Conversion of standardized ReadMe file for
file /./ftp/cats/J/AJ/126/1208 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-19
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/AJ/126/1208 UVBI magnitudes and redshifts in HDF-South (Sawicki+, 2003)
*================================================================================
*Redshifts in the Hubble Deep Field South.
* Sawicki M., Mallen-Ornelas G.
* <Astron. J. 126, 1208 (2003)>
* =2003AJ....126.1208S
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! HDFS objects with spectroscopic redshifts
integer*4 nr__
parameter (nr__=103) ! Number of records
character*139 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 v_SM2003_ (nr__) ! Object Identification
integer*4 RAh (nr__) ! (h) Hour of Right Ascension (J2000) (1)
integer*4 RAm (nr__) ! (min) Minute of Right Ascension (J2000) (1)
real*4 RAs (nr__) ! (s) Second of Right Ascension (J2000) (1)
character*1 DE_ (nr__) ! Sign of the Declination (J2000) (1)
integer*4 DEd (nr__) ! (deg) Degree of Declination (J2000) (1)
integer*4 DEm (nr__) ! (arcmin) Arcminute of Declination (J2000) (1)
real*4 DEs (nr__) ! (arcsec) Arcsecond of Declination (J2000) (1)
character*4 Field (nr__) ! Field identification
integer*4 Xpix (nr__) ! (pix) X pixel coordinate
integer*4 Ypix (nr__) ! (pix) Y pixel coordinate
real*4 Imag (nr__) ! (mag) HST I (814 nm) band aperture corrected
* magnitude (2)
real*4 e_Imag (nr__) ! (mag) Error in Imag
real*4 Vmag (nr__) ! (mag) ? HST V (606 nm) band aperture corrected
* magnitude (2)
real*4 e_Vmag (nr__) ! (mag) ? Error in Vmag
real*4 Bmag (nr__) ! (mag) ? HST B (450 nm) band aperture corrected
* magnitude (2)
real*4 e_Bmag (nr__) ! (mag) ? Error in Bmag
real*4 Umag (nr__) ! (mag) ? HST U (300 nm) band aperture corrected
* magnitude (2)
real*4 e_Umag (nr__) ! (mag) ? Error in Umag
real*4 zPhot (nr__) ! ? Photometric redshift
real*4 zSpec (nr__) ! Spectroscopic redshift
character*1 f_zSpec (nr__) ! [*] Indicates blended objects
character*34 Spec (nr__) ! Spectral features used (3)
*Note (1): From the Version 1 images of the HDFS and the Flanking Fields
*Note (2): Magnitudes are AB-normalized (Oke, 1974ApJS...27...21O) using the
* zero-points provided on the STScI HDFS website. See text for more
* details.
*Note (3): The comments are not meant to be an exhaustive list of features seen
* in each spectrum, and simply includes clearly-detected features used
* for redshift measurement.
*
* He5876 refers to He I emission;
* N6548 and N6583 refer to [N II] emission;
* O3727 refers to [O II] emission;
* O4959 and O5007 refer to [O III] emission;
* Ne3869 refers to [Ne III] emission;
* H and K refer to Ca II absorption;
* G refers to G-band absorption;
*
* For the purposes of this table, H{alpha}, H{beta}, H{gamma}, and
* H{delta} refer to emission lines H{eta} and H{zeta} refer to
* absorption lines.
C=============================================================================
C Loading file 'table1.dat' ! HDFS objects with spectroscopic redshifts
C Format for file interpretation
1 format(
+ I5,1X,I2,1X,I2,1X,F6.3,1X,A1,I2,1X,I2,1X,F5.2,1X,A4,1X,I4,1X,
+ I4,1X,F5.2,1X,F4.2,1X,F5.2,1X,F4.2,1X,F5.2,1X,F4.2,1X,F5.2,1X,
+ F4.2,1X,F4.2,1X,F6.4,A1,1X,A34)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,103
read(1,'(A139)')ar__
read(ar__,1)
+ v_SM2003_(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),Field(i__),Xpix(i__),Ypix(i__),Imag(i__),
+ e_Imag(i__),Vmag(i__),e_Vmag(i__),Bmag(i__),e_Bmag(i__),
+ Umag(i__),e_Umag(i__),zPhot(i__),zSpec(i__),f_zSpec(i__),
+ Spec(i__)
if(ar__(59:63) .EQ. '') Vmag(i__) = rNULL__
if(ar__(65:68) .EQ. '') e_Vmag(i__) = rNULL__
if(ar__(70:74) .EQ. '') Bmag(i__) = rNULL__
if(ar__(76:79) .EQ. '') e_Bmag(i__) = rNULL__
if(ar__(81:85) .EQ. '') Umag(i__) = rNULL__
if(ar__(87:90) .EQ. '') e_Umag(i__) = rNULL__
if(ar__(92:95) .EQ. '') zPhot(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)
+ v_SM2003_(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),Field(i__),Xpix(i__),Ypix(i__),Imag(i__),
+ e_Imag(i__),Vmag(i__),e_Vmag(i__),Bmag(i__),e_Bmag(i__),
+ Umag(i__),e_Umag(i__),zPhot(i__),zSpec(i__),f_zSpec(i__),
+ Spec(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end