Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/889/80 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-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 ! (deg) Right Ascension J2000
real*8 DEdeg ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 RAh ! (h) [9/10] 450um Hour of Right Ascension (J2000)
* (G1)
integer*4 RAm ! (min) 450um Minute of Right Ascension (J2000) (G1)
real*4 RAs ! (s) 450um Second of Right Ascension (J2000) (G1)
character*1 DE_ ! [+] 450um Sign of Declination (J2000) (G1)
integer*4 DEd ! (deg) [2] 450um Degree of Declination (J2000) (G1)
integer*4 DEm ! (arcmin) [12/33] 450um Arcminute of Declination (J2000)
* (G1)
real*4 DEs ! (arcsec) 450um Arcsecond of Declination (J2000) (G1)
integer*4 RACh ! (h) Hour of Right Ascension (J2000) (1)
integer*4 RACm ! (min) Minute of Right Ascension (J2000) (1)
real*4 RACs ! (s) Second of Right Ascension (J2000) (1)
character*1 DEC_ ! Sign of Declination (J2000) (1)
integer*4 DECd ! (deg) Degree of Declination (J2000) (1)
integer*4 DECm ! (arcmin) Arcminute of Declination (J2000) (1)
real*4 DECs ! (arcsec) Arcsecond of Declination (J2000) (1)
real*4 S450 ! (mJy) [1.9/42.3] The 450 micron flux density (G2)
real*4 e_S450 ! (mJy) [0.6/8.1] Uncertainty in S450
real*4 S850 ! (mJy) [1.4/14.3]? The 850 micron flux density (G2)
real*4 e_S850 ! (mJy) [0.1/1.6]? Uncertainty in S850
real*4 z ! [0.1/4.8]? Public redshift
real*4 e_z ! [0/1.9]? Uncertainty in z
integer*4 f_z ! [0/3] Flag on z (2)
real*4 logM_ ! ([Msun]) [7.7/11.6]? Log stellar mass
real*4 e_logM_ ! ([Msun]) [0.2/0.4]? Uncertainty in logM* (3)
real*4 logLUV ! ([Lsun]) [7.5/12.5]? Log GALEX UV luminosity (G3)
real*4 e_logLUV ! ([Lsun]) [0/0.5]? Uncertainty in logLUV
real*4 logLIR ! ([Lsun]) [10.2/13.4] Log IR luminosity
real*4 e_logLIR ! ([Lsun]) [0.03/0.6] Uncertainty in logLIR (3)
real*4 Td ! (K) [17/66]? Dust temperature
real*4 e_Td ! (K) [0.09/16]? Uncertainty in Td
real*4 betaUV ! [-11.3/11.6]? Dust UV emissivity spectral
* index
real*4 e_betaUV ! [0.2/4.4]? Uncertainty in betaUV
character*3 flag ! 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 ! (deg) Right Ascension J2000
real*8 DEdeg_1 ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 RAh_1 ! (h) [9/10] 450um Hour of Right Ascension (J2000)
* (G1)
integer*4 RAm_1 ! (min) 450um Minute of Right Ascension (J2000) (G1)
real*4 RAs_1 ! (s) 450um Second of Right Ascension (J2000) (G1)
character*1 DE__1 ! [+] 450um Sign of Declination (J2000) (G1)
integer*4 DEd_1 ! (deg) [2] 450um Degree of Declination (J2000) (G1)
integer*4 DEm_1 ! (arcmin) [12/33] 450um Arcminute of Declination (J2000)
* (G1)
real*4 DEs_1 ! (arcsec) 450um Arcsecond of Declination (J2000) (G1)
integer*4 RACh_1 ! (h) Hour of Right Ascension (J2000) (1)
integer*4 RACm_1 ! (min) Minute of Right Ascension (J2000) (1)
real*4 RACs_1 ! (s) Second of Right Ascension (J2000) (1)
character*1 DEC__1 ! Sign of Declination (J2000) (1)
integer*4 DECd_1 ! (deg) Degree of Declination (J2000) (1)
integer*4 DECm_1 ! (arcmin) Arcminute of Declination (J2000) (1)
real*4 DECs_1 ! (arcsec) Arcsecond of Declination (J2000) (1)
real*4 S450_1 ! (mJy) [1.9/42.3] The 450 micron flux density (G2)
real*4 e_S450_1 ! (mJy) [0.6/8.1] Uncertainty in S450
real*4 S850_1 ! (mJy) [1.4/14.3]? The 850 micron flux density (G2)
real*4 e_S850_1 ! (mJy) [0.1/1.6]? Uncertainty in S850
real*4 z_1 ! [0.1/4.8]? Public redshift
real*4 e_z_1 ! [0/1.9]? Uncertainty in z
integer*4 f_z_1 ! [0/3] Flag on z (2)
real*4 logM__1 ! ([Msun]) [7.7/11.6]? Log stellar mass
real*4 e_logM__1 ! ([Msun]) [0.2/0.4]? Uncertainty in logM* (3)
real*4 logLUV_1 ! ([Lsun]) [7.5/12.5]? Log GALEX UV luminosity (G3)
real*4 e_logLUV_1 ! ([Lsun]) [0/0.5]? Uncertainty in logLUV
real*4 logLIR_1 ! ([Lsun]) [10.2/13.4] Log IR luminosity
real*4 e_logLIR_1 ! ([Lsun]) [0.03/0.6] Uncertainty in logLIR (3)
real*4 Td_1 ! (K) [17/66]? Dust temperature
real*4 e_Td_1 ! (K) [0.09/16]? Uncertainty in Td
real*4 betaUV_1 ! [-11.3/11.6]? Dust UV emissivity spectral
* index
real*4 e_betaUV_1 ! [0.2/4.4]? Uncertainty in betaUV
character*3 flag_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 ! (deg) Right Ascension J2000
real*8 DEdeg_2 ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 RAh_2 ! (h) [9/10] 450um Hour of Right Ascension (J2000)
* (G1)
integer*4 RAm_2 ! (min) 450um Minute of Right Ascension (J2000) (G1)
real*4 RAs_2 ! (s) 450um Second of Right Ascension (J2000) (G1)
character*1 DE__2 ! [+] 450um Sign of Declination (J2000) (G1)
integer*4 DEd_2 ! (deg) [2] 450um Degree of Declination (J2000) (G1)
integer*4 DEm_2 ! (arcmin) [12/33] 450um Arcminute of Declination (J2000)
* (G1)
real*4 DEs_2 ! (arcsec) 450um Arcsecond of Declination (J2000) (G1)
integer*4 RAOh ! (h) ? Optical Hour of Right Ascension (J2000)
integer*4 RAOm ! (min) ? Optical Minute of Right Ascension (J2000)
real*4 RAOs ! (s) ? Optical Second of Right Ascension (J2000)
character*1 DEO_ ! ? Optical Sign of Declination (J2000) (G1)
integer*4 DEOd ! (deg) ? Optical Degree of Declination (J2000)
integer*4 DEOm ! (arcmin) ? Optical Arcminute of Declination (J2000)
real*4 DEOs ! (arcsec) ? Optical Arcsecond of Declination (J2000)
real*4 rmag ! (mag) [19.19/26.9]? Apparent Subaru/Suprime-cam
* r band magnitude (G3)
real*4 e_rmag ! (mag) [0/0.41]? Uncertainty in rmag
real*4 Ksmag ! (mag) [17.57/24.4]? Apparent VISTA/VIRCAM
* K_s_ band magnitude (G3)
real*4 e_Ksmag ! (mag) [0/0.28]? Uncertainty in Ksmag
real*4 S3_6 ! (mJy) [17.26/23.62]? The Spitzer/IRAC 3.6um flux
* density (from Sanders+ 2007ApJS..172...86S)
real*4 e_S3_6 ! (mJy) [0/0.06]? Uncertainty in S3.6
real*4 S250 ! (mJy) [0.7/87] The Herschel/SPIRE 250um flux
* density (G4)
real*4 e_S250 ! (mJy) [0.7/3.8] Uncertainty in S250
real*4 S450_2 ! (mJy) [1.98/42.3] The JCMT/SCUBA-2 450um flux
* density (G2)
real*4 e_S450_2 ! (mJy) [0.6/8.1] Uncertainty in S450
real*4 S850_2 ! (mJy) [1.45/14.3]? The JCMT/SCUBA-2 850um flux
* density (G2)
real*4 e_S850_2 ! (mJy) [0.1/1.6]? Uncertainty in S850
real*8 SC ! (mJy) The VLA 3GHz (Table 4) or MISP 24um (Table 5)
* flux density
real*4 e_SC ! (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 ! (deg) Right Ascension J2000
real*8 DEdeg_3 ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 RAh_3 ! (h) [9/10] 450um Hour of Right Ascension (J2000)
* (G1)
integer*4 RAm_3 ! (min) 450um Minute of Right Ascension (J2000) (G1)
real*4 RAs_3 ! (s) 450um Second of Right Ascension (J2000) (G1)
character*1 DE__3 ! [+] 450um Sign of Declination (J2000) (G1)
integer*4 DEd_3 ! (deg) [2] 450um Degree of Declination (J2000) (G1)
integer*4 DEm_3 ! (arcmin) [12/33] 450um Arcminute of Declination (J2000)
* (G1)
real*4 DEs_3 ! (arcsec) 450um Arcsecond of Declination (J2000) (G1)
integer*4 RAOh_1 ! (h) ? Optical Hour of Right Ascension (J2000)
integer*4 RAOm_1 ! (min) ? Optical Minute of Right Ascension (J2000)
real*4 RAOs_1 ! (s) ? Optical Second of Right Ascension (J2000)
character*1 DEO__1 ! ? Optical Sign of Declination (J2000) (G1)
integer*4 DEOd_1 ! (deg) ? Optical Degree of Declination (J2000)
integer*4 DEOm_1 ! (arcmin) ? Optical Arcminute of Declination (J2000)
real*4 DEOs_1 ! (arcsec) ? Optical Arcsecond of Declination (J2000)
real*4 rmag_1 ! (mag) [19.19/26.9]? Apparent Subaru/Suprime-cam
* r band magnitude (G3)
real*4 e_rmag_1 ! (mag) [0/0.41]? Uncertainty in rmag
real*4 Ksmag_1 ! (mag) [17.57/24.4]? Apparent VISTA/VIRCAM
* K_s_ band magnitude (G3)
real*4 e_Ksmag_1 ! (mag) [0/0.28]? Uncertainty in Ksmag
real*4 S3_6_1 ! (mJy) [17.26/23.62]? The Spitzer/IRAC 3.6um flux
* density (from Sanders+ 2007ApJS..172...86S)
real*4 e_S3_6_1 ! (mJy) [0/0.06]? Uncertainty in S3.6
real*4 S250_1 ! (mJy) [0.7/87] The Herschel/SPIRE 250um flux
* density (G4)
real*4 e_S250_1 ! (mJy) [0.7/3.8] Uncertainty in S250
real*4 S450_3 ! (mJy) [1.98/42.3] The JCMT/SCUBA-2 450um flux
* density (G2)
real*4 e_S450_3 ! (mJy) [0.6/8.1] Uncertainty in S450
real*4 S850_3 ! (mJy) [1.45/14.3]? The JCMT/SCUBA-2 850um flux
* density (G2)
real*4 e_S850_3 ! (mJy) [0.1/1.6]? Uncertainty in S850
real*8 SC_1 ! (mJy) The VLA 3GHz (Table 4) or MISP 24um (Table 5)
* flux density
real*4 e_SC_1 ! (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 ! (deg) Right Ascension J2000
real*8 DEdeg_4 ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 RAh_4 ! (h) [10] Hour of Right Ascension (J2000)
integer*4 RAm_4 ! (min) [0] Minute of Right Ascension (J2000)
real*4 RAs_4 ! (s) Second of Right Ascension (J2000)
character*1 DE__4 ! [+] 450um Sign of Declination (J2000) (G1)
integer*4 DEd_4 ! (deg) [2] Degree of Declination (J2000)
integer*4 DEm_4 ! (arcmin) [11/34] Arcminute of Declination (J2000)
real*4 DEs_4 ! (arcsec) Arcsecond of Declination (J2000)
real*4 S250_2 ! (mJy) [0.2/46] The Herschel/SPIRE 250um flux
* density (G4)
real*4 e_S250_2 ! (mJy) [0.4/3.1] Uncertainty in S250
real*4 S450_4 ! (mJy) [2.16/51.2] The JCMT/SCUBA-2 450um flux
* density (G2)
real*4 e_S450_4 ! (mJy) [0.6/13.7] Uncertainty in S450
real*4 S850_4 ! (mJy) [1.4/5]? The JCMT/SCUBA-2 850um flux
* density (G2)
real*4 e_S850_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,RAm,RAs,DE_,DEd,DEm,DEs,RACh,RACm,RACs,DEC_,DECd,DECm,
+ DECs,S450,e_S450,S850,e_S850,z,e_z,f_z,logM_,e_logM_,logLUV,
+ e_logLUV,logLIR,e_logLIR,Td,e_Td,betaUV,e_betaUV,flag
if(ar__(60:64) .EQ. '') S850 = rNULL__
if(ar__(66:69) .EQ. '') e_S850 = rNULL__
if(ar__(71:74) .EQ. '') z = rNULL__
if(ar__(76:79) .EQ. '') e_z = rNULL__
if(ar__(83:87) .EQ. '') logM_ = rNULL__
if(ar__(89:92) .EQ. '') e_logM_ = rNULL__
if(ar__(94:98) .EQ. '') logLUV = rNULL__
if(ar__(100:103) .EQ. '') e_logLUV = rNULL__
if(ar__(116:120) .EQ. '') Td = rNULL__
if(ar__(122:126) .EQ. '') e_Td = rNULL__
if(ar__(128:133) .EQ. '') betaUV = rNULL__
if(ar__(135:138) .EQ. '') e_betaUV = rNULL__
RAdeg = rNULL__
DEdeg = rNULL__
c Derive coordinates RAdeg and DEdeg from input data
c (RAdeg and DEdeg are set to rNULL__ when unknown)
if(RAh .GT. -180) RAdeg=RAh*15.
if(RAm .GT. -180) RAdeg=RAdeg+RAm/4.
if(RAs .GT. -180) RAdeg=RAdeg+RAs/240.
if(DEd .GE. 0) DEdeg=DEd
if(DEm .GE. 0) DEdeg=DEdeg+DEm/60.
if(DEs .GE. 0) DEdeg=DEdeg+DEs/3600.
if(DE_.EQ.'-'.AND.DEdeg.GE.0) DEdeg=-DEdeg
c ..............Just test output...........
write(6,1)
+ RAh,RAm,RAs,DE_,DEd,DEm,DEs,RACh,RACm,RACs,DEC_,DECd,DECm,
+ DECs,S450,e_S450,S850,e_S850,z,e_z,f_z,logM_,e_logM_,logLUV,
+ e_logLUV,logLIR,e_logLIR,Td,e_Td,betaUV,e_betaUV,flag
write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
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,RAm_1,RAs_1,DE__1,DEd_1,DEm_1,DEs_1,RACh_1,RACm_1,
+ RACs_1,DEC__1,DECd_1,DECm_1,DECs_1,S450_1,e_S450_1,S850_1,
+ e_S850_1,z_1,e_z_1,f_z_1,logM__1,e_logM__1,logLUV_1,
+ e_logLUV_1,logLIR_1,e_logLIR_1,Td_1,e_Td_1,betaUV_1,
+ e_betaUV_1,flag_1
if(ar__1(60:64) .EQ. '') S850_1 = rNULL__
if(ar__1(66:69) .EQ. '') e_S850_1 = rNULL__
if(ar__1(71:74) .EQ. '') z_1 = rNULL__
if(ar__1(76:79) .EQ. '') e_z_1 = rNULL__
if(ar__1(83:87) .EQ. '') logM__1 = rNULL__
if(ar__1(89:92) .EQ. '') e_logM__1 = rNULL__
if(ar__1(94:98) .EQ. '') logLUV_1 = rNULL__
if(ar__1(100:103) .EQ. '') e_logLUV_1 = rNULL__
if(ar__1(116:120) .EQ. '') Td_1 = rNULL__
if(ar__1(122:126) .EQ. '') e_Td_1 = rNULL__
if(ar__1(128:133) .EQ. '') betaUV_1 = rNULL__
if(ar__1(135:138) .EQ. '') e_betaUV_1 = rNULL__
RAdeg_1 = rNULL__
DEdeg_1 = 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 .GT. -180) RAdeg_1=RAh_1*15.
if(RAm_1 .GT. -180) RAdeg_1=RAdeg_1+RAm_1/4.
if(RAs_1 .GT. -180) RAdeg_1=RAdeg_1+RAs_1/240.
if(DEd_1 .GE. 0) DEdeg_1=DEd_1
if(DEm_1 .GE. 0) DEdeg_1=DEdeg_1+DEm_1/60.
if(DEs_1 .GE. 0) DEdeg_1=DEdeg_1+DEs_1/3600.
if(DE__1.EQ.'-'.AND.DEdeg_1.GE.0) DEdeg_1=-DEdeg_1
c ..............Just test output...........
write(6,2)
+ RAh_1,RAm_1,RAs_1,DE__1,DEd_1,DEm_1,DEs_1,RACh_1,RACm_1,
+ RACs_1,DEC__1,DECd_1,DECm_1,DECs_1,S450_1,e_S450_1,S850_1,
+ e_S850_1,z_1,e_z_1,f_z_1,logM__1,e_logM__1,logLUV_1,
+ e_logLUV_1,logLIR_1,e_logLIR_1,Td_1,e_Td_1,betaUV_1,
+ e_betaUV_1,flag_1
write(6,'(6H Pos: 2F8.4)') RAdeg_1,DEdeg_1
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,RAm_2,RAs_2,DE__2,DEd_2,DEm_2,DEs_2,RAOh,RAOm,RAOs,DEO_,
+ DEOd,DEOm,DEOs,rmag,e_rmag,Ksmag,e_Ksmag,S3_6,e_S3_6,S250,
+ e_S250,S450_2,e_S450_2,S850_2,e_S850_2,SC,e_SC
if(ar__2(25:26) .EQ. '') RAOh = iNULL__
if(ar__2(28:29) .EQ. '') RAOm = iNULL__
if(ar__2(31:35) .EQ. '') RAOs = rNULL__
if(ar__2(38:38) .EQ. '') DEOd = iNULL__
if(ar__2(40:41) .EQ. '') DEOm = iNULL__
if(ar__2(43:47) .EQ. '') DEOs = rNULL__
if(ar__2(49:53) .EQ. '') rmag = rNULL__
if(ar__2(55:58) .EQ. '') e_rmag = rNULL__
if(ar__2(60:64) .EQ. '') Ksmag = rNULL__
if(ar__2(66:69) .EQ. '') e_Ksmag = rNULL__
if(ar__2(71:75) .EQ. '') S3_6 = rNULL__
if(ar__2(77:80) .EQ. '') e_S3_6 = rNULL__
if(ar__2(104:108) .EQ. '') S850_2 = rNULL__
if(ar__2(110:113) .EQ. '') e_S850_2 = rNULL__
RAdeg_2 = rNULL__
DEdeg_2 = 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 .GT. -180) RAdeg_2=RAh_2*15.
if(RAm_2 .GT. -180) RAdeg_2=RAdeg_2+RAm_2/4.
if(RAs_2 .GT. -180) RAdeg_2=RAdeg_2+RAs_2/240.
if(DEd_2 .GE. 0) DEdeg_2=DEd_2
if(DEm_2 .GE. 0) DEdeg_2=DEdeg_2+DEm_2/60.
if(DEs_2 .GE. 0) DEdeg_2=DEdeg_2+DEs_2/3600.
if(DE__2.EQ.'-'.AND.DEdeg_2.GE.0) DEdeg_2=-DEdeg_2
c ..............Just test output...........
write(6,3)
+ RAh_2,RAm_2,RAs_2,DE__2,DEd_2,DEm_2,DEs_2,RAOh,RAOm,RAOs,DEO_,
+ DEOd,DEOm,DEOs,rmag,e_rmag,Ksmag,e_Ksmag,S3_6,e_S3_6,S250,
+ e_S250,S450_2,e_S450_2,S850_2,e_S850_2,SC,e_SC
write(6,'(6H Pos: 2F8.4)') RAdeg_2,DEdeg_2
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,RAm_3,RAs_3,DE__3,DEd_3,DEm_3,DEs_3,RAOh_1,RAOm_1,
+ RAOs_1,DEO__1,DEOd_1,DEOm_1,DEOs_1,rmag_1,e_rmag_1,Ksmag_1,
+ e_Ksmag_1,S3_6_1,e_S3_6_1,S250_1,e_S250_1,S450_3,e_S450_3,
+ S850_3,e_S850_3,SC_1,e_SC_1
if(ar__3(25:26) .EQ. '') RAOh_1 = iNULL__
if(ar__3(28:29) .EQ. '') RAOm_1 = iNULL__
if(ar__3(31:35) .EQ. '') RAOs_1 = rNULL__
if(ar__3(38:38) .EQ. '') DEOd_1 = iNULL__
if(ar__3(40:41) .EQ. '') DEOm_1 = iNULL__
if(ar__3(43:47) .EQ. '') DEOs_1 = rNULL__
if(ar__3(49:53) .EQ. '') rmag_1 = rNULL__
if(ar__3(55:58) .EQ. '') e_rmag_1 = rNULL__
if(ar__3(60:64) .EQ. '') Ksmag_1 = rNULL__
if(ar__3(66:69) .EQ. '') e_Ksmag_1 = rNULL__
if(ar__3(71:75) .EQ. '') S3_6_1 = rNULL__
if(ar__3(77:80) .EQ. '') e_S3_6_1 = rNULL__
if(ar__3(104:108) .EQ. '') S850_3 = rNULL__
if(ar__3(110:113) .EQ. '') e_S850_3 = rNULL__
RAdeg_3 = rNULL__
DEdeg_3 = 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 .GT. -180) RAdeg_3=RAh_3*15.
if(RAm_3 .GT. -180) RAdeg_3=RAdeg_3+RAm_3/4.
if(RAs_3 .GT. -180) RAdeg_3=RAdeg_3+RAs_3/240.
if(DEd_3 .GE. 0) DEdeg_3=DEd_3
if(DEm_3 .GE. 0) DEdeg_3=DEdeg_3+DEm_3/60.
if(DEs_3 .GE. 0) DEdeg_3=DEdeg_3+DEs_3/3600.
if(DE__3.EQ.'-'.AND.DEdeg_3.GE.0) DEdeg_3=-DEdeg_3
c ..............Just test output...........
write(6,4)
+ RAh_3,RAm_3,RAs_3,DE__3,DEd_3,DEm_3,DEs_3,RAOh_1,RAOm_1,
+ RAOs_1,DEO__1,DEOd_1,DEOm_1,DEOs_1,rmag_1,e_rmag_1,Ksmag_1,
+ e_Ksmag_1,S3_6_1,e_S3_6_1,S250_1,e_S250_1,S450_3,e_S450_3,
+ S850_3,e_S850_3,SC_1,e_SC_1
write(6,'(6H Pos: 2F8.4)') RAdeg_3,DEdeg_3
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,RAm_4,RAs_4,DE__4,DEd_4,DEm_4,DEs_4,S250_2,e_S250_2,
+ S450_4,e_S450_4,S850_4,e_S850_4
if(ar__4(48:51) .EQ. '') S850_4 = rNULL__
if(ar__4(53:56) .EQ. '') e_S850_4 = rNULL__
RAdeg_4 = rNULL__
DEdeg_4 = 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 .GT. -180) RAdeg_4=RAh_4*15.
if(RAm_4 .GT. -180) RAdeg_4=RAdeg_4+RAm_4/4.
if(RAs_4 .GT. -180) RAdeg_4=RAdeg_4+RAs_4/240.
if(DEd_4 .GE. 0) DEdeg_4=DEd_4
if(DEm_4 .GE. 0) DEdeg_4=DEdeg_4+DEm_4/60.
if(DEs_4 .GE. 0) DEdeg_4=DEdeg_4+DEs_4/3600.
if(DE__4.EQ.'-'.AND.DEdeg_4.GE.0) DEdeg_4=-DEdeg_4
c ..............Just test output...........
write(6,5)
+ RAh_4,RAm_4,RAs_4,DE__4,DEd_4,DEm_4,DEs_4,S250_2,e_S250_2,
+ S450_4,e_S450_4,S850_4,e_S850_4
write(6,'(6H Pos: 2F8.4)') RAdeg_4,DEdeg_4
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end