Conversion of standardized ReadMe file for
file /./ftp/cats/J/MNRAS/379/1546 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/MNRAS/379/1546 z'BVRi' photometry of ClG 0016+1609 (Tanaka+, 2007)
*================================================================================
*A huge filamentary structure at z = 0.55 and star formation histories
*of galaxies at z < 1.
* Tanaka M., Hoshi T., Kodama T., Kashikawa N.
* <Mon. Not. R. Astron. Soc., 379, 1546-1556 (2007)>
* =2007MNRAS.379.1546T
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Catalogue of our spectroscopic objects
integer*4 nr__
parameter (nr__=212) ! Number of records
character*94 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*5 v_THK2007_ (nr__) ! Galaxy designation (FN-NN)
character*1 m__THK2007_(nr__) ! [ab] Multiplicity index on [THK2007]
integer*4 RAh (nr__) ! (h) Right ascension (J2000) (1)
integer*4 RAm (nr__) ! (min) Right ascension (J2000) (1)
real*4 RAs (nr__) ! (s) Right ascension (J2000) (1)
character*1 DE_ (nr__) ! Declination sign (J2000) (1)
integer*4 DEd (nr__) ! (deg) Declination (J2000) (1)
integer*4 DEm (nr__) ! (arcmin) Declination (J2000) (1)
real*4 DEs (nr__) ! (arcsec) Declination (J2000) (1)
real*4 z_mag (nr__) ! (mag) Total z' AB magnitude measured in Kron-type
* apertures (mag_auto)
real*4 B_V (nr__) ! (mag) B-V colour index, measured within 2" aperture
real*4 V_R (nr__) ! (mag) V-R colour index, measured within 2" aperture
real*4 R_i_ (nr__) ! (mag) R-i' colour index, measured within 2" aperture
real*4 i__z_ (nr__) ! (mag) i'-z' colour index, measured within 2" aperture
real*4 zphot (nr__) ! ? Photometric redshift (2)
real*4 zspec (nr__) ! Spectroscopic redshift (3)
real*4 zspecm (nr__) ! Minimum value of spectroscopic redshift
* interval (3)
real*4 zspecM_1 (nr__) ! Maximum value of spectroscopic redshift
* interval (3)
integer*4 q_zspec (nr__) ! [0/1] Redshift confidence level (4)
*Note (1): The astrometric calibration is performed against the USNO-B1
* catalogue (Monet et al., 2003, Cat. <I/284>). An accuracy of our
* coordinates is ~0.2".
*Note (2): F5-28 has no photometric redshift due to its close proximity to a
* bright star.
*Note (3): Note that the redshift errors shown here do not include the error
* in the wavelength calibration, which is typically ~0.3{AA}. In some
* cases, two redshifts are obtained for the same object (e.g. F1-13).
* It is likely that two objects lie on the line-of-sight.
*Note (4): Redshift confidence level as follows:
* 0 = Objects with secure/probable redshift estimates
* 1 = Objects with likely redshifts
C=============================================================================
C Loading file 'table2.dat' ! Catalogue of our spectroscopic objects
C Format for file interpretation
1 format(
+ A5,A1,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,2X,F5.2,2X,
+ F4.2,2X,F4.2,2X,F4.2,1X,F5.2,1X,F5.2,2X,F6.4,2X,F6.4,2X,F6.4,
+ 2X,I1)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,212
read(1,'(A94)')ar__
read(ar__,1)
+ v_THK2007_(i__),m__THK2007_(i__),RAh(i__),RAm(i__),RAs(i__),
+ DE_(i__),DEd(i__),DEm(i__),DEs(i__),z_mag(i__),B_V(i__),
+ V_R(i__),R_i_(i__),i__z_(i__),zphot(i__),zspec(i__),
+ zspecm(i__),zspecM_1(i__),q_zspec(i__)
if(ar__(63:67) .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_THK2007_(i__),m__THK2007_(i__),RAh(i__),RAm(i__),RAs(i__),
+ DE_(i__),DEd(i__),DEm(i__),DEs(i__),z_mag(i__),B_V(i__),
+ V_R(i__),R_i_(i__),i__z_(i__),zphot(i__),zspec(i__),
+ zspecm(i__),zspecM_1(i__),q_zspec(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end