Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/889/80 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-Oct-10
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/ApJ/889/80 STUDIES. III. SCUBA-2 450um gal. with MIPS & VLA obs. (Lim+, 2020)
*================================================================================
*SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES).
*III. Multiwavelength properties, luminosity functions, and preliminary source
*catalog of 450 {mu}m selected galaxies.
* Lim C.-F., Wang W.-H., Smail I., Scott D., Chen C.-C., Chang Y.-Y.,
* Simpson J.M., Toba Y., Shu X., Clements D., Greenslade J., Ao Y., Babul A.,
* Birkin J., Chapman S.C., Cheng T.-A., Cho B.S., Dannerbauer H.,
* Dudzeviciute U., Dunlop J., Gao Y., Goto T., Ho L.C., Hsu L.-T.,
* Hwang H.S., Jeong W.-S., Koprowski M., Lee C.-H., Lin M.-Y., Lin W.-C.,
* Michalowski M.J., Parsons H., Sawicki M., Shirley R., Shim H., Urquhart S.,
* Wang J., Wang T.
* <Astrophys. J., 889, 80-80 (2020)>
* =2020ApJ...889...80L (SIMBAD/NED BibCode)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Derived properties of VLA 3-GHz
identified 450-um sources
integer*4 nr__
parameter (nr__=134) ! Number of records
character*142 ar__ ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg (nr__) ! (deg) Right Ascension J2000
real*8 DEdeg (nr__) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 RAh (nr__) ! (h) [9/10] 450um Hour of Right Ascension (J2000)
* (G1)
integer*4 RAm (nr__) ! (min) 450um Minute of Right Ascension (J2000) (G1)
real*4 RAs (nr__) ! (s) 450um Second of Right Ascension (J2000) (G1)
character*1 DE_ (nr__) ! [+] 450um Sign of Declination (J2000) (G1)
integer*4 DEd (nr__) ! (deg) [2] 450um Degree of Declination (J2000) (G1)
integer*4 DEm (nr__) ! (arcmin) [12/33] 450um Arcminute of Declination (J2000)
* (G1)
real*4 DEs (nr__) ! (arcsec) 450um Arcsecond of Declination (J2000) (G1)
integer*4 RACh (nr__) ! (h) Hour of Right Ascension (J2000) (1)
integer*4 RACm (nr__) ! (min) Minute of Right Ascension (J2000) (1)
real*4 RACs (nr__) ! (s) Second of Right Ascension (J2000) (1)
character*1 DEC_ (nr__) ! Sign of Declination (J2000) (1)
integer*4 DECd (nr__) ! (deg) Degree of Declination (J2000) (1)
integer*4 DECm (nr__) ! (arcmin) Arcminute of Declination (J2000) (1)
real*4 DECs (nr__) ! (arcsec) Arcsecond of Declination (J2000) (1)
real*4 S450 (nr__) ! (mJy) [1.9/42.3] The 450 micron flux density (G2)
real*4 e_S450 (nr__) ! (mJy) [0.6/8.1] Uncertainty in S450
real*4 S850 (nr__) ! (mJy) [1.4/14.3]? The 850 micron flux density (G2)
real*4 e_S850 (nr__) ! (mJy) [0.1/1.6]? Uncertainty in S850
real*4 z (nr__) ! [0.1/4.8]? Public redshift
real*4 e_z (nr__) ! [0/1.9]? Uncertainty in z
integer*4 f_z (nr__) ! [0/3] Flag on z (2)
real*4 logM_ (nr__) ! ([Msun]) [7.7/11.6]? Log stellar mass
real*4 e_logM_ (nr__) ! ([Msun]) [0.2/0.4]? Uncertainty in logM* (3)
real*4 logLUV (nr__) ! ([Lsun]) [7.5/12.5]? Log GALEX UV luminosity (G3)
real*4 e_logLUV (nr__) ! ([Lsun]) [0/0.5]? Uncertainty in logLUV
real*4 logLIR (nr__) ! ([Lsun]) [10.2/13.4] Log IR luminosity
real*4 e_logLIR (nr__) ! ([Lsun]) [0.03/0.6] Uncertainty in logLIR (3)
real*4 Td (nr__) ! (K) [17/66]? Dust temperature
real*4 e_Td (nr__) ! (K) [0.09/16]? Uncertainty in Td
real*4 betaUV (nr__) ! [-11.3/11.6]? Dust UV emissivity spectral
* index
real*4 e_betaUV (nr__) ! [0.2/4.4]? Uncertainty in betaUV
character*3 flag (nr__) ! AGN flag (s) (4)
*Note (1): VLA 3-GHz image coordinates (Table 2) or MIPS 24-um image
* coordinates (Table 3).
*Note (2): Flag as follows:
* 1 = spectroscopic redshift;
* 2 = photometric redshift;
* 3 = FIR redshift.
*Note (3): Derived from LE PHARE code (Arnouts+ 1999MNRAS.310..540A &
* Ilbert+ 2006A&A...457..841I) by including the photometric errors in
* each waveband but without including the redshift uncertainties.
*Note (4): AGN flag as follows:
* 1 = X-ray AGN;
* 2 = mid-infrared AGN;
* 3 = radio excess.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! Derived properties of MIPS 24-um
identified 450-um sources
integer*4 nr__1
parameter (nr__1=76) ! Number of records
character*142 ar__1 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_1 (nr__1) ! (deg) Right Ascension J2000
real*8 DEdeg_1 (nr__1) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 RAh_1 (nr__1) ! (h) [9/10] 450um Hour of Right Ascension (J2000)
* (G1)
integer*4 RAm_1 (nr__1) ! (min) 450um Minute of Right Ascension (J2000) (G1)
real*4 RAs_1 (nr__1) ! (s) 450um Second of Right Ascension (J2000) (G1)
character*1 DE__1 (nr__1) ! [+] 450um Sign of Declination (J2000) (G1)
integer*4 DEd_1 (nr__1) ! (deg) [2] 450um Degree of Declination (J2000) (G1)
integer*4 DEm_1 (nr__1) ! (arcmin) [12/33] 450um Arcminute of Declination (J2000)
* (G1)
real*4 DEs_1 (nr__1) ! (arcsec) 450um Arcsecond of Declination (J2000) (G1)
integer*4 RACh_1 (nr__1) ! (h) Hour of Right Ascension (J2000) (1)
integer*4 RACm_1 (nr__1) ! (min) Minute of Right Ascension (J2000) (1)
real*4 RACs_1 (nr__1) ! (s) Second of Right Ascension (J2000) (1)
character*1 DEC__1 (nr__1) ! Sign of Declination (J2000) (1)
integer*4 DECd_1 (nr__1) ! (deg) Degree of Declination (J2000) (1)
integer*4 DECm_1 (nr__1) ! (arcmin) Arcminute of Declination (J2000) (1)
real*4 DECs_1 (nr__1) ! (arcsec) Arcsecond of Declination (J2000) (1)
real*4 S450_1 (nr__1) ! (mJy) [1.9/42.3] The 450 micron flux density (G2)
real*4 e_S450_1 (nr__1) ! (mJy) [0.6/8.1] Uncertainty in S450
real*4 S850_1 (nr__1) ! (mJy) [1.4/14.3]? The 850 micron flux density (G2)
real*4 e_S850_1 (nr__1) ! (mJy) [0.1/1.6]? Uncertainty in S850
real*4 z_1 (nr__1) ! [0.1/4.8]? Public redshift
real*4 e_z_1 (nr__1) ! [0/1.9]? Uncertainty in z
integer*4 f_z_1 (nr__1) ! [0/3] Flag on z (2)
real*4 logM__1 (nr__1) ! ([Msun]) [7.7/11.6]? Log stellar mass
real*4 e_logM__1 (nr__1) ! ([Msun]) [0.2/0.4]? Uncertainty in logM* (3)
real*4 logLUV_1 (nr__1) ! ([Lsun]) [7.5/12.5]? Log GALEX UV luminosity (G3)
real*4 e_logLUV_1 (nr__1) ! ([Lsun]) [0/0.5]? Uncertainty in logLUV
real*4 logLIR_1 (nr__1) ! ([Lsun]) [10.2/13.4] Log IR luminosity
real*4 e_logLIR_1 (nr__1) ! ([Lsun]) [0.03/0.6] Uncertainty in logLIR (3)
real*4 Td_1 (nr__1) ! (K) [17/66]? Dust temperature
real*4 e_Td_1 (nr__1) ! (K) [0.09/16]? Uncertainty in Td
real*4 betaUV_1 (nr__1) ! [-11.3/11.6]? Dust UV emissivity spectral
* index
real*4 e_betaUV_1 (nr__1) ! [0.2/4.4]? Uncertainty in betaUV
character*3 flag_1 (nr__1) ! AGN flag (s) (4)
*Note (1): VLA 3-GHz image coordinates (Table 2) or MIPS 24-um image
* coordinates (Table 3).
*Note (2): Flag as follows:
* 1 = spectroscopic redshift;
* 2 = photometric redshift;
* 3 = FIR redshift.
*Note (3): Derived from LE PHARE code (Arnouts+ 1999MNRAS.310..540A &
* Ilbert+ 2006A&A...457..841I) by including the photometric errors in
* each waveband but without including the redshift uncertainties.
*Note (4): AGN flag as follows:
* 1 = X-ray AGN;
* 2 = mid-infrared AGN;
* 3 = radio excess.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table4.dat' ! Multi-wavelength photometry for VLA 3-GHz
identified 450-um sources
integer*4 nr__2
parameter (nr__2=134) ! Number of records
character*128 ar__2 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_2 (nr__2) ! (deg) Right Ascension J2000
real*8 DEdeg_2 (nr__2) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 RAh_2 (nr__2) ! (h) [9/10] 450um Hour of Right Ascension (J2000)
* (G1)
integer*4 RAm_2 (nr__2) ! (min) 450um Minute of Right Ascension (J2000) (G1)
real*4 RAs_2 (nr__2) ! (s) 450um Second of Right Ascension (J2000) (G1)
character*1 DE__2 (nr__2) ! [+] 450um Sign of Declination (J2000) (G1)
integer*4 DEd_2 (nr__2) ! (deg) [2] 450um Degree of Declination (J2000) (G1)
integer*4 DEm_2 (nr__2) ! (arcmin) [12/33] 450um Arcminute of Declination (J2000)
* (G1)
real*4 DEs_2 (nr__2) ! (arcsec) 450um Arcsecond of Declination (J2000) (G1)
integer*4 RAOh (nr__2) ! (h) ? Optical Hour of Right Ascension (J2000)
integer*4 RAOm (nr__2) ! (min) ? Optical Minute of Right Ascension (J2000)
real*4 RAOs (nr__2) ! (s) ? Optical Second of Right Ascension (J2000)
character*1 DEO_ (nr__2) ! ? Optical Sign of Declination (J2000) (G1)
integer*4 DEOd (nr__2) ! (deg) ? Optical Degree of Declination (J2000)
integer*4 DEOm (nr__2) ! (arcmin) ? Optical Arcminute of Declination (J2000)
real*4 DEOs (nr__2) ! (arcsec) ? Optical Arcsecond of Declination (J2000)
real*4 rmag (nr__2) ! (mag) [19.19/26.9]? Apparent Subaru/Suprime-cam
* r band magnitude (G3)
real*4 e_rmag (nr__2) ! (mag) [0/0.41]? Uncertainty in rmag
real*4 Ksmag (nr__2) ! (mag) [17.57/24.4]? Apparent VISTA/VIRCAM
* K_s_ band magnitude (G3)
real*4 e_Ksmag (nr__2) ! (mag) [0/0.28]? Uncertainty in Ksmag
real*4 S3_6 (nr__2) ! (mJy) [17.26/23.62]? The Spitzer/IRAC 3.6um flux
* density (from Sanders+ 2007ApJS..172...86S)
real*4 e_S3_6 (nr__2) ! (mJy) [0/0.06]? Uncertainty in S3.6
real*4 S250 (nr__2) ! (mJy) [0.7/87] The Herschel/SPIRE 250um flux
* density (G4)
real*4 e_S250 (nr__2) ! (mJy) [0.7/3.8] Uncertainty in S250
real*4 S450_2 (nr__2) ! (mJy) [1.98/42.3] The JCMT/SCUBA-2 450um flux
* density (G2)
real*4 e_S450_2 (nr__2) ! (mJy) [0.6/8.1] Uncertainty in S450
real*4 S850_2 (nr__2) ! (mJy) [1.45/14.3]? The JCMT/SCUBA-2 850um flux
* density (G2)
real*4 e_S850_2 (nr__2) ! (mJy) [0.1/1.6]? Uncertainty in S850
real*8 SC (nr__2) ! (mJy) The VLA 3GHz (Table 4) or MISP 24um (Table 5)
* flux density
real*4 e_SC (nr__2) ! (mJy) Uncertainty in SC
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table5.dat' ! Multi-wavelength photometry for MIPS 24-um
identified 450-um sources
integer*4 nr__3
parameter (nr__3=76) ! Number of records
character*128 ar__3 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_3 (nr__3) ! (deg) Right Ascension J2000
real*8 DEdeg_3 (nr__3) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 RAh_3 (nr__3) ! (h) [9/10] 450um Hour of Right Ascension (J2000)
* (G1)
integer*4 RAm_3 (nr__3) ! (min) 450um Minute of Right Ascension (J2000) (G1)
real*4 RAs_3 (nr__3) ! (s) 450um Second of Right Ascension (J2000) (G1)
character*1 DE__3 (nr__3) ! [+] 450um Sign of Declination (J2000) (G1)
integer*4 DEd_3 (nr__3) ! (deg) [2] 450um Degree of Declination (J2000) (G1)
integer*4 DEm_3 (nr__3) ! (arcmin) [12/33] 450um Arcminute of Declination (J2000)
* (G1)
real*4 DEs_3 (nr__3) ! (arcsec) 450um Arcsecond of Declination (J2000) (G1)
integer*4 RAOh_1 (nr__3) ! (h) ? Optical Hour of Right Ascension (J2000)
integer*4 RAOm_1 (nr__3) ! (min) ? Optical Minute of Right Ascension (J2000)
real*4 RAOs_1 (nr__3) ! (s) ? Optical Second of Right Ascension (J2000)
character*1 DEO__1 (nr__3) ! ? Optical Sign of Declination (J2000) (G1)
integer*4 DEOd_1 (nr__3) ! (deg) ? Optical Degree of Declination (J2000)
integer*4 DEOm_1 (nr__3) ! (arcmin) ? Optical Arcminute of Declination (J2000)
real*4 DEOs_1 (nr__3) ! (arcsec) ? Optical Arcsecond of Declination (J2000)
real*4 rmag_1 (nr__3) ! (mag) [19.19/26.9]? Apparent Subaru/Suprime-cam
* r band magnitude (G3)
real*4 e_rmag_1 (nr__3) ! (mag) [0/0.41]? Uncertainty in rmag
real*4 Ksmag_1 (nr__3) ! (mag) [17.57/24.4]? Apparent VISTA/VIRCAM
* K_s_ band magnitude (G3)
real*4 e_Ksmag_1 (nr__3) ! (mag) [0/0.28]? Uncertainty in Ksmag
real*4 S3_6_1 (nr__3) ! (mJy) [17.26/23.62]? The Spitzer/IRAC 3.6um flux
* density (from Sanders+ 2007ApJS..172...86S)
real*4 e_S3_6_1 (nr__3) ! (mJy) [0/0.06]? Uncertainty in S3.6
real*4 S250_1 (nr__3) ! (mJy) [0.7/87] The Herschel/SPIRE 250um flux
* density (G4)
real*4 e_S250_1 (nr__3) ! (mJy) [0.7/3.8] Uncertainty in S250
real*4 S450_3 (nr__3) ! (mJy) [1.98/42.3] The JCMT/SCUBA-2 450um flux
* density (G2)
real*4 e_S450_3 (nr__3) ! (mJy) [0.6/8.1] Uncertainty in S450
real*4 S850_3 (nr__3) ! (mJy) [1.45/14.3]? The JCMT/SCUBA-2 850um flux
* density (G2)
real*4 e_S850_3 (nr__3) ! (mJy) [0.1/1.6]? Uncertainty in S850
real*8 SC_1 (nr__3) ! (mJy) The VLA 3GHz (Table 4) or MISP 24um (Table 5)
* flux density
real*4 e_SC_1 (nr__3) ! (mJy) Uncertainty in SC
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table6.dat' ! List of 450-um sources without VLA 3GHz and
MIPS 24um counterparts
integer*4 nr__4
parameter (nr__4=46) ! Number of records
character*56 ar__4 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_4 (nr__4) ! (deg) Right Ascension J2000
real*8 DEdeg_4 (nr__4) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 RAh_4 (nr__4) ! (h) [10] Hour of Right Ascension (J2000)
integer*4 RAm_4 (nr__4) ! (min) [0] Minute of Right Ascension (J2000)
real*4 RAs_4 (nr__4) ! (s) Second of Right Ascension (J2000)
character*1 DE__4 (nr__4) ! [+] 450um Sign of Declination (J2000) (G1)
integer*4 DEd_4 (nr__4) ! (deg) [2] Degree of Declination (J2000)
integer*4 DEm_4 (nr__4) ! (arcmin) [11/34] Arcminute of Declination (J2000)
real*4 DEs_4 (nr__4) ! (arcsec) Arcsecond of Declination (J2000)
real*4 S250_2 (nr__4) ! (mJy) [0.2/46] The Herschel/SPIRE 250um flux
* density (G4)
real*4 e_S250_2 (nr__4) ! (mJy) [0.4/3.1] Uncertainty in S250
real*4 S450_4 (nr__4) ! (mJy) [2.16/51.2] The JCMT/SCUBA-2 450um flux
* density (G2)
real*4 e_S450_4 (nr__4) ! (mJy) [0.6/13.7] Uncertainty in S450
real*4 S850_4 (nr__4) ! (mJy) [1.4/5]? The JCMT/SCUBA-2 850um flux
* density (G2)
real*4 e_S850_4 (nr__4) ! (mJy) [0.1/0.3]? Uncertainty in S850
C=============================================================================
C Loading file 'table2.dat' ! Derived properties of VLA 3-GHz
* identified 450-um sources
C Format for file interpretation
1 format(
+ I2,1X,I2,1X,F5.2,1X,A1,I1,1X,I2,1X,F5.2,1X,I2,1X,I2,1X,F5.2,
+ 1X,A1,I1,1X,I2,1X,F5.2,1X,F5.2,1X,F4.2,1X,F5.2,1X,F4.2,1X,
+ F4.2,1X,F4.2,1X,I1,1X,F5.2,1X,F4.2,1X,F5.2,1X,F4.2,1X,F5.2,1X,
+ F4.2,1X,F5.2,1X,F5.2,1X,F6.2,1X,F4.2,1X,A3)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,134
read(1,'(A142)')ar__
read(ar__,1)
+ RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),DEm(i__),
+ DEs(i__),RACh(i__),RACm(i__),RACs(i__),DEC_(i__),DECd(i__),
+ DECm(i__),DECs(i__),S450(i__),e_S450(i__),S850(i__),
+ e_S850(i__),z(i__),e_z(i__),f_z(i__),logM_(i__),e_logM_(i__),
+ logLUV(i__),e_logLUV(i__),logLIR(i__),e_logLIR(i__),Td(i__),
+ e_Td(i__),betaUV(i__),e_betaUV(i__),flag(i__)
if(ar__(60:64) .EQ. '') S850(i__) = rNULL__
if(ar__(66:69) .EQ. '') e_S850(i__) = rNULL__
if(ar__(71:74) .EQ. '') z(i__) = rNULL__
if(ar__(76:79) .EQ. '') e_z(i__) = rNULL__
if(ar__(83:87) .EQ. '') logM_(i__) = rNULL__
if(ar__(89:92) .EQ. '') e_logM_(i__) = rNULL__
if(ar__(94:98) .EQ. '') logLUV(i__) = rNULL__
if(ar__(100:103) .EQ. '') e_logLUV(i__) = rNULL__
if(ar__(116:120) .EQ. '') Td(i__) = rNULL__
if(ar__(122:126) .EQ. '') e_Td(i__) = rNULL__
if(ar__(128:133) .EQ. '') betaUV(i__) = rNULL__
if(ar__(135:138) .EQ. '') e_betaUV(i__) = rNULL__
RAdeg(i__) = rNULL__
DEdeg(i__) = rNULL__
c Derive coordinates RAdeg and DEdeg from input data
c (RAdeg and DEdeg are set to rNULL__ when unknown)
if(RAh(i__) .GT. -180) RAdeg(i__)=RAh(i__)*15.
if(RAm(i__) .GT. -180) RAdeg(i__)=RAdeg(i__)+RAm(i__)/4.
if(RAs(i__) .GT. -180) RAdeg(i__)=RAdeg(i__)+RAs(i__)/240.
if(DEd(i__) .GE. 0) DEdeg(i__)=DEd(i__)
if(DEm(i__) .GE. 0) DEdeg(i__)=DEdeg(i__)+DEm(i__)/60.
if(DEs(i__) .GE. 0) DEdeg(i__)=DEdeg(i__)+DEs(i__)/3600.
if(DE_(i__).EQ.'-'.AND.DEdeg(i__).GE.0) DEdeg(i__)=-DEdeg(i__)
c ..............Just test output...........
write(6,1)
+ RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),DEm(i__),
+ DEs(i__),RACh(i__),RACm(i__),RACs(i__),DEC_(i__),DECd(i__),
+ DECm(i__),DECs(i__),S450(i__),e_S450(i__),S850(i__),
+ e_S850(i__),z(i__),e_z(i__),f_z(i__),logM_(i__),e_logM_(i__),
+ logLUV(i__),e_logLUV(i__),logLIR(i__),e_logLIR(i__),Td(i__),
+ e_Td(i__),betaUV(i__),e_betaUV(i__),flag(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table3.dat' ! Derived properties of MIPS 24-um
* identified 450-um sources
C Format for file interpretation
2 format(
+ I2,1X,I2,1X,F5.2,1X,A1,I1,1X,I2,1X,F5.2,1X,I2,1X,I2,1X,F5.2,
+ 1X,A1,I1,1X,I2,1X,F5.2,1X,F5.2,1X,F4.2,1X,F5.2,1X,F4.2,1X,
+ F4.2,1X,F4.2,1X,I1,1X,F5.2,1X,F4.2,1X,F5.2,1X,F4.2,1X,F5.2,1X,
+ F4.2,1X,F5.2,1X,F5.2,1X,F6.2,1X,F4.2,1X,A3)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,76
read(1,'(A142)')ar__1
read(ar__1,2)
+ RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),DEd_1(i__),
+ DEm_1(i__),DEs_1(i__),RACh_1(i__),RACm_1(i__),RACs_1(i__),
+ DEC__1(i__),DECd_1(i__),DECm_1(i__),DECs_1(i__),S450_1(i__),
+ e_S450_1(i__),S850_1(i__),e_S850_1(i__),z_1(i__),e_z_1(i__),
+ f_z_1(i__),logM__1(i__),e_logM__1(i__),logLUV_1(i__),
+ e_logLUV_1(i__),logLIR_1(i__),e_logLIR_1(i__),Td_1(i__),
+ e_Td_1(i__),betaUV_1(i__),e_betaUV_1(i__),flag_1(i__)
if(ar__1(60:64) .EQ. '') S850_1(i__) = rNULL__
if(ar__1(66:69) .EQ. '') e_S850_1(i__) = rNULL__
if(ar__1(71:74) .EQ. '') z_1(i__) = rNULL__
if(ar__1(76:79) .EQ. '') e_z_1(i__) = rNULL__
if(ar__1(83:87) .EQ. '') logM__1(i__) = rNULL__
if(ar__1(89:92) .EQ. '') e_logM__1(i__) = rNULL__
if(ar__1(94:98) .EQ. '') logLUV_1(i__) = rNULL__
if(ar__1(100:103) .EQ. '') e_logLUV_1(i__) = rNULL__
if(ar__1(116:120) .EQ. '') Td_1(i__) = rNULL__
if(ar__1(122:126) .EQ. '') e_Td_1(i__) = rNULL__
if(ar__1(128:133) .EQ. '') betaUV_1(i__) = rNULL__
if(ar__1(135:138) .EQ. '') e_betaUV_1(i__) = rNULL__
RAdeg_1(i__) = rNULL__
DEdeg_1(i__) = rNULL__
c Derive coordinates RAdeg_1 and DEdeg_1 from input data
c (RAdeg_1 and DEdeg_1 are set to rNULL__ when unknown)
if(RAh_1(i__) .GT. -180) RAdeg_1(i__)=RAh_1(i__)*15.
if(RAm_1(i__) .GT. -180) RAdeg_1(i__)=RAdeg_1(i__)+RAm_1(i__)/4.
if(RAs_1(i__) .GT. -180) RAdeg_1(i__)=RAdeg_1(i__)+RAs_1(i__)/240.
if(DEd_1(i__) .GE. 0) DEdeg_1(i__)=DEd_1(i__)
if(DEm_1(i__) .GE. 0) DEdeg_1(i__)=DEdeg_1(i__)+DEm_1(i__)/60.
if(DEs_1(i__) .GE. 0) DEdeg_1(i__)=DEdeg_1(i__)+DEs_1(i__)/3600.
if(DE__1(i__).EQ.'-'.AND.DEdeg_1(i__).GE.0) DEdeg_1(i__)=-DEdeg_1(i__)
c ..............Just test output...........
write(6,2)
+ RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),DEd_1(i__),
+ DEm_1(i__),DEs_1(i__),RACh_1(i__),RACm_1(i__),RACs_1(i__),
+ DEC__1(i__),DECd_1(i__),DECm_1(i__),DECs_1(i__),S450_1(i__),
+ e_S450_1(i__),S850_1(i__),e_S850_1(i__),z_1(i__),e_z_1(i__),
+ f_z_1(i__),logM__1(i__),e_logM__1(i__),logLUV_1(i__),
+ e_logLUV_1(i__),logLIR_1(i__),e_logLIR_1(i__),Td_1(i__),
+ e_Td_1(i__),betaUV_1(i__),e_betaUV_1(i__),flag_1(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_1(i__),DEdeg_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table4.dat' ! Multi-wavelength photometry for VLA 3-GHz
* identified 450-um sources
C Format for file interpretation
3 format(
+ I2,1X,I2,1X,F5.2,1X,A1,I1,1X,I2,1X,F5.2,1X,I2,1X,I2,1X,F5.2,
+ 1X,A1,I1,1X,I2,1X,F5.2,1X,F5.2,1X,F4.2,1X,F5.2,1X,F4.2,1X,
+ F5.2,1X,F4.2,1X,F5.2,1X,F4.2,1X,F5.2,1X,F4.2,1X,F5.2,1X,F4.2,
+ 1X,F7.2,1X,F6.2)
C Effective file loading
open(unit=1,status='old',file=
+'table4.dat')
write(6,*) '....Loading file: table4.dat'
do i__=1,134
read(1,'(A128)')ar__2
read(ar__2,3)
+ RAh_2(i__),RAm_2(i__),RAs_2(i__),DE__2(i__),DEd_2(i__),
+ DEm_2(i__),DEs_2(i__),RAOh(i__),RAOm(i__),RAOs(i__),DEO_(i__),
+ DEOd(i__),DEOm(i__),DEOs(i__),rmag(i__),e_rmag(i__),
+ Ksmag(i__),e_Ksmag(i__),S3_6(i__),e_S3_6(i__),S250(i__),
+ e_S250(i__),S450_2(i__),e_S450_2(i__),S850_2(i__),
+ e_S850_2(i__),SC(i__),e_SC(i__)
if(ar__2(25:26) .EQ. '') RAOh(i__) = iNULL__
if(ar__2(28:29) .EQ. '') RAOm(i__) = iNULL__
if(ar__2(31:35) .EQ. '') RAOs(i__) = rNULL__
if(ar__2(38:38) .EQ. '') DEOd(i__) = iNULL__
if(ar__2(40:41) .EQ. '') DEOm(i__) = iNULL__
if(ar__2(43:47) .EQ. '') DEOs(i__) = rNULL__
if(ar__2(49:53) .EQ. '') rmag(i__) = rNULL__
if(ar__2(55:58) .EQ. '') e_rmag(i__) = rNULL__
if(ar__2(60:64) .EQ. '') Ksmag(i__) = rNULL__
if(ar__2(66:69) .EQ. '') e_Ksmag(i__) = rNULL__
if(ar__2(71:75) .EQ. '') S3_6(i__) = rNULL__
if(ar__2(77:80) .EQ. '') e_S3_6(i__) = rNULL__
if(ar__2(104:108) .EQ. '') S850_2(i__) = rNULL__
if(ar__2(110:113) .EQ. '') e_S850_2(i__) = rNULL__
RAdeg_2(i__) = rNULL__
DEdeg_2(i__) = rNULL__
c Derive coordinates RAdeg_2 and DEdeg_2 from input data
c (RAdeg_2 and DEdeg_2 are set to rNULL__ when unknown)
if(RAh_2(i__) .GT. -180) RAdeg_2(i__)=RAh_2(i__)*15.
if(RAm_2(i__) .GT. -180) RAdeg_2(i__)=RAdeg_2(i__)+RAm_2(i__)/4.
if(RAs_2(i__) .GT. -180) RAdeg_2(i__)=RAdeg_2(i__)+RAs_2(i__)/240.
if(DEd_2(i__) .GE. 0) DEdeg_2(i__)=DEd_2(i__)
if(DEm_2(i__) .GE. 0) DEdeg_2(i__)=DEdeg_2(i__)+DEm_2(i__)/60.
if(DEs_2(i__) .GE. 0) DEdeg_2(i__)=DEdeg_2(i__)+DEs_2(i__)/3600.
if(DE__2(i__).EQ.'-'.AND.DEdeg_2(i__).GE.0) DEdeg_2(i__)=-DEdeg_2(i__)
c ..............Just test output...........
write(6,3)
+ RAh_2(i__),RAm_2(i__),RAs_2(i__),DE__2(i__),DEd_2(i__),
+ DEm_2(i__),DEs_2(i__),RAOh(i__),RAOm(i__),RAOs(i__),DEO_(i__),
+ DEOd(i__),DEOm(i__),DEOs(i__),rmag(i__),e_rmag(i__),
+ Ksmag(i__),e_Ksmag(i__),S3_6(i__),e_S3_6(i__),S250(i__),
+ e_S250(i__),S450_2(i__),e_S450_2(i__),S850_2(i__),
+ e_S850_2(i__),SC(i__),e_SC(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_2(i__),DEdeg_2(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table5.dat' ! Multi-wavelength photometry for MIPS 24-um
* identified 450-um sources
C Format for file interpretation
4 format(
+ I2,1X,I2,1X,F5.2,1X,A1,I1,1X,I2,1X,F5.2,1X,I2,1X,I2,1X,F5.2,
+ 1X,A1,I1,1X,I2,1X,F5.2,1X,F5.2,1X,F4.2,1X,F5.2,1X,F4.2,1X,
+ F5.2,1X,F4.2,1X,F5.2,1X,F4.2,1X,F5.2,1X,F4.2,1X,F5.2,1X,F4.2,
+ 1X,F7.2,1X,F6.2)
C Effective file loading
open(unit=1,status='old',file=
+'table5.dat')
write(6,*) '....Loading file: table5.dat'
do i__=1,76
read(1,'(A128)')ar__3
read(ar__3,4)
+ RAh_3(i__),RAm_3(i__),RAs_3(i__),DE__3(i__),DEd_3(i__),
+ DEm_3(i__),DEs_3(i__),RAOh_1(i__),RAOm_1(i__),RAOs_1(i__),
+ DEO__1(i__),DEOd_1(i__),DEOm_1(i__),DEOs_1(i__),rmag_1(i__),
+ e_rmag_1(i__),Ksmag_1(i__),e_Ksmag_1(i__),S3_6_1(i__),
+ e_S3_6_1(i__),S250_1(i__),e_S250_1(i__),S450_3(i__),
+ e_S450_3(i__),S850_3(i__),e_S850_3(i__),SC_1(i__),e_SC_1(i__)
if(ar__3(25:26) .EQ. '') RAOh_1(i__) = iNULL__
if(ar__3(28:29) .EQ. '') RAOm_1(i__) = iNULL__
if(ar__3(31:35) .EQ. '') RAOs_1(i__) = rNULL__
if(ar__3(38:38) .EQ. '') DEOd_1(i__) = iNULL__
if(ar__3(40:41) .EQ. '') DEOm_1(i__) = iNULL__
if(ar__3(43:47) .EQ. '') DEOs_1(i__) = rNULL__
if(ar__3(49:53) .EQ. '') rmag_1(i__) = rNULL__
if(ar__3(55:58) .EQ. '') e_rmag_1(i__) = rNULL__
if(ar__3(60:64) .EQ. '') Ksmag_1(i__) = rNULL__
if(ar__3(66:69) .EQ. '') e_Ksmag_1(i__) = rNULL__
if(ar__3(71:75) .EQ. '') S3_6_1(i__) = rNULL__
if(ar__3(77:80) .EQ. '') e_S3_6_1(i__) = rNULL__
if(ar__3(104:108) .EQ. '') S850_3(i__) = rNULL__
if(ar__3(110:113) .EQ. '') e_S850_3(i__) = rNULL__
RAdeg_3(i__) = rNULL__
DEdeg_3(i__) = rNULL__
c Derive coordinates RAdeg_3 and DEdeg_3 from input data
c (RAdeg_3 and DEdeg_3 are set to rNULL__ when unknown)
if(RAh_3(i__) .GT. -180) RAdeg_3(i__)=RAh_3(i__)*15.
if(RAm_3(i__) .GT. -180) RAdeg_3(i__)=RAdeg_3(i__)+RAm_3(i__)/4.
if(RAs_3(i__) .GT. -180) RAdeg_3(i__)=RAdeg_3(i__)+RAs_3(i__)/240.
if(DEd_3(i__) .GE. 0) DEdeg_3(i__)=DEd_3(i__)
if(DEm_3(i__) .GE. 0) DEdeg_3(i__)=DEdeg_3(i__)+DEm_3(i__)/60.
if(DEs_3(i__) .GE. 0) DEdeg_3(i__)=DEdeg_3(i__)+DEs_3(i__)/3600.
if(DE__3(i__).EQ.'-'.AND.DEdeg_3(i__).GE.0) DEdeg_3(i__)=-DEdeg_3(i__)
c ..............Just test output...........
write(6,4)
+ RAh_3(i__),RAm_3(i__),RAs_3(i__),DE__3(i__),DEd_3(i__),
+ DEm_3(i__),DEs_3(i__),RAOh_1(i__),RAOm_1(i__),RAOs_1(i__),
+ DEO__1(i__),DEOd_1(i__),DEOm_1(i__),DEOs_1(i__),rmag_1(i__),
+ e_rmag_1(i__),Ksmag_1(i__),e_Ksmag_1(i__),S3_6_1(i__),
+ e_S3_6_1(i__),S250_1(i__),e_S250_1(i__),S450_3(i__),
+ e_S450_3(i__),S850_3(i__),e_S850_3(i__),SC_1(i__),e_SC_1(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_3(i__),DEdeg_3(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table6.dat' ! List of 450-um sources without VLA 3GHz and
* MIPS 24um counterparts
C Format for file interpretation
5 format(
+ I2,1X,I2,1X,F5.2,1X,A1,I1,1X,I2,1X,F5.2,1X,F5.2,1X,F4.2,1X,
+ F5.2,1X,F5.2,1X,F4.2,1X,F4.2)
C Effective file loading
open(unit=1,status='old',file=
+'table6.dat')
write(6,*) '....Loading file: table6.dat'
do i__=1,46
read(1,'(A56)')ar__4
read(ar__4,5)
+ RAh_4(i__),RAm_4(i__),RAs_4(i__),DE__4(i__),DEd_4(i__),
+ DEm_4(i__),DEs_4(i__),S250_2(i__),e_S250_2(i__),S450_4(i__),
+ e_S450_4(i__),S850_4(i__),e_S850_4(i__)
if(ar__4(48:51) .EQ. '') S850_4(i__) = rNULL__
if(ar__4(53:56) .EQ. '') e_S850_4(i__) = rNULL__
RAdeg_4(i__) = rNULL__
DEdeg_4(i__) = rNULL__
c Derive coordinates RAdeg_4 and DEdeg_4 from input data
c (RAdeg_4 and DEdeg_4 are set to rNULL__ when unknown)
if(RAh_4(i__) .GT. -180) RAdeg_4(i__)=RAh_4(i__)*15.
if(RAm_4(i__) .GT. -180) RAdeg_4(i__)=RAdeg_4(i__)+RAm_4(i__)/4.
if(RAs_4(i__) .GT. -180) RAdeg_4(i__)=RAdeg_4(i__)+RAs_4(i__)/240.
if(DEd_4(i__) .GE. 0) DEdeg_4(i__)=DEd_4(i__)
if(DEm_4(i__) .GE. 0) DEdeg_4(i__)=DEdeg_4(i__)+DEm_4(i__)/60.
if(DEs_4(i__) .GE. 0) DEdeg_4(i__)=DEdeg_4(i__)+DEs_4(i__)/3600.
if(DE__4(i__).EQ.'-'.AND.DEdeg_4(i__).GE.0) DEdeg_4(i__)=-DEdeg_4(i__)
c ..............Just test output...........
write(6,5)
+ RAh_4(i__),RAm_4(i__),RAs_4(i__),DE__4(i__),DEd_4(i__),
+ DEm_4(i__),DEs_4(i__),S250_2(i__),e_S250_2(i__),S450_4(i__),
+ e_S450_4(i__),S850_4(i__),e_S850_4(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_4(i__),DEdeg_4(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end