ! Number of records
character*841 ar__6 ! Full-size record
integer*4 ID_SRC_6 (nr__6) ! [1/32683] ID of the sources in the
* eFEDS main X-ray catalog
* (Paper I) (ID_SRC)
real*4 z_4 (nr__6) ! [-0.01/8.0] The redshift adopted
* for the spectral model (Redshift)
real*8 lognHKL_4 (nr__6) ! log AGN column density,
* KL divergence (in nats units)
* (lognH_KL)
real*8 b_lognHH_8 (nr__6) ! ([cm-2]) log AGN column density,
* HDI lower limit (lognH_HLo)
real*8 B_lognHH_9 (nr__6) ! ([cm-2]) log AGN column density,
* HDI upper limit (lognH_HUp)
real*8 logPowNKL_3(nr__6) ! log power-law normalization,
* KL divergence (in nats units)
* (logPowNorm_KL)
real*8 b_logPowNH_6(nr__6) ! ([ph/keV/cm2/s]) log power-law normalization,
* HDI lower limit (logPowNorm_HLo)
real*8 B_logPowNH_7(nr__6) ! ([ph/keV/cm2/s]) log power-law normalization,
* HDI upper limit (logPowNorm_HUp)
real*8 lognHBF_4 (nr__6) ! ([cm-2]) log AGN column density,
* best-fit model (lognH_BF)
real*8 logPowNBF_3(nr__6) ! ([ph/keV/cm2/s]) log power-law normalization,
* best-fit model (logPowNorm_BF)
real*4 FluxObsBFS_4(nr__6) ! (mW/m2) Observed flux in observed
* 0.5-2 keV, best-fit model
* (FluxObsv_BF_s)
real*4 FluxObsMedS_6(nr__6) ! (mW/m2) Observed flux in observed
* 0.5-2 keV, posterior median
* (FluxObsv_Med_s)
real*4 b_FluxObsS_12(nr__6) ! (mW/m2) Observed flux in observed
* 0.5-2 keV, 1sigma lower limit
* (FluxObsv_Lo1_s)
real*4 B_FluxObsS_13(nr__6) ! (mW/m2) Observed flux in observed
* 0.5-2 keV, 1sigma upper limit
* (FluxObsv_Up1_s)
real*4 b2_FluxObsS_8(nr__6) ! (mW/m2) Observed flux in observed
* 0.5-2 keV, 2sigma lower limit
* (FluxObsv_Lo2_s)
real*4 B2_FluxObsS_9(nr__6) ! (mW/m2) Observed flux in observed
* 0.5-2 keV, 2sigma upper limit
* (FluxObsv_Up2_s)
real*4 FluxObsBFT_4(nr__6) ! (mW/m2) Observed flux in observed
* 2.3-5 keV, best-fit model
* (FluxObsv_BF_t)
real*4 FluxObsMedT_6(nr__6) ! (mW/m2) Observed flux in observed
* 2.3-5 keV, posterior median
* (FluxObsv_Med_t)
real*4 b_FluxObsT_12(nr__6) ! (mW/m2) Observed flux in observed
* 2.3-5 keV, 1sigma lower limit
* (FluxObsv_Lo1)
real*4 B_FluxObsT_13(nr__6) ! (mW/m2) Observed flux in observed
* 2.3-5 keV, 1sigma upper limit
* (FluxObsv_Up1)
real*4 b2_FluxObsT_8(nr__6) ! (mW/m2) Observed flux in observed
* 2.3-5 keV, 2sigma lower limit
* (FluxObsv_Lo2)
real*4 B2_FluxObsT_9(nr__6) ! (mW/m2) Observed flux in observed
* 2.3-5 keV, 2sigma upper limit
* (FluxObsv_Up2)
real*4 FluxCBFS_3 (nr__6) ! (mW/m2) Absorption corrected flux in
* observed 0.5-2 keV, best-fit
* model (FluxCorr_BF_s)
real*4 FluxCMedS_4(nr__6) ! (mW/m2) Absorption corrected flux in
* observed 0.5-2 keV, posterior
* median (FluxCorr_Med_s)
real*4 b_FluxCS_8 (nr__6) ! (mW/m2) Absorption corrected flux in
* observed 0.5-2 keV, 1sigma
* lower limit (FluxCorr_Lo1_s)
real*4 B_FluxCS_9 (nr__6) ! (mW/m2) Absorption corrected flux in
* observed 0.5-2 keV, 1sigma
* upper limit (FluxCorr_Up1_s)
real*4 b2_FluxCS_6(nr__6) ! (mW/m2) Absorption corrected flux in
* observed 0.5-2 keV, 2sigma
* lower limit (FluxCorr_Lo2_s)
real*4 B2_FluxCS_7(nr__6) ! (mW/m2) Absorption corrected flux in
* observed 0.5-2 keV, 2sigma
* upper limit (FluxCorr_Up2_s)
real*4 FluxCBFT_3 (nr__6) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV, best-fit
* model (FluxCorr_BF_t)
real*4 FluxCMedT_4(nr__6) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV, posterior
* median (FluxCorr_Med_t)
real*4 b_FluxCT_8 (nr__6) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV, 1sigma
* lower limit (FluxCorr_Lo1)
real*4 B_FluxCT_9 (nr__6) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV, 1sigma
* upper limit (FluxCorr_Up1)
real*4 b2_FluxCT_6(nr__6) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV, 2sigma
* lower limit (FluxCorr_Lo2)
real*4 B2_FluxCT_7(nr__6) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV, 2sigma
* upper limit (FluxCorr_Up2)
real*4 FluxIBFS_3 (nr__6) ! (mW/m2) Absorption corrected flux in
* rest-frame 0.5-2 keV, best-fit
* model (FluxIntr_BF_s)
real*4 FluxIMedS_4(nr__6) ! (mW/m2) Absorption corrected flux in
* rest-frame 0.5-2 keV, posterior
* median (FluxIntr_Med_s)
real*4 b_FluxIS_8 (nr__6) ! (mW/m2) Absorption corrected flux in
* rest-frame 0.5-2keV, 1sigma
* lower limit (FluxIntr_Lo1_s)
real*4 B_FluxIS_9 (nr__6) ! (mW/m2) Absorption corrected flux in
* rest-frame 0.5-2keV, 1sigma
* upper limit (FluxIntr_Up1_s)
real*4 b2_FluxIS_6(nr__6) ! (mW/m2) Absorption corrected flux in
* rest-frame 0.5-2 keV, 2sigma
* lower limit (FluxIntr_Lo2_s)
real*4 B2_FluxIS_7(nr__6) ! (mW/m2) Absorption corrected flux in
* rest-frame 0.5-2 keV, 2sigma
* upper limit (FluxIntr_Up2_s)
real*4 FluxIBF2keV_3(nr__6) ! (mW/m2/eV) Absorption corrected flux at
* rest-frame 2keV, best- fit
* (FluxIntr_BF_2keV)
real*4 FluxIMed2keV_4(nr__6) ! (mW/m2/eV) Absorption corrected flux at
* rest-frame 2keV, median
* (FluxIntr_Med_2keV)
real*4 b_FluxI2keV_8(nr__6) ! (mW/m2/eV) Absorption corrected flux at
* rest-frame 2keV, 1sigma
* lower limit (FluxIntr_Lo1_2keV)
real*4 B_FluxI2keV_9(nr__6) ! (mW/m2/eV) Absorption corrected flux at
* rest-frame 2keV, 1sigma
* upper limit (FluxIntr_Up1_2keV)
real*4 b2_FluxI2keV_6(nr__6) ! (mW/m2/eV) Absorption corrected flux at
* rest-frame 2keV, 2sigma
* lower limit (FluxIntr_Lo2_2keV)
real*4 B2_FluxI2keV_7(nr__6) ! (mW/m2/eV) Absorption corrected flux at
* rest-frame 2keV, 2sigma
* upper limit (FluxIntr_Up2_2keV)
real*8 LumIBFS_3 (nr__6) ! (10-7W) ?=-99 Intrinsic luminosity in
* rest-frame 0.5-2 keV, best-fit
* model (LumiIntr_BF_s)
real*8 LumIMedS_4 (nr__6) ! (10-7W) ?=-99 Intrinsic luminosity in
* rest-frame 0.5-2 keV, posterior
* median (LumiIntr_Med_s)
real*8 b_LumIS_8 (nr__6) ! (10-7W) ?=-99 Intrinsic luminosity in
* rest-frame 0.5-2 keV, 1sigma
* lower limit (LumiIntr_Lo1_s)
real*8 B_LumIS_9 (nr__6) ! (10-7W) ?=-99 Intrinsic luminosity in
* rest-frame 0.5-2 keV, 1sigma
* upper limit (LumiIntr_Up1_s)
real*8 b2_LumIS_6 (nr__6) ! (10-7W) ?=-99 Intrinsic luminosity in
* rest-frame 0.5-2 keV, 2sigma
* lower limit (LumiIntr_Lo2_s)
real*8 B2_LumIS_7 (nr__6) ! (10-7W) ?=-99 Intrinsic luminosity in
* rest-frame 0.5-2 keV, 2sigma
* upper limit (LumiIntr_Up2_s)
real*8 LumIBF2keV_3(nr__6) ! (10-7W/eV) ?=-99 Intrinsic luminosity at
* rest-frame 2keV, best-fit model
* (LumiIntr_BF_2keV)
real*8 LumIMed2keV_4(nr__6) ! (10-7W/eV) ?=-99 Intrinsic luminosity at
* rest-frame 2keV, posterior
* median (LumiIntr_Med_2keV)
real*8 b_LumI2keV_8(nr__6) ! (10-7W/eV) ?=-99 Intrinsic luminosity at
* rest-frame 2keV, 1sigma
* lower limit (LumiIntr_Lo1_2keV)
real*8 B_LumI2keV_9(nr__6) ! (10-7W/eV) ?=-99 Intrinsic luminosity at
* rest-frame 2keV, 1sigma
* upper limit (LumiIntr_Up1_2keV)
real*8 b2_LumI2keV_6(nr__6) ! (10-7W/eV) ?=-99 Intrinsic luminosity at
* rest-frame 2keV, 2sigma
* lower limit (LumiIntr_Lo2_2keV)
real*8 B2_LumI2keV_7(nr__6) ! (10-7W/eV) ?=-99 Intrinsic luminosity at
* rest-frame 2keV, 2sigma upper
* limit (LumiIntr_Up2_2keV)
real*8 lognHMed_4 (nr__6) ! ([cm-2]) log AGN column density,
* posterior median (lognH_Med)
real*8 b_lognH_8 (nr__6) ! ([cm-2]) log AGN column density,
* percentile lower limit (lognH_Lo)
real*8 B_lognH_9 (nr__6) ! ([cm-2]) log AGN column density,
* percentile upper limit (lognH_Up)
real*8 lognHMean_4(nr__6) ! ([cm-2]) log AGN column density, mean
* (lognH_Mean)
real*8 s_lognH_4 (nr__6) ! ([cm-2]) log AGN column density,
* standard deviation (lognH_Std)
real*8 logPowNMed_3(nr__6) ! ([ph/keV/cm2/s]) log power-law normalization,
* posterior median (logPowNorm_Med)
real*8 b_logPowN_6(nr__6) ! ([ph/keV/cm2/s]) log power-law normalization,
* percentile lower limit
* (logPowNorm_Lo)
real*8 B_logPowN_7(nr__6) ! ([ph/keV/cm2/s]) log power-law normalization,
* percentile upper limit
* (logPowNorm_Up)
real*8 logPowNMean_3(nr__6) ! ([ph/keV/cm2/s]) log power-law normalization,
* mean (logPowNorm_Mean)
real*8 s_logPowN_3(nr__6) ! ([ph/keV/cm2/s]) log power-law normalization,
* standard deviation
* (logPowNorm_Std)
real*4 logBkgNMed_4(nr__6) ! log background normalization,
* posterior median (logBkgNorm_Med)
real*4 b_logBkgN_8(nr__6) ! log background normalization,
* percentile lower limit
* (logBkgNorm_Lo)
real*4 B_logBkgN_9(nr__6) ! log background normalization,
* percentile upper limit
* (logBkgNorm_Up)
real*4 logBkgNMean_4(nr__6) ! log background normalization,
* mean (logBkgNorm_Mean)
real*8 s_logBkgN_4(nr__6) ! log background normalization,
* standard deviation
* (logBkgNorm_Std)
real*8 logZ_4 (nr__6) ! log10 Bayesian evidence (logZ)
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table8.dat' ! Shape-fixed-powerlaw results
integer*4 nr__7
parameter (nr__7=27910) ! Number of records
character*746 ar__7 ! Full-size record
integer*4 ID_SRC_7 (nr__7) ! [1/32683] ID of the sources in
* the eFEDS main X-ray catalog
* (Paper I) (ID_SRC)
real*4 z_5 (nr__7) ! [-0.01/8.0] The redshift adopted
* for the spectral model
* (Redshift)
real*8 logPowNKL_4(nr__7) ! log power-law normalization,
* KL divergence (in nats units)
* (logPowNorm_KL)
real*8 b_logPowNH_8(nr__7) ! ([ph/keV/cm2/s]) log power-law normalization,
* HDI lower limit (logPowNorm_HLo)
real*8 B_logPowNH_9(nr__7) ! ([ph/keV/cm2/s]) log power-law normalization,
* HDI upper limit (logPowNorm_HUp)
real*8 logPowNBF_4(nr__7) ! ([ph/keV/cm2/s]) log power-law normalization,
* best-fit model (logPowNorm_BF)
real*4 FluxObsBFS_5(nr__7) ! (mW/m2) Observed flux in observed
* 0.5-2 keV, best-fit model
* (FluxObsv_BF_s)
real*4 FluxObsMedS_7(nr__7) ! (mW/m2) Observed flux in observed
* 0.5-2 keV, posterior median
* (FluxObsv_Med_s)
real*4 b_FluxObsS_14(nr__7) ! (mW/m2) Observed flux in observed
* 0.5-2 keV, 1sigma lower limit
* (FluxObsv_Lo1_s)
real*4 B_FluxObsS_15(nr__7) ! (mW/m2) Observed flux in observed
* 0.5-2 keV, 1sigma upper limit
* (FluxObsvs)
real*4 b2_FluxObsS_10(nr__7) ! (mW/m2) Observed flux in observed
* 0.5-2 keV, 2sigma lower limit
* (FluxObsvs)
real*4 B2_FluxObsS_11(nr__7) ! (mW/m2) Observed flux in observed
* 0.5-2 keV, 2sigma upper limit
* (FluxObsvs)
real*4 FluxObsBFT_5(nr__7) ! (mW/m2) Observed flux in observed
* 2.3-5 keV, best-fit model
* (FluxObsv_BF_t)
real*4 FluxObsMedT_7(nr__7) ! (mW/m2) Observed flux in observed
* 2.3-5 keV, posterior median
* (FluxObsv_Med_t)
real*4 b_FluxObsT_14(nr__7) ! (mW/m2) Observed flux in observed
* 2.3-5 keV, 1sigma lower limit
* (FluxObsv_Lo1_t)
real*4 B_FluxObsT_15(nr__7) ! (mW/m2) Observed flux in observed
* 2.3-5 keV, 1sigma upper limit
* (FluxObsvt)
real*4 b2_FluxObsT_10(nr__7) ! (mW/m2) Observed flux in observed
* 2.3-5 keV, 2sigma lower limit
* (FluxObsvt)
real*4 B2_FluxObsT_11(nr__7) ! (mW/m2) Observed flux in observed
* 2.3-5 keV, 2sigma upper limit
* (FluxObsvt)
real*4 FluxCBFS_4 (nr__7) ! (mW/m2) Absorption corrected flux in
* observed 0.5-2 keV,
* best-fit model (FluxCorr_BF_s)
real*4 FluxCMedS_5(nr__7) ! (mW/m2) Absorption corrected flux in
* observed 0.5-2 keV, posterior
* median (FluxCorr_Med_s)
real*4 b_FluxCS_10(nr__7) ! (mW/m2) Absorption corrected flux in
* observed 0.5-2 keV, 1sigma
* lower limit (FluxCorr_Lo1_s)
real*4 B_FluxCS_11(nr__7) ! (mW/m2) Absorption corrected flux in
* observed 0.5-2 keV, 1sigma
* upper limit (FluxCorrs)
real*4 b2_FluxCS_8(nr__7) ! (mW/m2) Absorption corrected flux in
* observed 0.5-2 keV, 2sigma
* lower limit (FluxCorrs)
real*4 B2_FluxCS_9(nr__7) ! (mW/m2) Absorption corrected flux in
* observed 0.5-2 keV, 2sigma
* upper limit (FluxCorrs)
real*4 FluxCBFT_4 (nr__7) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV, best-fit
* model (FluxCorr_BF_t)
real*4 FluxCMedT_5(nr__7) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV, posterior
* median (FluxCorr_Med_t)
real*4 b_FluxCT_10(nr__7) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV, 1sigma
* lower limit (FluxCorr_Lo1_t)
real*4 B_FluxCT_11(nr__7) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV, 1sigma
* upper limit (FluxCorrt)
real*4 b2_FluxCT_8(nr__7) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV, 2sigma
* lower limit (FluxCorrt)
real*4 B2_FluxCT_9(nr__7) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV, 2sigma
* upper limit (FluxCorrt)
real*4 FluxIBFS_4 (nr__7) ! (mW/m2) Absorption corrected flux in
* rest-frame 0.5-2 keV, best-fit
* model (FluxIntr_BF_s)
real*4 FluxIMedS_5(nr__7) ! (mW/m2) Absorption corrected flux in
* rest-frame 0.5-2 keV, posterior
* median (FluxIntr_Med_s)
real*4 b_FluxIS_10(nr__7) ! (mW/m2) Absorption corrected flux in
* rest-frame 0.5-2keV, 1sigma
* lower limit (FluxIntr_Lo1_s)
real*4 B_FluxIS_11(nr__7) ! (mW/m2) Absorption corrected flux in
* rest-frame 0.5-2keV, 1sigma
* upper limit (FluxIntrs)
real*4 b2_FluxIS_8(nr__7) ! (mW/m2) Absorption corrected flux in
* rest-frame 0.5-2 keV, 2sigma
* lower limit (FluxIntrs)
real*4 B2_FluxIS_9(nr__7) ! (mW/m2) Absorption corrected flux in
* rest-frame 0.5-2 keV, 2sigma
* upper limit (FluxIntrs)
real*4 FluxIBF2keV_4(nr__7) ! (mW/m2/eV) Absorption corrected flux at
* rest-frame 2keV, best- fit
* (FluxIntr_BF_2keV)
real*4 FluxIMed2keV_5(nr__7) ! (mW/m2/eV) Absorption corrected flux at
* rest-frame 2keV, median
* (FluxIntr_Med_2keV)
real*4 b_FluxI2keV_10(nr__7) ! (mW/m2/eV) Absorption corrected flux at
* rest-frame 2keV, 1sigma
* lower limit (FluxIntr_Lo1_2keV)
real*4 B_FluxI2keV_11(nr__7) ! (mW/m2/eV) Absorption corrected flux at
* rest-frame 2keV, 1sigma
* upper limit (FluxIntr_Up1_2keV)
real*4 b2_FluxI2keV_8(nr__7) ! (mW/m2/eV) Absorption corrected flux at
* rest-frame 2keV, 2sigma
* lower limit (FluxIntr_Lo2_2keV)
real*4 B2_FluxI2keV_9(nr__7) ! (mW/m2/eV) Absorption corrected flux at
* rest-frame 2keV, 2sigma
* upper limit (FluxIntr_Up2_2keV)
real*8 LumIBFS_4 (nr__7) ! (10-7W) ?=-99 Intrinsic luminosity in
* rest-frame 0.5-2 keV, best-fit
* model (LumiIntr_BF_s)
real*8 LumIMedS_5 (nr__7) ! (10-7W) ?=-99 Intrinsic luminosity in
* rest-frame 0.5-2 keV, posterior
* median (LumiIntr_Med_s)
real*8 b_LumIS_10 (nr__7) ! (10-7W) ?=-99 Intrinsic luminosity in
* rest-frame 0.5-2 keV, 1sigma
* lower limit (LumiIntr_Lo1_s)
real*8 B_LumIS_11 (nr__7) ! (10-7W) ?=-99 Intrinsic luminosity in
* rest-frame 0.5-2 keV, 1sigma
* upper limit (LumiIntrs)
real*8 b2_LumI2S (nr__7) ! (10-7W) ?=-99 Intrinsic luminosity in
* rest-frame 0.5-2 keV, 2sigma
* lower limit (LumiIntrs)
real*8 B2_LumIS_8 (nr__7) ! (10-7W) ?=-99 Intrinsic luminosity in
* rest-frame 0.5-2 keV, 2sigma
* upper limit (LumiIntrs)
real*8 LumIBF2keV_4(nr__7) ! (10-7W/eV) ?=-99 Intrinsic luminosity at
* rest-frame 2keV, best-fit model
* (LumiIntr_BF_2keV)
real*8 LumIMed2keV_5(nr__7) ! (10-7W/eV) ?=-99 Intrinsic luminosity at
* rest-frame 2keV, posterior
* median (LumiIntr_Med_2keV)
real*8 b_LumI2keV_10(nr__7) ! (10-7W/eV) ?=-99 Intrinsic luminosity at
* rest-frame 2keV, 1sigma lower
* limit (LumiIntr_Lo1_2keV)
real*8 B_LumI2keV_11(nr__7) ! (10-7W/eV) ?=-99 Intrinsic luminosity at
* rest-frame 2keV, 1sigma upper
* limit (LumiIntr_Up1_2keV)
real*8 b2_LumI2keV_8(nr__7) ! (10-7W/eV) ?=-99 Intrinsic luminosity at
* rest-frame 2keV, 2sigma lower
* limit (LumiIntr_Lo2_2keV)
real*8 B2_LumI2keV_9(nr__7) ! (10-7W/eV) ?=-99 Intrinsic luminosity at
* rest-frame 2keV, 2sigma upper
* limit (LumiIntr_Up2_2keV)
real*8 logPowNMed_4(nr__7) ! ([ph/keV/cm2/s]) log power-law normalization,
* posterior median
* (logPowNorm_Med)
real*8 b_logPowN_8(nr__7) ! ([ph/keV/cm2/s]) log power-law normalization,
* percentile lower limit
* (logPowNorm_Lo)
real*8 B_logPowN_9(nr__7) ! ([ph/keV/cm2/s]) log power-law normalization,
* percentile upper limit
* (logPowNorm_Up)
real*8 logPowNMean_4(nr__7) ! ([ph/keV/cm2/s]) log power-law normalization,
* mean (logPowNorm_Mean)
real*8 s_logPowN_4(nr__7) ! ([ph/keV/cm2/s]) log power-law normalization,
* standard deviation
* (logPowNorm_Std)
real*4 logBkgNMed_5(nr__7) ! log background normalization,
* posterior median
* (logBkgNorm_Med)
real*4 b_logBkgN_10(nr__7) ! log background normalization,
* percentile lower limit
* (logBkgNorm_Lo)
real*4 B_logBkgN_11(nr__7) ! log background normalization,
* percentile upper limit
* (logBkgNorm_Up)
real*4 logBkgNMean_5(nr__7) ! log background normalization,
* mean (logBkgNorm_Mean)
real*8 s_logBkgN_5(nr__7) ! log background normalization,
* standard deviation
* (logBkgNorm_Std)
real*8 logZ_5 (nr__7) ! log10 Bayesian evidence (logZ)
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table9.dat' ! Soft-band fitting results
integer*4 nr__8
parameter (nr__8=27910) ! Number of records
character*489 ar__8 ! Full-size record
integer*4 ID_SRC_8 (nr__8) ! [1/32683] ID of the sources in the
* eFEDS main X-ray catalog
* (Paper I) (ID_SRC)
real*4 z_6 (nr__8) ! [-0.01/8.0] The redshift adopted
* for the spectral model (Redshift)
real*8 GammaKL_3 (nr__8) ! power-law slope, KL divergence
* (in nats units) (Gamma_KL)
real*8 b_GammaH_6 (nr__8) ! power-law slope, HDI lower limit
* (Gamma_HLo)
real*8 B_GammaH_7 (nr__8) ! power-law slope, HDI upper limit
* (Gamma_HUp)
real*8 lognHKL_5 (nr__8) ! log AGN column density,
* KL divergence (in nats units)
* (lognH_KL)
real*8 b_lognHH_10(nr__8) ! ([cm-2]) log AGN column density,
* HDI lower limit (lognH_HLo)
real*8 B_lognHH_11(nr__8) ! ([cm-2]) log AGN column density,
* HDI upper limit (lognH_HUp)
real*8 logPowNKL_5(nr__8) ! log power-law normalization,
* KL divergence (in nats units)
* (logPowNorm_KL)
real*8 b_logPowNH_10(nr__8) ! ([ph/keV/cm2/s]) log power-law normalization,
* HDI lower limit (logPowNorm_HLo)
real*8 B_logPowNH_11(nr__8) ! ([ph/keV/cm2/s]) log power-law normalization,
* HDI upper limit (logPowNorm_HUp)
real*8 GammaBF_3 (nr__8) ! power-law slope, best-fit model
* (Gamma_BF)
real*8 lognHBF_5 (nr__8) ! ([cm-2]) log AGN column density,
* best-fit model (lognH_BF)
real*4 logPowNBF_5(nr__8) ! ([ph/keV/cm2/s]) log power-law normalization,
* best-fit model (logPowNorm_BF)
real*4 FluxObsBFS_6(nr__8) ! (mW/m2) Observed flux in observed
* 0.5-2 keV, best-fit model
* (FluxObsv_BF_s)
real*4 FluxObsMedS_8(nr__8) ! (mW/m2) Observed flux in observed
* 0.5-2 keV, posterior median
* (FluxObsv_Med_s)
real*4 b_FluxObsS_16(nr__8) ! (mW/m2) Observed flux in observed
* 0.5-2 keV, 1sigma lower limit
* (FluxObsv_Lo1_s)
real*4 B_FluxObsS_17(nr__8) ! (mW/m2) Observed flux in observed
* 0.5-2 keV, 1sigma upper limit
* (FluxObsv_Up1_s)
real*4 b2_FluxObsS_12(nr__8) ! (mW/m2) Observed flux in observed
* 0.5-2 keV, 2sigma lower limit
* (FluxObsv_Lo2_s)
real*4 B2_FluxObsS_13(nr__8) ! (mW/m2) Observed flux in observed
* 0.5-2 keV, 2sigma upper limit
* (FluxObsv_Up2_s)
real*8 GammaMed_3 (nr__8) ! power-law slope, posterior median
* (Gamma_Med)
real*8 b_Gamma_6 (nr__8) ! power-law slope, percentile
* lower limit (Gamma_Lo)
real*8 B_Gamma_7 (nr__8) ! power-law slope, percentile
* upper limit (Gamma_Up)
real*8 GammaMean_3(nr__8) ! power-law slope, mean (Gamma_Mean)
real*8 s_Gamma_3 (nr__8) ! power-law slope,
* standard deviation (Gamma_Std)
real*8 lognHMed_5 (nr__8) ! ([cm-2]) log AGN column density,
* posterior median (lognH_Med)
real*8 b_lognH_10 (nr__8) ! ([cm-2]) log AGN column density, percentile
* lower limit (lognH_Lo)
real*8 B_lognH_11 (nr__8) ! ([cm-2]) log AGN column density, percentile
* upper limit (lognH_Up)
real*8 lognHMean_5(nr__8) ! ([cm-2]) log AGN column density,
* mean (lognH_Mean)
real*8 s_lognH_5 (nr__8) ! ([cm-2]) log AGN column density,
* standard deviation (lognH_Std)
real*8 logPowNMed_5(nr__8) ! ([ph/keV/cm2/s]) log power-law normalization,
* posterior median (logPowNorm_Med)
real*8 b_logPowN_10(nr__8) ! ([ph/keV/cm2/s]) log power-law normalization,
* percentile lower limit
* (logPowNorm_Lo)
real*8 B_logPowN_11(nr__8) ! ([ph/keV/cm2/s]) log power-law normalization,
* percentile upper limit
* (logPowNorm_Up)
real*8 logPowNMean_5(nr__8) ! ([ph/keV/cm2/s]) log power-law normalization,
* mean (logPowNorm_Mean)
real*8 s_logPowN_5(nr__8) ! ([ph/keV/cm2/s]) log power-law normalization,
* standard deviation
* (logPowNorm_Std)
real*4 logBkgNMed_6(nr__8) ! log background normalization,
* posterior median (logBkgNorm_Med)
real*4 blogBkgN (nr__8) ! log background normalization,
* percentile lower limit
* (logBkgNorm_Lo)
real*4 BlogBkgN_1 (nr__8) ! log background normalization,
* percentile upper limit
* (logBkgNorm_Up)
real*4 logBkgNMean_6(nr__8) ! log background normalization,
* mean (logBkgNorm_Mean)
real*8 logBkgN (nr__8) ! log background normalization,
* standard deviation
* (logBkgNorm_Std)
real*8 logZ_6 (nr__8) ! log10 Bayesian evidence (logZ)
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table10.dat' ! Hard-band fitting results
integer*4 nr__9
parameter (nr__9=27910) ! Number of records
character*543 ar__9 ! Full-size record
integer*4 ID_SRC_9 (nr__9) ! [1/32683] ID of the sources in the
* eFEDS main X-ray catalog
* (Paper I) (ID_SRC)
real*4 z_7 (nr__9) ! [-0.01/8.0] The redshift adopted
* for the spectral model (Redshift)
real*8 GammaKL_4 (nr__9) ! power-law slope, KL divergence
* (in nats units) (Gamma_KL)
real*8 e_Gamma (nr__9) ! power-law slope, HDI lower limit
* (Gamma_HLo)
real*8 E_Gamma_1 (nr__9) ! power-law slope, HDI upper limit
* (Gamma_HUp)
real*8 lognHKL_6 (nr__9) ! log AGN column density,
* KL divergence (in nats units)
* (lognH_KL)
real*8 b_lognH_12 (nr__9) ! ([cm-2]) log AGN column density,
* HDI lower limit (lognH_HLo)
real*8 B_lognH_13 (nr__9) ! ([cm-2]) log AGN column density,
* HDI upper limit (lognH_HUp)
real*8 logPowNKL_6(nr__9) ! log power-law normalization,
* KL divergence (in nats units)
* (logPowNorm_KL)
real*8 b_logPowN_12(nr__9) ! ([ph/keV/cm2/s]) log power-law normalization,
* HDI lower limit (logPowNorm_HLo)
real*8 B_logPowN_13(nr__9) ! ([ph/keV/cm2/s]) log power-law normalization,
* HDI upper limit (logPowNorm_HUp)
real*8 GammaBF_4 (nr__9) ! power-law slope, best-fit model
* (Gamma_BF)
real*8 lognHBF_6 (nr__9) ! ([cm-2]) log AGN column density,
* best-fit model (lognH_BF)
real*8 logPowNBF_6(nr__9) ! ([ph/keV/cm2/s]) log power-law normalization,
* best-fit model (logPowNorm_BF)
real*4 FluxObsBFT_6(nr__9) ! (mW/m2) Observed flux in observed 2.3-5keV,
* best-fit model (FluxObsv_BF_t)
real*4 FluxObsMedT_8(nr__9) ! (mW/m2) Observed flux in observed 2.3-5keV,
* posterior median (FluxObsv_Med_t)
real*4 b_FluxObsT_16(nr__9) ! (mW/m2) Observed flux in observed 2.3-5keV,
* 1sigma lower limit
* (FluxObsv_Lo1_t)
real*4 B_FluxObsT_17(nr__9) ! (mW/m2) Observed flux in observed 2.3-5keV,
* 1sigma upper limit
* (FluxObsv_Up1_t)
real*4 b2_FluxObsT_12(nr__9) ! (mW/m2) Observed flux in observed 2.3-5keV,
* 2sigma lower limit
* (FluxObsv_Lo2_t)
real*4 B2_FluxObsT_13(nr__9) ! (mW/m2) Observed flux in observed 2.3-5keV,
* 2sigma upper limit
* (FluxObsv_Up2_t)
real*4 FluxCBFT_5 (nr__9) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV, best-fit model
* (FluxCorr_BF_t)
real*4 FluxCMedT_6(nr__9) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV, posterior
* median (FluxCorr_Med_t)
real*4 b_FluxCMedT(nr__9) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV, 1sigma
* lower limit (FluxCorr_Lo1_t)
real*4 B_FluxCMedT_1(nr__9) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV, 1sigma
* upper limit (FluxCorr_Up1_t)
real*4 b2_FluxCMedT(nr__9) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV, 2sigma
* lower limit (FluxCorr_Lo2_t)
real*4 B2_FluxCMedT_1(nr__9) ! (mW/m2) Absorption corrected flux in
* observed 2.3-5 keV, 2sigma
* upper limit (FluxCorr_Up2_t)
real*8 GammaMed_4 (nr__9) ! power-law slope, posterior median
* (Gamma_Med)
real*8 b_GammaMed (nr__9) ! power-law slope, percentile
* lower limit (Gamma_Lo)
real*8 B_GammaMed_1(nr__9) ! power-law slope, percentile
* upper limit (Gamma_Up)
real*8 GammaMean_4(nr__9) ! power-law slope, mean (Gamma_Mean)
real*8 s_Gamma_4 (nr__9) ! power-law slope,
* standard deviation (Gamma_Std)
real*8 lognHMed_6 (nr__9) ! ([cm-2]) log AGN column density,
* posterior median (lognH_Med)
real*8 b_lognHMed (nr__9) ! ([cm-2]) log AGN column density,
* percentile lower limit (lognH_Lo)
real*8 B_lognHMed_1(nr__9) ! ([cm-2]) log AGN column density,
* percentile upper limit (lognH_Up)
real*8 lognHMean_6(nr__9) ! ([cm-2]) log AGN column density,
* mean (lognH_Mean)
real*8 s_lognH_6 (nr__9) ! ([cm-2]) log AGN column density,
* standard deviation (lognH_Std)
real*8 logPowNMed_6(nr__9) ! ([ph/keV/cm2/s]) log power-law normalization,
* posterior median (logPowNorm_Med)
real*8 b_logPowNMed(nr__9) ! ([ph/keV/cm2/s]) log power-law normalization,
* percentile lower limit
* (logPowNorm_Lo)
real*8 B_logPowNMed_1(nr__9) ! ([ph/keV/cm2/s]) log power-law normalization,
* percentile upper limit
* (logPowNorm_Up)
real*8 logPowNMean_6(nr__9) ! ([ph/keV/cm2/s]) log power-law normalization,
* mean (logPowNorm_Mean)
real*8 s_logPowN_6(nr__9) ! ([ph/keV/cm2/s]) log power-law normalization,
* standard deviation
* (logPowNorm_Std)
real*4 logBkgNMed_7(nr__9) ! log background normalization,
* posterior median (logBkgNorm_Med)
real*4 b_logBkgNMed(nr__9) ! log background normalization,
* percentile lower limit
* (logBkgNorm_Lo)
real*4 B_logBkgNMed_1(nr__9) ! log background normalization,
* percentile upper limit
* (logBkgNorm_Up)
real*4 logBkgNMean_7(nr__9) ! log background normalization,
* mean (logBkgNorm_Mean)
real*8 s_logBkgN_6(nr__9) ! log background normalization,
* standard deviation
* (logBkgNorm_Std)
real*8 logZ_7 (nr__9) ! log10 Bayesian evidence (logZ)
C=============================================================================
C Loading file 'table1.dat' ! The eFEDS AGN catalog
C Format for file interpretation
1 format(
+ I5,1X,F18.14,1X,E24.17,1X,F13.7,1X,E5.4,1X,A11,1X,F18.14,1X,
+ E23.17,1X,I1,1X,I1,1X,F12.10,1X,I1,1X,I1,1X,I1,1X,I1,1X,I1,1X,
+ I1,1X,E22.17,1X,E22.17,1X,F24.18,1X,E11.6,1X,E11.6,1X,E11.6,
+ 1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,
+ E14.9,1X,E14.9,1X,E14.9,1X,F7.4,1X,F7.4,1X,F7.4,1X,F9.6,1X,
+ F9.6,1X,F9.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,
+ E11.6,1X,F11.9,1X,F9.6,1X,F9.6,1X,F9.6,1X,F11.9,1X,F11.9,1X,
+ F9.7,1X,F10.8,1X,F11.6,1X,F11.6,1X,F11.6,1X,F11.6,1X,F11.6,1X,
+ F11.6,1X,F10.6,1X,F10.6,1X,F11.7,1X,E13.8,1X,F11.7,1X,E13.7)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,22079
read(1,'(A736)')ar__
read(ar__,1)
+ ID_SRC(i__),RAcdeg(i__),DEcdeg(i__),DetLike(i__),
+ inArea90(i__),CTPLS8(i__),RALdeg(i__),DELdeg(i__),
+ CTPqual(i__),CTPClass(i__),CTPz(i__),CTPzgrade(i__),
+ inKiDSFlag(i__),LxModel(i__),NHclass(i__),FSModel(i__),
+ FHModel(i__),galNH(i__),galNHI(i__),SrcCts(i__),
+ FluxcMedS(i__),b_FluxcS(i__),B_FluxcS_1(i__),FluxcMedT(i__),
+ b_FluxcT(i__),B_FluxcT_1(i__),FluxIMedS(i__),b_FluxIS(i__),
+ B_FluxIS_1(i__),FluxIMed2keV(i__),b_FluxI2keV(i__),
+ B_FluxI2keV_1(i__),LumIMedS(i__),b_LumIS(i__),B_LumIS_1(i__),
+ LumIMed2keV(i__),b_LumI2keV(i__),B_LumI2keV_1(i__),
+ FluxObsMedS(i__),b_FluxObsS(i__),B_FluxObsS_1(i__),
+ FluxObsMedT(i__),b_FluxObsT(i__),B_FluxObsT_1(i__),
+ lognHKLm1(i__),b_lognHm1(i__),B_lognHm1_1(i__),
+ lognHMedm1(i__),GammaKLm3(i__),b_GammaHm3(i__),
+ B_GammaHm3_1(i__),GammaMedm3(i__),logZm0(i__),logZm1(i__),
+ logZm2(i__),logZm3(i__),logZm4(i__),logZm5(i__),L2500(i__),
+ L5100(i__),W1mag(i__),e_W1mag(i__),W2mag(i__),e_W2mag(i__)
if(ar__(686:696) .EQ. '') W1mag(i__) = rNULL__
if(ar__(698:710) .EQ. '') e_W1mag(i__) = rNULL__
if(ar__(712:722) .EQ. '') W2mag(i__) = rNULL__
if(ar__(724:736) .EQ. '') e_W2mag(i__) = rNULL__
c ..............Just test output...........
write(6,1)
+ ID_SRC(i__),RAcdeg(i__),DEcdeg(i__),DetLike(i__),
+ inArea90(i__),CTPLS8(i__),RALdeg(i__),DELdeg(i__),
+ CTPqual(i__),CTPClass(i__),CTPz(i__),CTPzgrade(i__),
+ inKiDSFlag(i__),LxModel(i__),NHclass(i__),FSModel(i__),
+ FHModel(i__),galNH(i__),galNHI(i__),SrcCts(i__),
+ FluxcMedS(i__),b_FluxcS(i__),B_FluxcS_1(i__),FluxcMedT(i__),
+ b_FluxcT(i__),B_FluxcT_1(i__),FluxIMedS(i__),b_FluxIS(i__),
+ B_FluxIS_1(i__),FluxIMed2keV(i__),b_FluxI2keV(i__),
+ B_FluxI2keV_1(i__),LumIMedS(i__),b_LumIS(i__),B_LumIS_1(i__),
+ LumIMed2keV(i__),b_LumI2keV(i__),B_LumI2keV_1(i__),
+ FluxObsMedS(i__),b_FluxObsS(i__),B_FluxObsS_1(i__),
+ FluxObsMedT(i__),b_FluxObsT(i__),B_FluxObsT_1(i__),
+ lognHKLm1(i__),b_lognHm1(i__),B_lognHm1_1(i__),
+ lognHMedm1(i__),GammaKLm3(i__),b_GammaHm3(i__),
+ B_GammaHm3_1(i__),GammaMedm3(i__),logZm0(i__),logZm1(i__),
+ logZm2(i__),logZm3(i__),logZm4(i__),logZm5(i__),L2500(i__),
+ L5100(i__),W1mag(i__),e_W1mag(i__),W2mag(i__),e_W2mag(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table2.dat' ! Spectral properties
C Format for file interpretation
2 format(
+ I5,1X,F18.14,1X,E24.17,1X,F13.7,1X,F11.7,1X,E5.4,1X,E22.17,1X,
+ E22.17,1X,F11.6,1X,F24.18,1X,F10.6,1X,E10.3,1X,I3,1X,I3,1X,I3,
+ 1X,E13.8,1X,E13.8,1X,F12.10,1X,I1,1X,I1,1X,E13.7,1X,F13.11,1X,
+ E16.9,1X,E13.8,1X,E16.9,1X,E13.8,1X,E16.9,1X,E13.8,1X,E16.9,
+ 1X,E14.9,1X,E16.9,1X,E14.9,1X,E16.9,1X,E14.9,1X,F6.1,1X,F10.7,
+ 1X,F6.1,1X,F10.7,1X,F6.1,1X,F10.7,1X,F6.1,1X,F10.7,1X,F8.6,1X,
+ F8.6,1X,F8.6,1X,F9.7,1X,I3,1X,E11.6,1X,E11.6,1X,E11.6,1X,
+ E11.6,1X,E11.6,1X,E11.6)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,27910
read(1,'(A645)')ar__1
read(ar__1,2)
+ ID_SRC_1(i__),RAcdeg_1(i__),DEcdeg_1(i__),DetLike_1(i__),
+ ExtLike(i__),inArea90_1(i__),galNH_1(i__),galNHI_1(i__),
+ ExpTime(i__),SrcCts_1(i__),RAdeg(i__),DEdeg(i__),Rad(i__),
+ Ann1(i__),Ann2(i__),RegArea(i__),Backscal(i__),
+ BackscalBkg(i__),FSModel_1(i__),FHModel_1(i__),
+ Rate0_2_2_3(i__),e_Rate0_2_2_3(i__),Rate0_2_0_5(i__),
+ e_Rate0_2_0_5(i__),Rate0_5_1(i__),e_Rate0_5_1(i__),
+ Rate1_2(i__),e_Rate1_2(i__),Rate2_4_5(i__),e_Rate2_4_5(i__),
+ Rate2_3_5(i__),e_Rate2_3_5(i__),Rate5_8(i__),e_Rate5_8(i__),
+ BkgCts0_2_0_6(i__),e_BkgCts0_2_0_6(i__),BkgCts0_6_2_3(i__),
+ e_BkgCts0_6_2_3(i__),BkgCts2_3_5(i__),e_BkgCts2_3_5(i__),
+ BkgCts5_8(i__),e_BkgCts5_8(i__),PSFCor0_2_0_5(i__),
+ PSFCor0_5_1(i__),PSFCor1_2(i__),PSFCor2_3_5(i__),Nempty(i__),
+ FluxObsMedS_1(i__),b_FluxObsS_2(i__),B_FluxObsS_3(i__),
+ FluxObsMedT_1(i__),b_FluxObsT_2(i__),B_FluxObsT_3(i__)
c ..............Just test output...........
write(6,2)
+ ID_SRC_1(i__),RAcdeg_1(i__),DEcdeg_1(i__),DetLike_1(i__),
+ ExtLike(i__),inArea90_1(i__),galNH_1(i__),galNHI_1(i__),
+ ExpTime(i__),SrcCts_1(i__),RAdeg(i__),DEdeg(i__),Rad(i__),
+ Ann1(i__),Ann2(i__),RegArea(i__),Backscal(i__),
+ BackscalBkg(i__),FSModel_1(i__),FHModel_1(i__),
+ Rate0_2_2_3(i__),e_Rate0_2_2_3(i__),Rate0_2_0_5(i__),
+ e_Rate0_2_0_5(i__),Rate0_5_1(i__),e_Rate0_5_1(i__),
+ Rate1_2(i__),e_Rate1_2(i__),Rate2_4_5(i__),e_Rate2_4_5(i__),
+ Rate2_3_5(i__),e_Rate2_3_5(i__),Rate5_8(i__),e_Rate5_8(i__),
+ BkgCts0_2_0_6(i__),e_BkgCts0_2_0_6(i__),BkgCts0_6_2_3(i__),
+ e_BkgCts0_6_2_3(i__),BkgCts2_3_5(i__),e_BkgCts2_3_5(i__),
+ BkgCts5_8(i__),e_BkgCts5_8(i__),PSFCor0_2_0_5(i__),
+ PSFCor0_5_1(i__),PSFCor1_2(i__),PSFCor2_3_5(i__),Nempty(i__),
+ FluxObsMedS_1(i__),b_FluxObsS_2(i__),B_FluxObsS_3(i__),
+ FluxObsMedT_1(i__),b_FluxObsT_2(i__),B_FluxObsT_3(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table3.dat' ! APEC fitting results
C Format for file interpretation
3 format(
+ I5,1X,F3.1,1X,F12.10,1X,F10.7,1X,F10.7,1X,F11.9,1X,E15.8,1X,
+ E15.8,1X,F12.10,1X,F11.8,1X,E15.8,1X,F10.8,1X,F10.7,1X,F10.7,
+ 1X,F10.7,1X,E15.8,1X,E15.8,1X,F10.7,1X,E11.6,1X,E11.6,1X,
+ E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,
+ 1X,E11.6,1X,E11.6,1X,E11.6,1X,F10.7,1X,F10.7,1X,F10.7,1X,
+ F10.7,1X,F12.10,1X,E14.8,1X,E14.7,1X,E14.8,1X,E15.8,1X,F12.10,
+ 1X,F12.9,1X,F11.8,1X,F12.9,1X,F11.8,1X,F12.10,1X,F10.7,1X,
+ F11.7,1X,F10.7,1X,F10.7,1X,F12.10,1X,E16.9,1X,E13.7,1X,E13.8,
+ 1X,E15.9,1X,F12.10,1X,F12.6,1X,I3,1X,F11.6)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,27910
read(1,'(A715)')ar__2
read(ar__2,3)
+ ID_SRC_2(i__),z(i__),lognHKL(i__),b_lognHH(i__),
+ B_lognHH_1(i__),logkTKL(i__),b_logkTH(i__),B_logkTH_1(i__),
+ logAbundKL(i__),b_logAbunH(i__),B_logAbunH_1(i__),
+ logApecNormKL(i__),b_logApecNormH(i__),B_logApecNormH_1(i__),
+ lognHBF(i__),logkTBF(i__),logAbundBF(i__),logApecNBF(i__),
+ FluxObsBFS(i__),FluxObsMedS_2(i__),b_FluxObsS_4(i__),
+ B_FluxObsS_5(i__),b2_FluxObsS(i__),B2_FluxObsS_1(i__),
+ FluxObsBFT(i__),FluxObsMedT_2(i__),b_FluxObsT_4(i__),
+ B_FluxObsT_5(i__),b2_FluxObsT(i__),B2_FluxObsT_1(i__),
+ lognHMed(i__),b_lognH(i__),B_lognH_1(i__),lognHMean(i__),
+ s_lognH(i__),logkTMed(i__),b_logkT(i__),B_logkT_1(i__),
+ logkTMean(i__),s_logkT(i__),logAbundMed(i__),b_logAbund(i__),
+ B_logAbund_1(i__),logAbundMean(i__),s_logAbund(i__),
+ logApecNMed(i__),b_logApecN(i__),B_logApecN_1(i__),
+ logApecNMean(i__),s_logApecN(i__),logBkgNMed(i__),
+ b_logBkgN(i__),B_logBkgN_1(i__),logBkgNMean(i__),
+ s_logBkgN(i__),chi25(i__),dof25(i__),logZ(i__)
c ..............Just test output...........
write(6,3)
+ ID_SRC_2(i__),z(i__),lognHKL(i__),b_lognHH(i__),
+ B_lognHH_1(i__),logkTKL(i__),b_logkTH(i__),B_logkTH_1(i__),
+ logAbundKL(i__),b_logAbunH(i__),B_logAbunH_1(i__),
+ logApecNormKL(i__),b_logApecNormH(i__),B_logApecNormH_1(i__),
+ lognHBF(i__),logkTBF(i__),logAbundBF(i__),logApecNBF(i__),
+ FluxObsBFS(i__),FluxObsMedS_2(i__),b_FluxObsS_4(i__),
+ B_FluxObsS_5(i__),b2_FluxObsS(i__),B2_FluxObsS_1(i__),
+ FluxObsBFT(i__),FluxObsMedT_2(i__),b_FluxObsT_4(i__),
+ B_FluxObsT_5(i__),b2_FluxObsT(i__),B2_FluxObsT_1(i__),
+ lognHMed(i__),b_lognH(i__),B_lognH_1(i__),lognHMean(i__),
+ s_lognH(i__),logkTMed(i__),b_logkT(i__),B_logkT_1(i__),
+ logkTMean(i__),s_logkT(i__),logAbundMed(i__),b_logAbund(i__),
+ B_logAbund_1(i__),logAbundMean(i__),s_logAbund(i__),
+ logApecNMed(i__),b_logApecN(i__),B_logApecN_1(i__),
+ logApecNMean(i__),s_logApecN(i__),logBkgNMed(i__),
+ b_logBkgN(i__),B_logBkgN_1(i__),logBkgNMean(i__),
+ s_logBkgN(i__),chi25(i__),dof25(i__),logZ(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table4.dat' ! Single-powerlaw results
C Format for file interpretation
4 format(
+ I5,1X,E9.2,1X,F12.9,1X,F10.8,1X,F9.7,1X,F11.9,1X,F9.6,1X,F9.6,
+ 1X,F10.8,1X,F10.7,1X,F10.7,1X,F12.9,1X,F9.6,1X,F10.7,1X,E11.6,
+ 1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,
+ E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,
+ 1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,
+ E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,
+ 1X,E11.6,1X,E11.6,1X,E11.6,1X,E14.8,1X,E14.8,1X,E14.8,1X,
+ E14.8,1X,E14.8,1X,E14.8,1X,F8.4,1X,F8.4,1X,F8.4,1X,F8.4,1X,
+ F8.4,1X,F8.4,1X,F10.6,1X,F10.6,1X,F10.6,1X,F10.6,1X,F10.6,1X,
+ F10.6,1X,F10.8,1X,F10.8,1X,F9.7,1X,F10.8,1X,F11.9,1X,F9.6,1X,
+ F9.6,1X,F9.6,1X,F9.6,1X,F11.9,1X,F10.7,1X,F10.7,1X,F10.7,1X,
+ F10.7,1X,F12.10,1X,E16.9,1X,F14.11,1X,E14.7,1X,E16.9,1X,
+ F12.10,1X,F12.6,1X,I3,1X,F11.6,1X,I1)
C Effective file loading
open(unit=1,status='old',file=
+'table4.dat')
write(6,*) '....Loading file: table4.dat'
do i__=1,27910
read(1,'(A990)')ar__3
read(ar__3,4)
+ ID_SRC_3(i__),z_1(i__),GammaKL(i__),b_GammaH(i__),
+ B_GammaH_1(i__),lognHKL_1(i__),b_lognHH_2(i__),
+ B_lognHH_3(i__),logPowNKL(i__),b_logPowNH(i__),
+ B_logPowNH_1(i__),GammaBF(i__),lognHBF_1(i__),logPowNBF(i__),
+ FluxObsBFS_1(i__),FluxObsMedS_3(i__),b_FluxObsS_6(i__),
+ B_FluxObsS_7(i__),b2_FluxObsS_2(i__),B2_FluxObsS_3(i__),
+ FluxObsBFT_1(i__),FluxObsMedT_3(i__),b_FluxObsT_6(i__),
+ B_FluxObsT_7(i__),b2_FluxObsT_2(i__),B2_FluxObsT_3(i__),
+ FluxcBFS(i__),FluxcMedS_1(i__),b_FluxcS_2(i__),
+ B_FluxcS_3(i__),b2_FluxcS(i__),B2_FluxcS_1(i__),FluxcBFT(i__),
+ FluxcMedT_1(i__),b_FluxcT_2(i__),B_FluxcT_3(i__),
+ b2_FluxcT(i__),B2_FluxcT_1(i__),FluxIBFS(i__),
+ FluxIMedS_1(i__),b_FluxIS_2(i__),B_FluxIS_3(i__),
+ b2_FluxIS(i__),B2_FluxIS_1(i__),FluxIBF2keV(i__),
+ FluxIMed2keV_1(i__),b_FluxI2keV_2(i__),B_FluxI2keV_3(i__),
+ b2_FluxI2keV(i__),B2_FluxI2keV_1(i__),LumIBFS(i__),
+ LumIMedS_1(i__),b_LumIS_2(i__),B_LumIS_3(i__),b2_LumIS(i__),
+ B2_LumIS_1(i__),LumIBF2keV(i__),LumIMed2keV_1(i__),
+ b_LumI2keV_2(i__),B_LumI2keV_3(i__),b2_LumI2keV(i__),
+ B2_LumI2keV_1(i__),GammaMed(i__),b_Gamma(i__),B_Gamma_1(i__),
+ GammaMean(i__),s_Gamma(i__),lognHMed_1(i__),b_lognH_2(i__),
+ B_lognH_3(i__),lognHMean_1(i__),s_lognH_1(i__),
+ logPowNMed(i__),b_logPowN(i__),B_logPowN_1(i__),
+ logPowNMean(i__),s_logPowN(i__),logBkgNMed_1(i__),
+ b_logBkgN_2(i__),B_logBkgN_3(i__),logBkgNMean_1(i__),
+ s_logBkgN_1(i__),chi25_1(i__),dof25_1(i__),logZ_1(i__),
+ NHclass_1(i__)
c ..............Just test output...........
write(6,4)
+ ID_SRC_3(i__),z_1(i__),GammaKL(i__),b_GammaH(i__),
+ B_GammaH_1(i__),lognHKL_1(i__),b_lognHH_2(i__),
+ B_lognHH_3(i__),logPowNKL(i__),b_logPowNH(i__),
+ B_logPowNH_1(i__),GammaBF(i__),lognHBF_1(i__),logPowNBF(i__),
+ FluxObsBFS_1(i__),FluxObsMedS_3(i__),b_FluxObsS_6(i__),
+ B_FluxObsS_7(i__),b2_FluxObsS_2(i__),B2_FluxObsS_3(i__),
+ FluxObsBFT_1(i__),FluxObsMedT_3(i__),b_FluxObsT_6(i__),
+ B_FluxObsT_7(i__),b2_FluxObsT_2(i__),B2_FluxObsT_3(i__),
+ FluxcBFS(i__),FluxcMedS_1(i__),b_FluxcS_2(i__),
+ B_FluxcS_3(i__),b2_FluxcS(i__),B2_FluxcS_1(i__),FluxcBFT(i__),
+ FluxcMedT_1(i__),b_FluxcT_2(i__),B_FluxcT_3(i__),
+ b2_FluxcT(i__),B2_FluxcT_1(i__),FluxIBFS(i__),
+ FluxIMedS_1(i__),b_FluxIS_2(i__),B_FluxIS_3(i__),
+ b2_FluxIS(i__),B2_FluxIS_1(i__),FluxIBF2keV(i__),
+ FluxIMed2keV_1(i__),b_FluxI2keV_2(i__),B_FluxI2keV_3(i__),
+ b2_FluxI2keV(i__),B2_FluxI2keV_1(i__),LumIBFS(i__),
+ LumIMedS_1(i__),b_LumIS_2(i__),B_LumIS_3(i__),b2_LumIS(i__),
+ B2_LumIS_1(i__),LumIBF2keV(i__),LumIMed2keV_1(i__),
+ b_LumI2keV_2(i__),B_LumI2keV_3(i__),b2_LumI2keV(i__),
+ B2_LumI2keV_1(i__),GammaMed(i__),b_Gamma(i__),B_Gamma_1(i__),
+ GammaMean(i__),s_Gamma(i__),lognHMed_1(i__),b_lognH_2(i__),
+ B_lognH_3(i__),lognHMean_1(i__),s_lognH_1(i__),
+ logPowNMed(i__),b_logPowN(i__),B_logPowN_1(i__),
+ logPowNMean(i__),s_logPowN(i__),logBkgNMed_1(i__),
+ b_logBkgN_2(i__),B_logBkgN_3(i__),logBkgNMean_1(i__),
+ s_logBkgN_1(i__),chi25_1(i__),dof25_1(i__),logZ_1(i__),
+ NHclass_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table5.dat' ! Double-powerlaw results
C Format for file interpretation
5 format(
+ I5,1X,E9.2,1X,F12.10,1X,F10.8,1X,F9.7,1X,F13.9,1X,F10.8,1X,
+ F9.7,1X,F11.9,1X,F9.6,1X,F9.6,1X,F11.9,1X,F10.7,1X,F10.7,1X,
+ F13.10,1X,F11.8,1X,E16.9,1X,F8.6,1X,F11.8,1X,F9.6,1X,F10.7,1X,
+ E15.8,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,
+ 1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,
+ E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,
+ 1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,
+ E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,
+ 1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,F8.4,1X,F8.4,1X,F8.4,
+ 1X,F8.4,1X,F8.4,1X,F8.4,1X,F8.4,1X,F8.4,1X,F8.4,1X,F8.4,1X,
+ F8.4,1X,F8.4,1X,F9.7,1X,F10.8,1X,F9.7,1X,F9.7,1X,F11.9,1X,
+ F10.8,1X,F10.8,1X,F9.7,1X,F10.8,1X,E12.7,1X,F9.6,1X,F9.6,1X,
+ F9.6,1X,F9.6,1X,F11.9,1X,F10.7,1X,F10.7,1X,F10.7,1X,F10.7,1X,
+ F12.10,1X,F11.8,1X,F11.8,1X,F12.9,1X,F11.8,1X,F10.8,1X,E16.9,
+ 1X,F14.11,1X,E14.7,1X,E16.9,1X,F12.10,1X,F12.6,1X,I3,1X,F11.6)
C Effective file loading
open(unit=1,status='old',file=
+'table5.dat')
write(6,*) '....Loading file: table5.dat'
do i__=1,27910
read(1,'(A1175)')ar__4
read(ar__4,5)
+ ID_SRC_4(i__),z_2(i__),dGmKL(i__),b_dGmH(i__),B_dGmH_1(i__),
+ GammaKL_1(i__),b_GammaH_2(i__),B_GammaH_3(i__),lognHKL_2(i__),
+ b_lognHH_4(i__),B_lognHH_5(i__),logPowNKL_1(i__),
+ b_logPowNH_2(i__),B_logPowNH_3(i__),logFracKL(i__),
+ b_logFracH(i__),B_logFracH_1(i__),dGmBF(i__),GammaBF_1(i__),
+ lognHBF_2(i__),logPowNBF_1(i__),logFracBF(i__),
+ FluxObsBFS_2(i__),FluxObsMedS_4(i__),b_FluxObsS_8(i__),
+ B_FluxObsS_9(i__),b2_FluxObsS_4(i__),B2_FluxObsS_5(i__),
+ FluxObsBFT_2(i__),FluxObsMedT_4(i__),b_FluxObsT_8(i__),
+ B_FluxObsT_9(i__),b2_FluxObsT_4(i__),B2_FluxObsT_5(i__),
+ FluxCBFS_1(i__),FluxCMedS_2(i__),b_FluxCS_4(i__),
+ B_FluxCS_5(i__),b2_FluxCS_2(i__),B2_FluxCS_3(i__),
+ FluxCBFT_1(i__),FluxCMedT_2(i__),b_FluxCT_4(i__),
+ B_FluxCT_5(i__),b2_FluxCT_2(i__),B2_FluxCT_3(i__),
+ FluxIBFS_1(i__),FluxIMedS_2(i__),b_FluxIS_4(i__),
+ B_FluxIS_5(i__),b2_FluxIS_2(i__),B2_FluxIS_3(i__),
+ FluxIBF2keV_1(i__),FluxIMed2keV_2(i__),b_FluxI2keV_4(i__),
+ B_FluxI2keV_5(i__),b2_FluxI2keV_2(i__),B2_FluxI2keV_3(i__),
+ LumIBFS_1(i__),LumIMedS_2(i__),b_LumIS_4(i__),B_LumIS_5(i__),
+ b2_LumIS_2(i__),B2_LumIS_3(i__),LumIBF2keV_1(i__),
+ LumIMed2keV_2(i__),b_LumI2keV_4(i__),B_LumI2keV_5(i__),
+ b2_LumI2keV_2(i__),B2_LumI2keV_3(i__),dGmMed(i__),b_dGm(i__),
+ B_dGm_1(i__),dGmMean(i__),s_dGm(i__),GammaMed_1(i__),
+ b_Gamma_2(i__),B_Gamma_3(i__),GammaMean_1(i__),s_Gamma_1(i__),
+ lognHMed_2(i__),b_lognH_4(i__),B_lognH_5(i__),
+ lognHMean_2(i__),s_lognH_2(i__),logPowNMed_1(i__),
+ b_logPowN_2(i__),B_logPowN_3(i__),logPowNMean_1(i__),
+ s_logPowN_1(i__),logFracMed(i__),b_logFrac(i__),
+ B_logFrac_1(i__),logFracMean(i__),s_logFrac(i__),
+ logBkgNMed_2(i__),b_logBkgN_4(i__),B_logBkgN_5(i__),
+ logBkgNMean_2(i__),s_logBkgN_2(i__),chi25_2(i__),dof25_2(i__),
+ logZ_2(i__)
if(ar__4(51:63) .EQ. '') GammaKL_1(i__) = rNULL__
if(ar__4(152:164) .EQ. '') logFracKL(i__) = rNULL__
c ..............Just test output...........
write(6,5)
+ ID_SRC_4(i__),z_2(i__),dGmKL(i__),b_dGmH(i__),B_dGmH_1(i__),
+ GammaKL_1(i__),b_GammaH_2(i__),B_GammaH_3(i__),lognHKL_2(i__),
+ b_lognHH_4(i__),B_lognHH_5(i__),logPowNKL_1(i__),
+ b_logPowNH_2(i__),B_logPowNH_3(i__),logFracKL(i__),
+ b_logFracH(i__),B_logFracH_1(i__),dGmBF(i__),GammaBF_1(i__),
+ lognHBF_2(i__),logPowNBF_1(i__),logFracBF(i__),
+ FluxObsBFS_2(i__),FluxObsMedS_4(i__),b_FluxObsS_8(i__),
+ B_FluxObsS_9(i__),b2_FluxObsS_4(i__),B2_FluxObsS_5(i__),
+ FluxObsBFT_2(i__),FluxObsMedT_4(i__),b_FluxObsT_8(i__),
+ B_FluxObsT_9(i__),b2_FluxObsT_4(i__),B2_FluxObsT_5(i__),
+ FluxCBFS_1(i__),FluxCMedS_2(i__),b_FluxCS_4(i__),
+ B_FluxCS_5(i__),b2_FluxCS_2(i__),B2_FluxCS_3(i__),
+ FluxCBFT_1(i__),FluxCMedT_2(i__),b_FluxCT_4(i__),
+ B_FluxCT_5(i__),b2_FluxCT_2(i__),B2_FluxCT_3(i__),
+ FluxIBFS_1(i__),FluxIMedS_2(i__),b_FluxIS_4(i__),
+ B_FluxIS_5(i__),b2_FluxIS_2(i__),B2_FluxIS_3(i__),
+ FluxIBF2keV_1(i__),FluxIMed2keV_2(i__),b_FluxI2keV_4(i__),
+ B_FluxI2keV_5(i__),b2_FluxI2keV_2(i__),B2_FluxI2keV_3(i__),
+ LumIBFS_1(i__),LumIMedS_2(i__),b_LumIS_4(i__),B_LumIS_5(i__),
+ b2_LumIS_2(i__),B2_LumIS_3(i__),LumIBF2keV_1(i__),
+ LumIMed2keV_2(i__),b_LumI2keV_4(i__),B_LumI2keV_5(i__),
+ b2_LumI2keV_2(i__),B2_LumI2keV_3(i__),dGmMed(i__),b_dGm(i__),
+ B_dGm_1(i__),dGmMean(i__),s_dGm(i__),GammaMed_1(i__),
+ b_Gamma_2(i__),B_Gamma_3(i__),GammaMean_1(i__),s_Gamma_1(i__),
+ lognHMed_2(i__),b_lognH_4(i__),B_lognH_5(i__),
+ lognHMean_2(i__),s_lognH_2(i__),logPowNMed_1(i__),
+ b_logPowN_2(i__),B_logPowN_3(i__),logPowNMean_1(i__),
+ s_logPowN_1(i__),logFracMed(i__),b_logFrac(i__),
+ B_logFrac_1(i__),logFracMean(i__),s_logFrac(i__),
+ logBkgNMed_2(i__),b_logBkgN_4(i__),B_logBkgN_5(i__),
+ logBkgNMean_2(i__),s_logBkgN_2(i__),chi25_2(i__),dof25_2(i__),
+ logZ_2(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table6.dat' ! Powerlaw+blackbody results
C Format for file interpretation
6 format(
+ I5,1X,E9.2,1X,F12.9,1X,F11.9,1X,F9.7,1X,F11.9,1X,F9.6,1X,F9.6,
+ 1X,F11.9,1X,F10.7,1X,F10.7,1X,F12.10,1X,F11.8,1X,F11.8,1X,
+ F12.10,1X,F10.7,1X,F10.7,1X,F11.8,1X,F9.6,1X,F10.7,1X,F11.8,
+ 1X,F10.7,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,
+ E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,
+ 1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,
+ E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,
+ 1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E14.8,1X,
+ E14.8,1X,E14.8,1X,E14.8,1X,E14.8,1X,E14.8,1X,F8.4,1X,F8.4,1X,
+ F8.4,1X,F8.4,1X,F8.4,1X,F8.4,1X,F10.6,1X,F10.6,1X,F10.6,1X,
+ F10.6,1X,F10.6,1X,F10.6,1X,F10.8,1X,F10.8,1X,F9.7,1X,F10.8,1X,
+ F11.9,1X,F9.6,1X,F9.6,1X,F9.6,1X,F9.6,1X,F11.9,1X,F10.7,1X,
+ F10.7,1X,F10.7,1X,F10.7,1X,F12.10,1X,F11.8,1X,F11.8,1X,F11.8,
+ 1X,F11.8,1X,F12.10,1X,F10.7,1X,F10.7,1X,F10.7,1X,F10.7,1X,
+ F11.9,1X,E16.9,1X,F14.11,1X,E15.8,1X,E16.9,1X,F12.10,1X,F11.6,
+ 1X,I3,1X,F11.6,1X,F15.11)
C Effective file loading
open(unit=1,status='old',file=
+'table6.dat')
write(6,*) '....Loading file: table6.dat'
do i__=1,27910
read(1,'(A1217)')ar__5
read(ar__5,6)
+ ID_SRC_5(i__),z_3(i__),GammaKL_2(i__),b_GammaH_4(i__),
+ B_GammaH_5(i__),lognHKL_3(i__),b_lognHH_6(i__),
+ B_lognHH_7(i__),logPowNKL_2(i__),b_logPowNH_4(i__),
+ B_logPowNH_5(i__),logkTKL_1(i__),b_logkTH_2(i__),
+ B_logkTH_3(i__),logBBNKL(i__),b_logBBNH(i__),B_logBBNH_1(i__),
+ GammaBF_2(i__),lognHBF_3(i__),logPowNBF_2(i__),logkTBF_1(i__),
+ logBBNBF(i__),FluxObsBFS_3(i__),FluxObsMedS_5(i__),
+ b_FluxObsS_10(i__),B_FluxObsS_11(i__),b2_FluxObsS_6(i__),
+ B2_FluxObsS_7(i__),FluxObsBFT_3(i__),FluxObsMedT_5(i__),
+ b_FluxObsT_10(i__),B_FluxObsT_11(i__),b2_FluxObsT_6(i__),
+ B2_FluxObsT_7(i__),FluxCBFS_2(i__),FluxCMedS_3(i__),
+ b_FluxCS_6(i__),B_FluxCS_7(i__),b2_FluxCS_4(i__),
+ B2_FluxCS_5(i__),FluxCBFT_2(i__),FluxCMedT_3(i__),
+ b_FluxCT_6(i__),B_FluxCT_7(i__),b2_FluxCT_4(i__),
+ B2_FluxCT_5(i__),FluxIBFS_2(i__),FluxIMedS_3(i__),
+ b_FluxIS_6(i__),B_FluxIS_7(i__),b2_FluxIS_4(i__),
+ B2_FluxIS_5(i__),FluxIBF2keV_2(i__),FluxIMed2keV_3(i__),
+ b_FluxI2keV_6(i__),B_FluxI2keV_7(i__),b2_FluxI2keV_4(i__),
+ B2_FluxI2keV_5(i__),LumIBFS_2(i__),LumIMedS_3(i__),
+ b_LumIS_6(i__),B_LumIS_7(i__),b2_LumIS_4(i__),B2_LumIS_5(i__),
+ LumIBF2keV_2(i__),LumIMed2keV_3(i__),b_LumI2keV_6(i__),
+ B_LumI2keV_7(i__),b2_LumI2keV_4(i__),B2_LumI2keV_5(i__),
+ GammaMed_2(i__),b_Gamma_4(i__),B_Gamma_5(i__),
+ GammaMean_2(i__),s_Gamma_2(i__),lognHMed_3(i__),
+ b_lognH_6(i__),B_lognH_7(i__),lognHMean_3(i__),s_lognH_3(i__),
+ logPowNMed_2(i__),b_logPowN_4(i__),B_logPowN_5(i__),
+ logPowNMean_2(i__),s_logPowN_2(i__),logkTMed_1(i__),
+ b_logkT_2(i__),B_logkT_3(i__),logkTMean_1(i__),s_logkT_1(i__),
+ logBBNMed(i__),b_logBBN(i__),B_logBBN_1(i__),logBBNMean(i__),
+ s_logBBN(i__),logBkgNMed_3(i__),b_logBkgN_6(i__),
+ B_logBkgN_7(i__),logBkgNMean_3(i__),s_logBkgN_3(i__),
+ chi25_3(i__),dof25_3(i__),logZ_3(i__),logRbb(i__)
c ..............Just test output...........
write(6,6)
+ ID_SRC_5(i__),z_3(i__),GammaKL_2(i__),b_GammaH_4(i__),
+ B_GammaH_5(i__),lognHKL_3(i__),b_lognHH_6(i__),
+ B_lognHH_7(i__),logPowNKL_2(i__),b_logPowNH_4(i__),
+ B_logPowNH_5(i__),logkTKL_1(i__),b_logkTH_2(i__),
+ B_logkTH_3(i__),logBBNKL(i__),b_logBBNH(i__),B_logBBNH_1(i__),
+ GammaBF_2(i__),lognHBF_3(i__),logPowNBF_2(i__),logkTBF_1(i__),
+ logBBNBF(i__),FluxObsBFS_3(i__),FluxObsMedS_5(i__),
+ b_FluxObsS_10(i__),B_FluxObsS_11(i__),b2_FluxObsS_6(i__),
+ B2_FluxObsS_7(i__),FluxObsBFT_3(i__),FluxObsMedT_5(i__),
+ b_FluxObsT_10(i__),B_FluxObsT_11(i__),b2_FluxObsT_6(i__),
+ B2_FluxObsT_7(i__),FluxCBFS_2(i__),FluxCMedS_3(i__),
+ b_FluxCS_6(i__),B_FluxCS_7(i__),b2_FluxCS_4(i__),
+ B2_FluxCS_5(i__),FluxCBFT_2(i__),FluxCMedT_3(i__),
+ b_FluxCT_6(i__),B_FluxCT_7(i__),b2_FluxCT_4(i__),
+ B2_FluxCT_5(i__),FluxIBFS_2(i__),FluxIMedS_3(i__),
+ b_FluxIS_6(i__),B_FluxIS_7(i__),b2_FluxIS_4(i__),
+ B2_FluxIS_5(i__),FluxIBF2keV_2(i__),FluxIMed2keV_3(i__),
+ b_FluxI2keV_6(i__),B_FluxI2keV_7(i__),b2_FluxI2keV_4(i__),
+ B2_FluxI2keV_5(i__),LumIBFS_2(i__),LumIMedS_3(i__),
+ b_LumIS_6(i__),B_LumIS_7(i__),b2_LumIS_4(i__),B2_LumIS_5(i__),
+ LumIBF2keV_2(i__),LumIMed2keV_3(i__),b_LumI2keV_6(i__),
+ B_LumI2keV_7(i__),b2_LumI2keV_4(i__),B2_LumI2keV_5(i__),
+ GammaMed_2(i__),b_Gamma_4(i__),B_Gamma_5(i__),
+ GammaMean_2(i__),s_Gamma_2(i__),lognHMed_3(i__),
+ b_lognH_6(i__),B_lognH_7(i__),lognHMean_3(i__),s_lognH_3(i__),
+ logPowNMed_2(i__),b_logPowN_4(i__),B_logPowN_5(i__),
+ logPowNMean_2(i__),s_logPowN_2(i__),logkTMed_1(i__),
+ b_logkT_2(i__),B_logkT_3(i__),logkTMean_1(i__),s_logkT_1(i__),
+ logBBNMed(i__),b_logBBN(i__),B_logBBN_1(i__),logBBNMean(i__),
+ s_logBBN(i__),logBkgNMed_3(i__),b_logBkgN_6(i__),
+ B_logBkgN_7(i__),logBkgNMean_3(i__),s_logBkgN_3(i__),
+ chi25_3(i__),dof25_3(i__),logZ_3(i__),logRbb(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table7.dat' ! Gamma-fixed-powerlaw results
C Format for file interpretation
7 format(
+ I5,1X,E9.2,1X,F11.9,1X,F9.6,1X,F9.6,1X,F10.8,1X,F10.7,1X,
+ F10.7,1X,F9.6,1X,F10.7,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,
+ E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,
+ 1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,
+ E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,
+ 1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,
+ E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,F8.4,1X,
+ F8.4,1X,F8.4,1X,F8.4,1X,F8.4,1X,F8.4,1X,F8.4,1X,F8.4,1X,F8.4,
+ 1X,F8.4,1X,F8.4,1X,F8.4,1X,F9.6,1X,F9.6,1X,F9.6,1X,F9.6,1X,
+ F12.10,1X,F10.7,1X,F10.7,1X,F10.7,1X,F10.7,1X,F12.10,1X,E16.9,
+ 1X,E14.7,1X,E15.8,1X,E16.9,1X,F12.10,1X,F11.6)
C Effective file loading
open(unit=1,status='old',file=
+'table7.dat')
write(6,*) '....Loading file: table7.dat'
do i__=1,27910
read(1,'(A841)')ar__6
read(ar__6,7)
+ ID_SRC_6(i__),z_4(i__),lognHKL_4(i__),b_lognHH_8(i__),
+ B_lognHH_9(i__),logPowNKL_3(i__),b_logPowNH_6(i__),
+ B_logPowNH_7(i__),lognHBF_4(i__),logPowNBF_3(i__),
+ FluxObsBFS_4(i__),FluxObsMedS_6(i__),b_FluxObsS_12(i__),
+ B_FluxObsS_13(i__),b2_FluxObsS_8(i__),B2_FluxObsS_9(i__),
+ FluxObsBFT_4(i__),FluxObsMedT_6(i__),b_FluxObsT_12(i__),
+ B_FluxObsT_13(i__),b2_FluxObsT_8(i__),B2_FluxObsT_9(i__),
+ FluxCBFS_3(i__),FluxCMedS_4(i__),b_FluxCS_8(i__),
+ B_FluxCS_9(i__),b2_FluxCS_6(i__),B2_FluxCS_7(i__),
+ FluxCBFT_3(i__),FluxCMedT_4(i__),b_FluxCT_8(i__),
+ B_FluxCT_9(i__),b2_FluxCT_6(i__),B2_FluxCT_7(i__),
+ FluxIBFS_3(i__),FluxIMedS_4(i__),b_FluxIS_8(i__),
+ B_FluxIS_9(i__),b2_FluxIS_6(i__),B2_FluxIS_7(i__),
+ FluxIBF2keV_3(i__),FluxIMed2keV_4(i__),b_FluxI2keV_8(i__),
+ B_FluxI2keV_9(i__),b2_FluxI2keV_6(i__),B2_FluxI2keV_7(i__),
+ LumIBFS_3(i__),LumIMedS_4(i__),b_LumIS_8(i__),B_LumIS_9(i__),
+ b2_LumIS_6(i__),B2_LumIS_7(i__),LumIBF2keV_3(i__),
+ LumIMed2keV_4(i__),b_LumI2keV_8(i__),B_LumI2keV_9(i__),
+ b2_LumI2keV_6(i__),B2_LumI2keV_7(i__),lognHMed_4(i__),
+ b_lognH_8(i__),B_lognH_9(i__),lognHMean_4(i__),s_lognH_4(i__),
+ logPowNMed_3(i__),b_logPowN_6(i__),B_logPowN_7(i__),
+ logPowNMean_3(i__),s_logPowN_3(i__),logBkgNMed_4(i__),
+ b_logBkgN_8(i__),B_logBkgN_9(i__),logBkgNMean_4(i__),
+ s_logBkgN_4(i__),logZ_4(i__)
c ..............Just test output...........
write(6,7)
+ ID_SRC_6(i__),z_4(i__),lognHKL_4(i__),b_lognHH_8(i__),
+ B_lognHH_9(i__),logPowNKL_3(i__),b_logPowNH_6(i__),
+ B_logPowNH_7(i__),lognHBF_4(i__),logPowNBF_3(i__),
+ FluxObsBFS_4(i__),FluxObsMedS_6(i__),b_FluxObsS_12(i__),
+ B_FluxObsS_13(i__),b2_FluxObsS_8(i__),B2_FluxObsS_9(i__),
+ FluxObsBFT_4(i__),FluxObsMedT_6(i__),b_FluxObsT_12(i__),
+ B_FluxObsT_13(i__),b2_FluxObsT_8(i__),B2_FluxObsT_9(i__),
+ FluxCBFS_3(i__),FluxCMedS_4(i__),b_FluxCS_8(i__),
+ B_FluxCS_9(i__),b2_FluxCS_6(i__),B2_FluxCS_7(i__),
+ FluxCBFT_3(i__),FluxCMedT_4(i__),b_FluxCT_8(i__),
+ B_FluxCT_9(i__),b2_FluxCT_6(i__),B2_FluxCT_7(i__),
+ FluxIBFS_3(i__),FluxIMedS_4(i__),b_FluxIS_8(i__),
+ B_FluxIS_9(i__),b2_FluxIS_6(i__),B2_FluxIS_7(i__),
+ FluxIBF2keV_3(i__),FluxIMed2keV_4(i__),b_FluxI2keV_8(i__),
+ B_FluxI2keV_9(i__),b2_FluxI2keV_6(i__),B2_FluxI2keV_7(i__),
+ LumIBFS_3(i__),LumIMedS_4(i__),b_LumIS_8(i__),B_LumIS_9(i__),
+ b2_LumIS_6(i__),B2_LumIS_7(i__),LumIBF2keV_3(i__),
+ LumIMed2keV_4(i__),b_LumI2keV_8(i__),B_LumI2keV_9(i__),
+ b2_LumI2keV_6(i__),B2_LumI2keV_7(i__),lognHMed_4(i__),
+ b_lognH_8(i__),B_lognH_9(i__),lognHMean_4(i__),s_lognH_4(i__),
+ logPowNMed_3(i__),b_logPowN_6(i__),B_logPowN_7(i__),
+ logPowNMean_3(i__),s_logPowN_3(i__),logBkgNMed_4(i__),
+ b_logBkgN_8(i__),B_logBkgN_9(i__),logBkgNMean_4(i__),
+ s_logBkgN_4(i__),logZ_4(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table8.dat' ! Shape-fixed-powerlaw results
C Format for file interpretation
8 format(
+ I5,1X,E9.2,1X,F10.8,1X,F10.7,1X,F10.7,1X,F10.7,1X,E11.6,1X,
+ E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,
+ 1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,
+ E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,
+ 1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,
+ E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,
+ 1X,E11.6,1X,E11.6,1X,F8.4,1X,F8.4,1X,F8.4,1X,F8.4,1X,F8.4,1X,
+ F8.4,1X,F8.4,1X,F8.4,1X,F8.4,1X,F8.4,1X,F8.4,1X,F8.4,1X,F10.7,
+ 1X,F10.7,1X,F10.7,1X,F10.7,1X,F12.10,1X,E15.9,1X,E15.8,1X,
+ E15.8,1X,E16.9,1X,F12.10,1X,F11.6)
C Effective file loading
open(unit=1,status='old',file=
+'table8.dat')
write(6,*) '....Loading file: table8.dat'
do i__=1,27910
read(1,'(A746)')ar__7
read(ar__7,8)
+ ID_SRC_7(i__),z_5(i__),logPowNKL_4(i__),b_logPowNH_8(i__),
+ B_logPowNH_9(i__),logPowNBF_4(i__),FluxObsBFS_5(i__),
+ FluxObsMedS_7(i__),b_FluxObsS_14(i__),B_FluxObsS_15(i__),
+ b2_FluxObsS_10(i__),B2_FluxObsS_11(i__),FluxObsBFT_5(i__),
+ FluxObsMedT_7(i__),b_FluxObsT_14(i__),B_FluxObsT_15(i__),
+ b2_FluxObsT_10(i__),B2_FluxObsT_11(i__),FluxCBFS_4(i__),
+ FluxCMedS_5(i__),b_FluxCS_10(i__),B_FluxCS_11(i__),
+ b2_FluxCS_8(i__),B2_FluxCS_9(i__),FluxCBFT_4(i__),
+ FluxCMedT_5(i__),b_FluxCT_10(i__),B_FluxCT_11(i__),
+ b2_FluxCT_8(i__),B2_FluxCT_9(i__),FluxIBFS_4(i__),
+ FluxIMedS_5(i__),b_FluxIS_10(i__),B_FluxIS_11(i__),
+ b2_FluxIS_8(i__),B2_FluxIS_9(i__),FluxIBF2keV_4(i__),
+ FluxIMed2keV_5(i__),b_FluxI2keV_10(i__),B_FluxI2keV_11(i__),
+ b2_FluxI2keV_8(i__),B2_FluxI2keV_9(i__),LumIBFS_4(i__),
+ LumIMedS_5(i__),b_LumIS_10(i__),B_LumIS_11(i__),
+ b2_LumI2S(i__),B2_LumIS_8(i__),LumIBF2keV_4(i__),
+ LumIMed2keV_5(i__),b_LumI2keV_10(i__),B_LumI2keV_11(i__),
+ b2_LumI2keV_8(i__),B2_LumI2keV_9(i__),logPowNMed_4(i__),
+ b_logPowN_8(i__),B_logPowN_9(i__),logPowNMean_4(i__),
+ s_logPowN_4(i__),logBkgNMed_5(i__),b_logBkgN_10(i__),
+ B_logBkgN_11(i__),logBkgNMean_5(i__),s_logBkgN_5(i__),
+ logZ_5(i__)
c ..............Just test output...........
write(6,8)
+ ID_SRC_7(i__),z_5(i__),logPowNKL_4(i__),b_logPowNH_8(i__),
+ B_logPowNH_9(i__),logPowNBF_4(i__),FluxObsBFS_5(i__),
+ FluxObsMedS_7(i__),b_FluxObsS_14(i__),B_FluxObsS_15(i__),
+ b2_FluxObsS_10(i__),B2_FluxObsS_11(i__),FluxObsBFT_5(i__),
+ FluxObsMedT_7(i__),b_FluxObsT_14(i__),B_FluxObsT_15(i__),
+ b2_FluxObsT_10(i__),B2_FluxObsT_11(i__),FluxCBFS_4(i__),
+ FluxCMedS_5(i__),b_FluxCS_10(i__),B_FluxCS_11(i__),
+ b2_FluxCS_8(i__),B2_FluxCS_9(i__),FluxCBFT_4(i__),
+ FluxCMedT_5(i__),b_FluxCT_10(i__),B_FluxCT_11(i__),
+ b2_FluxCT_8(i__),B2_FluxCT_9(i__),FluxIBFS_4(i__),
+ FluxIMedS_5(i__),b_FluxIS_10(i__),B_FluxIS_11(i__),
+ b2_FluxIS_8(i__),B2_FluxIS_9(i__),FluxIBF2keV_4(i__),
+ FluxIMed2keV_5(i__),b_FluxI2keV_10(i__),B_FluxI2keV_11(i__),
+ b2_FluxI2keV_8(i__),B2_FluxI2keV_9(i__),LumIBFS_4(i__),
+ LumIMedS_5(i__),b_LumIS_10(i__),B_LumIS_11(i__),
+ b2_LumI2S(i__),B2_LumIS_8(i__),LumIBF2keV_4(i__),
+ LumIMed2keV_5(i__),b_LumI2keV_10(i__),B_LumI2keV_11(i__),
+ b2_LumI2keV_8(i__),B2_LumI2keV_9(i__),logPowNMed_4(i__),
+ b_logPowN_8(i__),B_logPowN_9(i__),logPowNMean_4(i__),
+ s_logPowN_4(i__),logBkgNMed_5(i__),b_logBkgN_10(i__),
+ B_logBkgN_11(i__),logBkgNMean_5(i__),s_logBkgN_5(i__),
+ logZ_5(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table9.dat' ! Soft-band fitting results
C Format for file interpretation
9 format(
+ I5,1X,E9.2,1X,F12.9,1X,F10.8,1X,F9.7,1X,F11.9,1X,F9.6,1X,F9.6,
+ 1X,F11.9,1X,F11.8,1X,F13.10,1X,F11.8,1X,F9.6,1X,E15.8,1X,
+ E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,F10.8,
+ 1X,F10.8,1X,F9.7,1X,F9.7,1X,F11.9,1X,F9.6,1X,F9.6,1X,F9.6,1X,
+ F9.6,1X,F11.9,1X,F11.8,1X,F11.8,1X,F12.9,1X,F11.8,1X,F12.10,
+ 1X,E16.9,1X,E15.8,1X,E16.9,1X,E15.8,1X,F12.10,1X,F12.7)
C Effective file loading
open(unit=1,status='old',file=
+'table9.dat')
write(6,*) '....Loading file: table9.dat'
do i__=1,27910
read(1,'(A489)')ar__8
read(ar__8,9)
+ ID_SRC_8(i__),z_6(i__),GammaKL_3(i__),b_GammaH_6(i__),
+ B_GammaH_7(i__),lognHKL_5(i__),b_lognHH_10(i__),
+ B_lognHH_11(i__),logPowNKL_5(i__),b_logPowNH_10(i__),
+ B_logPowNH_11(i__),GammaBF_3(i__),lognHBF_5(i__),
+ logPowNBF_5(i__),FluxObsBFS_6(i__),FluxObsMedS_8(i__),
+ b_FluxObsS_16(i__),B_FluxObsS_17(i__),b2_FluxObsS_12(i__),
+ B2_FluxObsS_13(i__),GammaMed_3(i__),b_Gamma_6(i__),
+ B_Gamma_7(i__),GammaMean_3(i__),s_Gamma_3(i__),
+ lognHMed_5(i__),b_lognH_10(i__),B_lognH_11(i__),
+ lognHMean_5(i__),s_lognH_5(i__),logPowNMed_5(i__),
+ b_logPowN_10(i__),B_logPowN_11(i__),logPowNMean_5(i__),
+ s_logPowN_5(i__),logBkgNMed_6(i__),blogBkgN(i__),
+ BlogBkgN_1(i__),logBkgNMean_6(i__),logBkgN(i__),logZ_6(i__)
c ..............Just test output...........
write(6,9)
+ ID_SRC_8(i__),z_6(i__),GammaKL_3(i__),b_GammaH_6(i__),
+ B_GammaH_7(i__),lognHKL_5(i__),b_lognHH_10(i__),
+ B_lognHH_11(i__),logPowNKL_5(i__),b_logPowNH_10(i__),
+ B_logPowNH_11(i__),GammaBF_3(i__),lognHBF_5(i__),
+ logPowNBF_5(i__),FluxObsBFS_6(i__),FluxObsMedS_8(i__),
+ b_FluxObsS_16(i__),B_FluxObsS_17(i__),b2_FluxObsS_12(i__),
+ B2_FluxObsS_13(i__),GammaMed_3(i__),b_Gamma_6(i__),
+ B_Gamma_7(i__),GammaMean_3(i__),s_Gamma_3(i__),
+ lognHMed_5(i__),b_lognH_10(i__),B_lognH_11(i__),
+ lognHMean_5(i__),s_lognH_5(i__),logPowNMed_5(i__),
+ b_logPowN_10(i__),B_logPowN_11(i__),logPowNMean_5(i__),
+ s_logPowN_5(i__),logBkgNMed_6(i__),blogBkgN(i__),
+ BlogBkgN_1(i__),logBkgNMean_6(i__),logBkgN(i__),logZ_6(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table10.dat' ! Hard-band fitting results
C Format for file interpretation
10 format(
+ I5,1X,E9.2,1X,F11.9,1X,F9.7,1X,F9.7,1X,F12.10,1X,F9.6,1X,F9.6,
+ 1X,F11.9,1X,F10.7,1X,F12.9,1X,F11.8,1X,F9.6,1X,F13.10,1X,
+ E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,
+ 1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,E11.6,1X,F9.7,1X,F9.7,
+ 1X,F9.7,1X,F9.7,1X,F10.8,1X,F9.6,1X,F9.6,1X,F9.6,1X,F9.6,1X,
+ F10.8,1X,F10.7,1X,F10.7,1X,F11.8,1X,F10.7,1X,F10.8,1X,E15.9,
+ 1X,E15.8,1X,E15.8,1X,E15.8,1X,F12.10,1X,F11.7)
C Effective file loading
open(unit=1,status='old',file=
+'table10.dat')
write(6,*) '....Loading file: table10.dat'
do i__=1,27910
read(1,'(A543)')ar__9
read(ar__9,10)
+ ID_SRC_9(i__),z_7(i__),GammaKL_4(i__),e_Gamma(i__),
+ E_Gamma_1(i__),lognHKL_6(i__),b_lognH_12(i__),B_lognH_13(i__),
+ logPowNKL_6(i__),b_logPowN_12(i__),B_logPowN_13(i__),
+ GammaBF_4(i__),lognHBF_6(i__),logPowNBF_6(i__),
+ FluxObsBFT_6(i__),FluxObsMedT_8(i__),b_FluxObsT_16(i__),
+ B_FluxObsT_17(i__),b2_FluxObsT_12(i__),B2_FluxObsT_13(i__),
+ FluxCBFT_5(i__),FluxCMedT_6(i__),b_FluxCMedT(i__),
+ B_FluxCMedT_1(i__),b2_FluxCMedT(i__),B2_FluxCMedT_1(i__),
+ GammaMed_4(i__),b_GammaMed(i__),B_GammaMed_1(i__),
+ GammaMean_4(i__),s_Gamma_4(i__),lognHMed_6(i__),
+ b_lognHMed(i__),B_lognHMed_1(i__),lognHMean_6(i__),
+ s_lognH_6(i__),logPowNMed_6(i__),b_logPowNMed(i__),
+ B_logPowNMed_1(i__),logPowNMean_6(i__),s_logPowN_6(i__),
+ logBkgNMed_7(i__),b_logBkgNMed(i__),B_logBkgNMed_1(i__),
+ logBkgNMean_7(i__),s_logBkgN_6(i__),logZ_7(i__)
c ..............Just test output...........
write(6,10)
+ ID_SRC_9(i__),z_7(i__),GammaKL_4(i__),e_Gamma(i__),
+ E_Gamma_1(i__),lognHKL_6(i__),b_lognH_12(i__),B_lognH_13(i__),
+ logPowNKL_6(i__),b_logPowN_12(i__),B_logPowN_13(i__),
+ GammaBF_4(i__),lognHBF_6(i__),logPowNBF_6(i__),
+ FluxObsBFT_6(i__),FluxObsMedT_8(i__),b_FluxObsT_16(i__),
+ B_FluxObsT_17(i__),b2_FluxObsT_12(i__),B2_FluxObsT_13(i__),
+ FluxCBFT_5(i__),FluxCMedT_6(i__),b_FluxCMedT(i__),
+ B_FluxCMedT_1(i__),b2_FluxCMedT(i__),B2_FluxCMedT_1(i__),
+ GammaMed_4(i__),b_GammaMed(i__),B_GammaMed_1(i__),
+ GammaMean_4(i__),s_Gamma_4(i__),lognHMed_6(i__),
+ b_lognHMed(i__),B_lognHMed_1(i__),lognHMean_6(i__),
+ s_lognH_6(i__),logPowNMed_6(i__),b_logPowNMed(i__),
+ B_logPowNMed_1(i__),logPowNMean_6(i__),s_logPowN_6(i__),
+ logBkgNMed_7(i__),b_logBkgNMed(i__),B_logBkgNMed_1(i__),
+ logBkgNMean_7(i__),s_logBkgN_6(i__),logZ_7(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end