Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/723/993 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-12
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/723/993 Spatial extent of (U)LIRGs in the MIR. I. (Diaz-Santos+, 2010)
*================================================================================
*The spatial extent of (U)LIRGs in the mid-infrared.
*I. The continuum emission.
* Diaz-Santos T., Charmandaris V., Armus L., Petric A.O., Howell J.H.,
* Murphy E.J., Mazzarella J.M., Veilleux S., Bothun G., Inami H.,
* Appleton P.N., Evans A.S., Haan S., Marshall J.A., Sanders D.B.,
* Stierwalt S., Surace J.A.
* <Astrophys. J., 723, 993-1005 (2010)>
* =2010ApJ...723..993D
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Properties of the sample
integer*4 nr__
parameter (nr__=221) ! Number of records
character*88 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)
character*20 Name (nr__) ! Galaxy name (1)
integer*4 RAh (nr__) ! (h) Hour of Right Ascension (J2000)
integer*4 RAm (nr__) ! (min) Minute of Right Ascension (J2000)
real*4 RAs (nr__) ! (s) Second of Right Ascension (J2000)
character*1 DE_ (nr__) ! Sign of the Declination (J2000)
integer*4 DEd (nr__) ! (deg) Degree of Declination (J2000)
integer*4 DEm (nr__) ! (arcmin) Arcminute of Declination (J2000)
integer*4 DEs (nr__) ! (arcsec) Arcsecond of Declination (J2000)
real*4 Dist (nr__) ! (Mpc) Luminosity distance (2)
real*4 logL (nr__) ! ([Lsun]) Log IR luminosity
real*4 FEE (nr__) ! Fraction of extended emission at 13.2{MU}m
real*4 e_FEE (nr__) ! Uncertainty in FEE
real*4 Size (nr__) ! (kpc) Core size, FHWM, at 13.2{MU}m
real*4 e_Size (nr__) ! (kpc) Uncertainty in Size
character*1 u_Size (nr__) ! [*:] Unresolved core or uncertain size (3)
real*4 logR (nr__) ! ([-]) ? Log IRAS 60/100um band flux density ratio (4)
real*4 e_logR (nr__) ! ([-]) ? Uncertainty in logR (4)
*Note (1): Multiple systems are indicated with the same name but providing the
* right ascension and declination of the individual galaxies.
*Note (2): See Armus et al. 2009PASP..121..559A, for details. LogL is accurate to
* within 0.01 dex (U et al. 2011, in preparation).
*Note (3): Flag as follows:
* * = unresolved cores (FWHM within 10% of that of the unresolved
* stellar PSF).
* : = galaxy whose IRS spectra has been contaminated by a close companion
* galaxy. In this cases, the Frac and the core size are not reliable.
*Note (4): Values are given only for sources with a unique IRAS color, i.e.,
* not associated to two individual galaxies.
C=============================================================================
C Loading file 'table1.dat' ! Properties of the sample
C Format for file interpretation
1 format(
+ A20,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,I2,1X,F5.1,1X,F5.2,
+ 1X,F4.2,1X,F4.2,1X,F5.2,1X,F4.2,A1,1X,F6.3,1X,F5.3)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,221
read(1,'(A88)')ar__
read(ar__,1)
+ Name(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),Dist(i__),logL(i__),FEE(i__),e_FEE(i__),
+ Size(i__),e_Size(i__),u_Size(i__),logR(i__),e_logR(i__)
if(ar__(77:82) .EQ. '') logR(i__) = rNULL__
if(ar__(84:88) .EQ. '') e_logR(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)
+ Name(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),Dist(i__),logL(i__),FEE(i__),e_FEE(i__),
+ Size(i__),e_Size(i__),u_Size(i__),logR(i__),e_logR(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end