Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/517/148 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 2024-Apr-16
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/517/148 ISO observations of the CFRS field (Flores+, 1999)
*================================================================================
*15 micron Infrared Space Observatory observations of the 1415+52 Canada-France
*redshift survey field: the cosmic star formation rate as derived from deep
*ultraviolet, optical, mid-infrared, and radio photometry
* Flores H., Hammer F., Thuan T.X., Cesarsky C., Desert F.X., Omont A.,
* Lilly S .J., Eales S., Crampton D., Le Fevre O.
* <Astrophys. J. 517, 148 (1999)>
* =1999ApJ...517..148F (SIMBAD/NED BibCode)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Optical counterparts of ISOCAM LW3 sources
integer*4 nr__
parameter (nr__=85) ! Number of records
character*124 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*10 Catalog (nr__) ! Catalog object was obtained from (1)
integer*4 ISOName (nr__) ! Name in the ISO catalog of Flores et al.
* (1999A&A...343..389)
character*1 n_ISOName (nr__) ! [g] Note on ISOName (2)
integer*4 RAh (nr__) ! (h) Right Ascension (J2000)
integer*4 RAm (nr__) ! (min) Right Ascension (J2000)
real*4 RAs (nr__) ! (s) Right Ascension (J2000)
character*1 DE_ (nr__) ! Declination sign (J2000)
integer*4 DEd (nr__) ! (deg) Declination (J2000)
integer*4 DEm (nr__) ! (arcmin) Declination (J2000)
real*4 DEs (nr__) ! (arcsec) Declination (J2000)
real*8 CFRS (nr__) ! ? Canada-France Redshift Survey number
character*1 n_z (nr__) ! Indicates that a redshift of 0.7217 was
* given by Lilly+ (1995).
character*1 f_ISOName (nr__) ! [s] Indicates object is a star
real*4 z (nr__) ! ? Redshift
real*4 Imag (nr__) ! (mag) ? I band isophotal magnitude in the AB system
real*4 Vmag (nr__) ! (mag) ? V band isophotal magnitude in the AB system
real*4 Kmag (nr__) ! (mag) ? K band isophotal magnitude in the AB system
real*4 Dist (nr__) ! (arcsec) ? Distance between ISO source and optical
* or radio counterpart
real*8 Prob (nr__) ! Associated probability of coincidence of
* sources
character*1 f_Prob (nr__) ! Indicates radio source with probability
* based on radio-source counts
integer*4 Flux (nr__) ! (uJy) Flux density at 12-18 {mu}m within and
* 9'' aperture
integer*4 e_Flux (nr__) ! (uJy) Uncertainty in Flux
*Note (1):
* Catalog 1 = Objects with S/N > 4, Probability < 0.02
* Catalog 2 = Objects with S/N > 4, P(d,I) > 0.02
* Catalog 3 = Objects with S/N > 4, without optical counterpart in I_AB_
* Catalog 4 = Objects with 4 > S/N > 3, Probability < 0.02
* Catalog 5 = Objects with 4 > S/N > 3, Probability > 0.02
* Catalog 6 = Objects with 4 > S/N > 3, without optical counterpart in I_AB_
*Note (2): Hammer et al. (1995MNRAS.276.1085H) and Fomalont et al.
* (1991AJ....102.1258F) comment that the fainter source (I_AB_ {~} 23.9)
* galaxy, which is 2'' away, should be the optical counterpart.
* Unfortunately, no spectrum of the fainter galaxy is available.
C=============================================================================
C Loading file 'table1.dat' ! Optical counterparts of ISOCAM LW3 sources
C Format for file interpretation
1 format(
+ A10,3X,I3,2X,A1,3X,I2,1X,I2,1X,F4.1,A1,I2,1X,I2,1X,F4.1,2X,
+ F7.4,1X,A1,1X,A1,4X,F5.3,4X,F5.2,4X,F5.2,6X,F5.2,4X,F5.2,1X,
+ F9.7,1X,A1,2X,I4,1X,I2)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,85
read(1,'(A124)')ar__
read(ar__,1)
+ Catalog(i__),ISOName(i__),n_ISOName(i__),RAh(i__),RAm(i__),
+ RAs(i__),DE_(i__),DEd(i__),DEm(i__),DEs(i__),CFRS(i__),
+ n_z(i__),f_ISOName(i__),z(i__),Imag(i__),Vmag(i__),Kmag(i__),
+ Dist(i__),Prob(i__),f_Prob(i__),Flux(i__),e_Flux(i__)
if(ar__(46:52) .EQ. '') CFRS(i__) = rNULL__
if(ar__(61:65) .EQ. '') z(i__) = rNULL__
if(ar__(70:74) .EQ. '') Imag(i__) = rNULL__
if(ar__(79:83) .EQ. '') Vmag(i__) = rNULL__
if(ar__(90:94) .EQ. '') Kmag(i__) = rNULL__
if(ar__(99:103) .EQ. '') Dist(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)
+ Catalog(i__),ISOName(i__),n_ISOName(i__),RAh(i__),RAm(i__),
+ RAs(i__),DE_(i__),DEd(i__),DEm(i__),DEs(i__),CFRS(i__),
+ n_z(i__),f_ISOName(i__),z(i__),Imag(i__),Vmag(i__),Kmag(i__),
+ Dist(i__),Prob(i__),f_Prob(i__),Flux(i__),e_Flux(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end