Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJS/192/10 into FORTRAN code for reading data files line by line.
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-Oct-14
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/ApJS/192/10 Chandra ACIS survey in 383 nearby galaxies. I. (Liu, 2011)
*================================================================================
*Chandra ACIS survey of X-ray point sources in 383 nearby galaxies.
*I. The source catalog.
* Liu J.
* <Astrophys. J. Suppl. Ser., 192, 10 (2011)>
* =2011ApJS..192...10L
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Properties of surveyed galaxies
integer*4 nr__
parameter (nr__=391) ! Number of records
character*123 ar__ ! Full-size record
C Position composed of: GLON GLAT
character*8 Gal ! Galaxy name (NGC, IC or PGC)
character*9 r_Gal ! Galaxy reference(s) (1)
real*4 GLON ! (deg) Galactic longitude of the galaxy
real*4 GLAT ! (deg) Galactic latitude of the galaxy
real*4 R25 ! (arcmin) Semimajor axis of the D_25_ isophotal ellipsis
real*4 r25_1 ! (arcmin) Semiminor axis of the D_25_ isophotal
* ellipsis
real*4 nH ! (cm-2) Galactic HI column density (2)
real*8 Dist ! (Mpc) Distance
character*3 r_Dist ! Distance reference; see refs.dat file
character*10 MType ! Morphological type from RC3 (3)
real*4 TT ! ? Hubble type T of galaxies taken from RC3
real*4 LB ! (Lsun) ? Blue luminosity (4)
character*1 l_F60um ! Limit flag on F60um
real*4 F60um ! (Jy) ? 60um flux density from IRAS (5)
integer*4 Group ! [1/320]? Group number as in table 2
real*4 Flim ! (10-7W) 0.3-8keV flux of the faintest X-ray source
* in this galaxy
character*11 Class ! NED classification (6)
*Note (1): Point source catalogs of 50 galaxies are present in the VizieR
* service; see refs.dat file.
*Note (2): taken from the dust map by Dickey & Lockman (1990)
*Note (3): In the type code S stands for spiral, E for elliptical, S0 for
* lenticular, I for irregular; (r) for inner ring, (s) for S-shaped,
* (rs) for mixed; B for barred, A for non-barred, AB for mixed; Im for
* Magellanic irregular, I0 for non-Magellanic irregular; the trailing
* -/o/+ for early/intermediate/late stage, etc. The detailed
* explanations can be found in the RC3 catalog (p. 15, Vol. I).
*Note (4): The blue luminosity calculated from the apparent blue magnitude
* taken from RC3. The luminosity is expressed in unit of solar
* luminosity assuming an absolute blue magnitude of 5.47 for the Sun.
*Note (5): The flux density at 60um taken from the IRAS point source catalog
* (IPAC, 1986), with some nearby galaxies from Rice et al. (1988). When
* the galaxy is below detection, the 3{sigma} upper limit is calculated
* by adopting noise levels of 8.5mJy/arcmin^2^ for 60um (Rice et al. 1988).
*Note (6): Whether the galaxy is an HII/starburst/LINER/Seyfert galaxy, as
* extracted from the NED classification.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Groups of surveyed galaxies and ACIS observations
integer*4 nr__1
parameter (nr__1=667) ! Number of records
character*74 ar__1 ! Full-size record
integer*4 Group_1 ! [1/320] Group number
character*8 Gal_1 ! Galaxy name
integer*4 Nobs ! Number of observations
integer*4 ExpTot ! (s) Total exposure time
integer*4 ObsID ! Observation number
character*10 ObsDate ! ("YYYY/MM/DD") Observation date
real*8 MJD ! (d) Modified Julian Date of observation
integer*4 Exp ! (s) ? Exposure time
character*7 Chip ! Chips used for analysis
real*4 Bkgd ! ? Average background (1)
integer*4 Npt ! ? Total number of point sources detected
*Note (1): The average background for the on-axis chip in unit of photons
* per 100 pixels, computed using 0.1-8keV photons outside three times
* of the source regions of detected sources.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! Individual observations of X-ray sources
integer*4 nr__2
parameter (nr__2=52542) ! Number of records
character*164 ar__2 ! Full-size record
integer*4 Group_2 ! [1/320] Group number
character*21 CXO ! Source name (JHHMMSS.sss+DDMMSS.ss) (1)
character*18 IDet ! Individual detection designation (2)
integer*4 Exp_1 ! (s) Exposure time after deadtime correction
real*8 MJD_1 ! (d) Modified Julian Date of observation
integer*4 OAA ! (arcsec) Off-axis angle
real*4 VigF ! Vignetting factor (3)
real*4 eRA ! (arcsec) ? Right Ascension statistical positional error
real*4 eDE ! (arcsec) ? Declination statistical positional error
real*4 ePos ! (arcsec) ? Source positional uncertainty (4)
real*4 Sigma ! Detection significance (5)
real*8 Cts ! (ct) Background-subtracted photon counts (6)
real*4 e_Cts ! (ct) Uncertainty in Cts
real*8 bgct ! (ct) ? Expected background counts (7)
real*4 CMS ! ? The (M-S)/(H+M+S) X-ray color (8)
real*4 e_CMS ! ? Uncertainty in CMS
real*4 CHM ! ? The (H-M)/(H+M+S) X-ray color (8)
real*4 e_CHM ! ? Uncertainty in CHM
real*4 FX ! (mW/m2) Source flux; in erg/s/cm^2^ (9)
real*4 PKS ! ? Kolmogorov-Smirnov variability probability (10)
character*4 SQH ! Source description (11)
*Note (1): Composed from their positions following CXO naming conventions.
*Note (2): In the form of IIIi.ss.nn, with IIIi as the observation ID, ss as
* the CCD chip, and nn as the source number from wavdetect (nn=u if the
* source was not detected in an observation). Enclosed in parenthesis is
* the split fraction, which is less than unity if the source is a split
* component of a merged source in an observation.
*Note (3): Derived from the exposure map as the ratio between the local and
* the maximum map value.
*Note (4): Computed from the scheme of Kim et al. (2004, Cat. J/ApJS/150/19).
*Note (5): From wavdetect. For the upper limit, it is computed as
* (net count)/(count error) and prefixed with a minus sign.
*Note (6): From wavdetect or computed from a circular region equivalent to
* the PSF enclosing 95% of the energy at 1.5keV for the upper limit.
*Note (7): Within the source region as computed in Section 3.2 for detected
* sources.
*Note (8): H/M/S stands for background-subtracted photon counts in hard
* (2-8keV), medium (1-2keV) and soft (0.3-1keV) bands.
*Note (9): Computed from the vignetting corrected count rate in 0.3-8keV
* assuming a power law of {Gamma}=1.7 and Galactic n_H_ absorption.
*Note (10): Probability that a source is constant within an observation. A
* source is considered as variable if PKS<0.01.
*Note (11): Sources as follows:
* SSS = supersoft;
* QSS = quasi-soft;
* hard = hard phase;
* dim = too dim, i.e. below 10 counts.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table4.dat' ! X-ray point sources in nearby galaxies
integer*4 nr__3
parameter (nr__3=17559) ! Number of records
character*164 ar__3 ! Full-size record
integer*4 Group_3 ! [1/320] Group number
character*21 CXO_1 ! Source name (JHHMMSS.sss+DDMMSS.ss) (1)
real*4 ePos_1 ! (arcsec) Source positional uncertainty (2)
character*12 Name ! Galatic source name (3)
real*4 alpha ! (arcmin) ? Galactic source nuclear separation
real*4 r25_2 ! ? Galactic source nuclear separation (4)
real*8 Dist_1 ! (Mpc) Distance to source
character*5 V_D ! Ratio of time source was observed to detected
real*4 LX ! (10-7W) Maximum computed luminosity; in erg/s
real*4 FX_1 ! (mW/m2) Average computed X-ray flux; in erg/s/cm^2^
real*4 F_F ! The F_max_/F_min_ flux ratio (5)
real*8 E_F_F ! ? Positive error in F/F
real*8 e_F_F_1 ! ? Negative error in F/F
real*8 Sigmax ! Maximum detection significance
real*8 Cmax ! Maximum photon counts from detections
character*12 SQH_1 ! Phase statistics (6)
character*4 PKS_1 ! K-S criterion variability statistics (7)
character*10 Note ! Source identification (8)
*Note (1): Composed from their positions following CXO naming conventions.
*Note (2): Computed from the scheme of Kim et al. (2004, Cat. J/ApJS/150/19).
*Note (3): Numbered sequentially by its maximum detection significance.
*Note (4): In units of the elliptical radius.
*Note (5): As a variability indicator. F_max_ is the maximum 0.3-8keV flux
* from all detections and F_min_ is the minimum flux from all detections
* and upper limits. The ratio is unity without errors if F_max_ and
* F_min_ are the same.
*Note (6): Statistics for supersoft/quasisoft/hard/dim phases. For example,
* s2 means supersoft in two observations, q3 means quasisoft in three
* observations, h4 means hard in four observations, and d1 means too dim
* (below 10 counts) in one observations.
*Note (7): Statistics for variability within single observations by the K-S
* criterion. For example, v/3 means the source was variable by the K-S
* criterion (i.e., P_KS_<0.01, more than 10 counts, and the background
* fraction is <10%) in three observations.
*Note (8): Sources as follows:
* ULX = ultraluminous X-ray source;
* ULS = ultraluminous supersoft source;
* NGC3031 = the galactic nucleus for NGC1313.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table5.dat' ! X-ray identifications for galactic nuclei of
nearby galaxies
integer*4 nr__4
parameter (nr__4=391) ! Number of records
character*104 ar__4 ! Full-size record
integer*4 Group_4 ! [1/320] Group number
character*8 Gal_2 ! Galaxy name
integer*4 N6 ! ? Number of X-ray sources within 6" of the
* galactic nucleus
integer*4 N12 ! ? Number of X-ray sources within 12" of the
* galactic nucleus
integer*4 Nf ! ? Number of HST images in different filters
* available for the galactic nuclei region
character*24 XID ! CXO counterpart
integer*4 pos ! ? Position flag (1)
integer*4 ext ! ? X-ray source extendness flag (2)
integer*4 V ! Numbers the source was observed
integer*4 D ! Numbers the source was detected
real*4 LXmax ! (10-7W) Maximum X-ray luminosity in 0.3-8keV among all
* detections
real*4 LXmin ! (10-7W) ? Minimum X-ray luminosity in 0.3-8keV among
* all detections
real*8 CntMax ! (ct) ? Maximum X-ray photon counts among all
* detections
real*8 Sigmax_1 ! ? Maximum detection sigma among all detections
character*12 SQH_2 ! Statistics for supersoft/quasi-soft/hard/dim
* phases (3)
*Note (1): Position flag as follows:
* 1 = the X-ray and optical positions align up within the X-ray positional
* error,
* 2 = offset in excess of the X-ray positional error presents when there is
* a clear optical nucleus from DSS or HST images;
* 3 = alignment
* 4 = misalignment when the optical nucleus is extended.
*Note (2): X-ray source extendness flag as follows:
* 1 = perfect point source,
* 2 = there is slight extended emission,
* 3 = extended emission is moderate,
* 4 = the source is dominantly extended emission.
*Note (3): For example, s2 means supersoft in two observations, q3 means
* quasi-soft in three observations, h4 means hard in four observations,
* and d1 means too dim (below 10 counts) in one observations.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table6.dat' ! Ultraluminous X-ray sources in nearby galaxies
integer*4 nr__5
parameter (nr__5=480) ! Number of records
character*157 ar__5 ! Full-size record
integer*4 Group_5 ! [1/320] Group number
character*22 CXO_2 ! CXO designation (JHHMMSS.sss+DDMMSS.ss)
real*4 ePos_2 ! (arcsec) Source positional uncertainties computed from
* the scheme of Kim et al. (2004)
character*12 Name_1 ! Galactic source name (1)
real*4 alpha_1 ! (arcmin) Galactic source nuclear separation
real*4 r25_3 ! Galactic source nuclear separation in unit
* of the elliptical radius
real*8 Dist_2 ! (Mpc) Distance for the source
integer*4 V_1 ! Numbers the source was observed
integer*4 D_1 ! Numbers the source was detected
real*4 LXmax_1 ! (10-7W) Maximum luminosity in erg/s computed from
* detections
real*4 FX_2 ! (10-3W/m2) Average flux in erg/s/cm^2^ computed from
* detections
real*4 F_F_1 ! F_max_/F_min_ ratio as a variability
* indicator (2)
real*4 E_F_F_2 ! ? Positive error in F/F
real*4 e_F_F_3 ! ? Negative error in F/F
real*8 Sigmax_2 ! The maximum detection significance
real*8 Cmax_1 ! The maximum photon counts from detections
character*12 SQH_3 ! Statistics for supersoft/quasi-soft/hard/dim
* phases (3)
character*3 PKS_2 ! K-S criterion variability (4)
character*8 Notes ! Source identification (ULX/ULS)
*Note (1): numbered sequentially by its maximum detection significance.
*Note (2): F_max_ is the maximum 0.3-8keV flux from all detections, and
* F_min_ is the minimum flux from all detections and upper limits. The
* ratio is unity without errors if F_max_ and F_min_ are the same.
*Note (3): For example, s2 means supersoft in two observations, q3 means
* quasi-soft in three observations, h4 means hard in four observations,
* and d1 means too dim (below 10 counts) in one observations.
*Note (4): Statistics for variability within single observations by the K-S
* criterion. For example, v:3 means the source was variable by the K-S
* criterion (i.e., PK-S<0.01, more than 10 counts, and the background
* fraction is <10%) in three observations.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table7.dat' ! Ultraluminous supersoft X-ray sources in nearby
galaxies
integer*4 nr__6
parameter (nr__6=70) ! Number of records
character*157 ar__6 ! Full-size record
integer*4 Group_6 ! [1/320] Group number
character*22 CXO_3 ! CXO designation (JHHMMSS.sss+DDMMSS.ss)
real*4 ePos_3 ! (arcsec) Source positional uncertainties computed from
* the scheme of Kim et al. (2004)
character*12 Name_2 ! Galactic source name (1)
real*4 alpha_2 ! (arcmin) Galactic source nuclear separation
real*4 r25_4 ! Galactic source nuclear separation in unit
* of the elliptical radius
real*8 Dist_3 ! (Mpc) Distance for the source
integer*4 V_2 ! Numbers the source was observed
integer*4 D_2 ! Numbers the source was detected
real*4 LXmax_2 ! (10-7W) Maximum luminosity in erg/s computed from
* detections
real*4 FX_3 ! (10-3W/m2) Average flux in erg/s/cm^2^ computed from
* detections
real*4 F_F_2 ! F_max_/F_min_ ratio as a variability
* indicator (2)
real*4 E_F_F_4 ! ? Positive error in F/F
real*4 e_F_F_5 ! ? Negative error in F/F
real*8 Sigmax_3 ! The maximum detection significance
real*8 Cmax_2 ! The maximum photon counts from detections
character*12 SQH_4 ! Statistics for supersoft/quasi-soft/hard/dim
* phases (3)
character*3 PKS_3 ! K-S criterion variability (4)
character*8 Notes_1 ! Source identification (ULX/ULS)
*Note (1): numbered sequentially by its maximum detection significance.
*Note (2): F_max_ is the maximum 0.3-8keV flux from all detections, and
* F_min_ is the minimum flux from all detections and upper limits. The
* ratio is unity without errors if F_max_ and F_min_ are the same.
*Note (3): For example, s2 means supersoft in two observations, q3 means
* quasi-soft in three observations, h4 means hard in four observations,
* and d1 means too dim (below 10 counts) in one observations.
*Note (4): Statistics for variability within single observations by the K-S
* criterion. For example, v:3 means the source was variable by the K-S
* criterion (i.e., PK-S<0.01, more than 10 counts, and the background
* fraction is <10%) in three observations.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'refs.dat' ! References for table 1
integer*4 nr__7
parameter (nr__7=32) ! Number of records
character*116 ar__7 ! Full-size record
character*3 Ref ! Reference code
character*19 BibCode ! Bibcode
character*18 Aut ! Author's name
character*73 Note_1 ! Comment or catalog reference in VizieR
C=============================================================================
C Loading file 'table1.dat' ! Properties of surveyed galaxies
C Format for file interpretation
1 format(
+ A8,1X,A9,1X,F6.2,1X,F6.2,1X,F5.2,1X,F5.2,1X,E8.3,1X,F7.4,1X,
+ A3,1X,A10,1X,F4.1,1X,E7.2,1X,A1,E8.2,1X,I3,1X,E7.2,1X,A11)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,391
read(1,'(A123)')ar__
read(ar__,1)
+ Gal,r_Gal,GLON,GLAT,R25,r25_1,nH,Dist,r_Dist,MType,TT,LB,
+ l_F60um,F60um,Group,Flim,Class
if(ar__(78:81) .EQ. '') TT = rNULL__
if(ar__(83:89) .EQ. '') LB = rNULL__
if(ar__(92:99) .EQ. '') F60um = rNULL__
if(ar__(101:103) .EQ. '') Group = iNULL__
c ..............Just test output...........
write(6,1)
+ Gal,r_Gal,GLON,GLAT,R25,r25_1,nH,Dist,r_Dist,MType,TT,LB,
+ l_F60um,F60um,Group,Flim,Class
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table2.dat' ! Groups of surveyed galaxies and ACIS observations
C Format for file interpretation
2 format(
+ I3,1X,A8,1X,I2,1X,I7,1X,I4,1X,A10,1X,F9.3,1X,I6,1X,A7,1X,F5.2,
+ 1X,I3)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,667
read(1,'(A74)')ar__1
read(ar__1,2)
+ Group_1,Gal_1,Nobs,ExpTot,ObsID,ObsDate,MJD,Exp,Chip,Bkgd,Npt
if(ar__1(51:56) .EQ. '') Exp = iNULL__
if(ar__1(66:70) .EQ. '') Bkgd = rNULL__
if(ar__1(72:74) .EQ. '') Npt = iNULL__
c ..............Just test output...........
write(6,2)
+ Group_1,Gal_1,Nobs,ExpTot,ObsID,ObsDate,MJD,Exp,Chip,Bkgd,Npt
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table3.dat' ! Individual observations of X-ray sources
C Format for file interpretation
3 format(
+ I3,4X,A21,1X,A18,1X,I6,1X,F9.3,1X,I3,1X,F5.3,1X,F4.2,1X,F4.2,
+ 1X,F4.1,1X,F6.1,1X,F7.1,1X,F5.1,1X,F7.1,1X,F5.2,1X,F4.2,1X,
+ F5.2,1X,F4.2,1X,E8.2,1X,E9.2,1X,A4)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,52542
read(1,'(A164)')ar__2
read(ar__2,3)
+ Group_2,CXO,IDet,Exp_1,MJD_1,OAA,VigF,eRA,eDE,ePos,Sigma,Cts,
+ e_Cts,bgct,CMS,e_CMS,CHM,e_CHM,FX,PKS,SQH
if(ar__2(76:79) .EQ. '') eRA = rNULL__
if(ar__2(81:84) .EQ. '') eDE = rNULL__
if(ar__2(86:89) .EQ. '') ePos = rNULL__
if(ar__2(112:118) .EQ. '') bgct = rNULL__
if(ar__2(120:124) .EQ. '') CMS = rNULL__
if(ar__2(126:129) .EQ. '') e_CMS = rNULL__
if(ar__2(131:135) .EQ. '') CHM = rNULL__
if(ar__2(137:140) .EQ. '') e_CHM = rNULL__
if(ar__2(151:159) .EQ. '') PKS = rNULL__
c ..............Just test output...........
write(6,3)
+ Group_2,CXO,IDet,Exp_1,MJD_1,OAA,VigF,eRA,eDE,ePos,Sigma,Cts,
+ e_Cts,bgct,CMS,e_CMS,CHM,e_CHM,FX,PKS,SQH
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table4.dat' ! X-ray point sources in nearby galaxies
C Format for file interpretation
4 format(
+ I3,4X,A21,1X,F5.2,1X,A12,1X,F6.3,1X,F4.2,1X,F8.4,1X,A5,1X,
+ E9.4,1X,E8.3,1X,F6.1,1X,F7.3,1X,F7.3,1X,F8.3,1X,F9.3,1X,A12,
+ 1X,A4,1X,A10)
C Effective file loading
open(unit=1,status='old',file=
+'table4.dat')
write(6,*) '....Loading file: table4.dat'
do i__=1,17559
read(1,'(A164)')ar__3
read(ar__3,4)
+ Group_3,CXO_1,ePos_1,Name,alpha,r25_2,Dist_1,V_D,LX,FX_1,F_F,
+ E_F_F,e_F_F_1,Sigmax,Cmax,SQH_1,PKS_1,Note
if(ar__3(49:54) .EQ. '') alpha = rNULL__
if(ar__3(56:59) .EQ. '') r25_2 = rNULL__
if(ar__3(102:108) .EQ. '') E_F_F = rNULL__
if(ar__3(110:116) .EQ. '') e_F_F_1 = rNULL__
c ..............Just test output...........
write(6,4)
+ Group_3,CXO_1,ePos_1,Name,alpha,r25_2,Dist_1,V_D,LX,FX_1,F_F,
+ E_F_F,e_F_F_1,Sigmax,Cmax,SQH_1,PKS_1,Note
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table5.dat' ! X-ray identifications for galactic nuclei of
* nearby galaxies
C Format for file interpretation
5 format(
+ I3,1X,A8,1X,I1,1X,I2,1X,I2,1X,A24,1X,I1,1X,I1,1X,I2,1X,I2,1X,
+ E9.4,1X,E8.3,1X,F8.2,1X,F7.2,1X,A12)
C Effective file loading
open(unit=1,status='old',file=
+'table5.dat')
write(6,*) '....Loading file: table5.dat'
do i__=1,391
read(1,'(A104)')ar__4
read(ar__4,5)
+ Group_4,Gal_2,N6,N12,Nf,XID,pos,ext,V,D,LXmax,LXmin,CntMax,
+ Sigmax_1,SQH_2
if(ar__4(14:14) .EQ. '') N6 = iNULL__
if(ar__4(16:17) .EQ. '') N12 = iNULL__
if(ar__4(19:20) .EQ. '') Nf = iNULL__
if(ar__4(47:47) .EQ. '') pos = iNULL__
if(ar__4(49:49) .EQ. '') ext = iNULL__
if(ar__4(67:74) .EQ. '') LXmin = rNULL__
if(ar__4(76:83) .EQ. '') CntMax = rNULL__
if(ar__4(85:91) .EQ. '') Sigmax_1 = rNULL__
c ..............Just test output...........
write(6,5)
+ Group_4,Gal_2,N6,N12,Nf,XID,pos,ext,V,D,LXmax,LXmin,CntMax,
+ Sigmax_1,SQH_2
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table6.dat' ! Ultraluminous X-ray sources in nearby galaxies
C Format for file interpretation
6 format(
+ I3,4X,A22,F4.2,1X,A12,1X,F6.3,1X,F4.2,1X,F7.3,1X,I2,1X,I2,1X,
+ E8.3,1X,E8.3,1X,F6.1,1X,F6.3,1X,F6.3,1X,F9.4,1X,F9.3,1X,A12,
+ 1X,A3,1X,A8)
C Effective file loading
open(unit=1,status='old',file=
+'table6.dat')
write(6,*) '....Loading file: table6.dat'
do i__=1,480
read(1,'(A157)')ar__5
read(ar__5,6)
+ Group_5,CXO_2,ePos_2,Name_1,alpha_1,r25_3,Dist_2,V_1,D_1,
+ LXmax_1,FX_2,F_F_1,E_F_F_2,e_F_F_3,Sigmax_2,Cmax_1,SQH_3,
+ PKS_2,Notes
if(ar__5(99:104) .EQ. '') E_F_F_2 = rNULL__
if(ar__5(106:111) .EQ. '') e_F_F_3 = rNULL__
c ..............Just test output...........
write(6,6)
+ Group_5,CXO_2,ePos_2,Name_1,alpha_1,r25_3,Dist_2,V_1,D_1,
+ LXmax_1,FX_2,F_F_1,E_F_F_2,e_F_F_3,Sigmax_2,Cmax_1,SQH_3,
+ PKS_2,Notes
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table7.dat' ! Ultraluminous supersoft X-ray sources in nearby
* galaxies
C Format for file interpretation
7 format(
+ I3,4X,A22,F4.2,1X,A12,1X,F6.3,1X,F4.2,1X,F7.3,1X,I2,1X,I2,1X,
+ E8.3,1X,E8.3,1X,F6.1,1X,F6.3,1X,F6.3,1X,F9.4,1X,F9.3,1X,A12,
+ 1X,A3,1X,A8)
C Effective file loading
open(unit=1,status='old',file=
+'table7.dat')
write(6,*) '....Loading file: table7.dat'
do i__=1,70
read(1,'(A157)')ar__6
read(ar__6,7)
+ Group_6,CXO_3,ePos_3,Name_2,alpha_2,r25_4,Dist_3,V_2,D_2,
+ LXmax_2,FX_3,F_F_2,E_F_F_4,e_F_F_5,Sigmax_3,Cmax_2,SQH_4,
+ PKS_3,Notes_1
if(ar__6(99:104) .EQ. '') E_F_F_4 = rNULL__
if(ar__6(106:111) .EQ. '') e_F_F_5 = rNULL__
c ..............Just test output...........
write(6,7)
+ Group_6,CXO_3,ePos_3,Name_2,alpha_2,r25_4,Dist_3,V_2,D_2,
+ LXmax_2,FX_3,F_F_2,E_F_F_4,e_F_F_5,Sigmax_3,Cmax_2,SQH_4,
+ PKS_3,Notes_1
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'refs.dat' ! References for table 1
C Format for file interpretation
8 format(A3,1X,A19,1X,A18,1X,A73)
C Effective file loading
open(unit=1,status='old',file=
+'refs.dat')
write(6,*) '....Loading file: refs.dat'
do i__=1,32
read(1,'(A116)')ar__7
read(ar__7,8)Ref,BibCode,Aut,Note_1
c ..............Just test output...........
write(6,8)Ref,BibCode,Aut,Note_1
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end