Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/686/966 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 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/ApJ/686/966 Spitzer-FLS catalog of clusters of galaxies (Muzzin+, 2008)
*================================================================================
*The evolution of dusty star formation and stellar mass assembly in clusters:
*results from the IRAC 3.6, 4.5, 5.8, and 8.0 {mu}m cluster luminosity functions.
* Muzzin A., Wilson G., Lacy M., Yee H.K.C., Stanford S.A.
* <Astrophys. J., 686, 966-994 (2008)>
* =2008ApJ...686..966M
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! FLS cluster catalog
integer*4 nr__
parameter (nr__=99) ! Number of records
character*86 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 Seq ! Running sequence number
character*14 FLS ! Name (<[MWL2008] FLS JHHMMSS+DDMM.m> in Simbad)
real*4 zph ! Photometric redshift estimated from red
* sequence color
real*4 zsp ! ? Spectroscopic redshift of galaxies with red
* sequence weights >0.2
integer*4 o_zsp ! ? Number of spectroscopic redshift
integer*4 RAh ! (h) Hour of right ascension (J2000)
integer*4 RAm ! (min) Minute of right ascension (J2000)
real*4 RAs ! (s) Second of right ascension (J2000)
character*1 DE_ ! Declination sign (J2000)
integer*4 DEd ! (deg) Degree of declination (J2000)
integer*4 DEm ! (arcmin) Arcminute of declination (J2000)
real*4 DEs ! (arcsec) Arcsecond of declination (J2000)
integer*4 BgcR ! Cluster richness parameterized by B_gc,R_ (1)
integer*4 e_BgcR ! Error in BgcR
real*4 M200 ! (10+14Msun) M_200_ estimated from BgcR (2)
real*4 R200 ! (Mpc) R_200_ estimated from BgcR (2)
character*7 Note ! Best centroid of the cluster:
* "RS flux" [red sequence] or
* "BCG" [brightest cluster galaxy])
*Note (1): B_gc_ is the correlation amplitude between the cluster center and
* galaxies; the centroid that produces the largest value should be the
* best centroid of the galaxy population. See section 3.8 and 3.9 for
* further details (exoressed in Mpc^1.8^)
*Note (2): Using Muzzin et al. (2007ApJ...663..150M):
* logM_200_=(1.62+/-0.24)logB_gc_+(9.86+/-0.77) and
* logR_200_=(0.53+/-0.09)logB_gc_-(1.42+/-0.29).
* See section 4 for further details.
C=============================================================================
C Loading file 'table1.dat' ! FLS cluster catalog
C Format for file interpretation
1 format(
+ I2,5X,A14,1X,F4.2,1X,F5.3,1X,I2,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,
+ 1X,I2,1X,F4.1,1X,I4,1X,I3,1X,F5.2,1X,F4.2,1X,A7)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,99
read(1,'(A86)')ar__
read(ar__,1)
+ Seq,FLS,zph,zsp,o_zsp,RAh,RAm,RAs,DE_,DEd,DEm,DEs,BgcR,e_BgcR,
+ M200,R200,Note
if(ar__(28:32) .EQ. '') zsp = rNULL__
if(ar__(34:35) .EQ. '') o_zsp = iNULL__
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)
+ Seq,FLS,zph,zsp,o_zsp,RAh,RAm,RAs,DE_,DEd,DEm,DEs,BgcR,e_BgcR,
+ M200,R200,Note
write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end