Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJS/213/25 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 2026-Oct-15
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/ApJS/213/25 WISE Massive & Distant Clusters (MaDCoWS). II. (Stanford+, 2014)
*================================================================================
*The Massive and Distant Clusters of WISE Survey.
*II. Initial spectroscopic confirmation of z~1 galaxy clusters selected from
*10,000 deg^2^.
* Stanford S.A., Gonzalez A.H., Brodwin M., Gettings D.P., Eisenhardt P.R.M.,
* Stern D., Wylezalek D.
* <Astrophys. J. Suppl. Ser., 213, 25 (2014)>
* =2014ApJS..213...25S
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Follow-up observations
integer*4 nr__
parameter (nr__=19) ! Number of records
character*87 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)
character*9 MOO ! Cluster identifier (HHMM+DDMM; J2000) (1)
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_ ! Sign of declination (J2000)
integer*4 DEd ! (deg) Degree of declination (J2000)
integer*4 DEm ! (arcmin) Arcminute of declination (J2000)
integer*4 DEs ! (arcsec) Arcsecond of declination (J2000)
character*8 Im ! Imaging
character*42 Inst ! Spectroscopy instrument and UT dates
*Note (1): MOO stands for MaDCoWS Overdense Object.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Redshifts of spectroscopic members
integer*4 nr__1
parameter (nr__1=220) ! Number of records
character*53 ar__1 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_1 ! (deg) Right Ascension J2000
real*8 DEdeg_1 ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
character*9 MOO_1 ! Cluster identifier (HHMM+DDMM; J2000) (1)
integer*4 Seq ! [7/15580] Object identifier (1)
integer*4 RAh_1 ! (h) Hour of Right Ascension (J2000)
integer*4 RAm_1 ! (min) Minute of Right Ascension (J2000)
real*4 RAs_1 ! (s) Second of Right Ascension (J2000)
character*1 DE__1 ! Sign of the Declination (J2000)
integer*4 DEd_1 ! (deg) Degree of Declination (J2000)
integer*4 DEm_1 ! (arcmin) Arcminude of Declination (J2000)
real*4 DEs_1 ! (arcsec) Arcsecond of Declination (J2000)
real*4 z ! [0.7/1.3] Spectroscopic redshift
character*1 q_z ! Redshift quality (A=best) (2)
character*1 Type ! Source type (3)
*Note (1): The object ID is created from the cluster MOO ID followed by
* the sequence of the object.
*Note (2): Quality flag as follows:
* A = high degree of certainty based on multiple features;
* B = reasonable certainty based on at least two features.
*Note (3): Source type as follows:
* E = the optical spectrum has an emission line (nearly always
* [O II] {lambda}3727);
* A = an absorption line (Ca H+K, D4000) spectrum.
C=============================================================================
C Loading file 'table1.dat' ! Follow-up observations
C Format for file interpretation
1 format(
+ 5X,A9,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,I2,1X,A8,1X,A42)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,19
read(1,'(A87)')ar__
read(ar__,1)MOO,RAh,RAm,RAs,DE_,DEd,DEm,DEs,Im,Inst
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)MOO,RAh,RAm,RAs,DE_,DEd,DEm,DEs,Im,Inst
write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table2.dat' ! Redshifts of spectroscopic members
C Format for file interpretation
2 format(
+ 3X,A9,1X,I5,1X,I2,1X,I2,1X,F6.3,1X,A1,I2,1X,I2,1X,F4.1,1X,
+ F5.3,1X,A1,1X,A1)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,220
read(1,'(A53)')ar__1
read(ar__1,2)
+ MOO_1,Seq,RAh_1,RAm_1,RAs_1,DE__1,DEd_1,DEm_1,DEs_1,z,q_z,Type
RAdeg_1 = rNULL__
DEdeg_1 = rNULL__
c Derive coordinates RAdeg_1 and DEdeg_1 from input data
c (RAdeg_1 and DEdeg_1 are set to rNULL__ when unknown)
if(RAh_1 .GT. -180) RAdeg_1=RAh_1*15.
if(RAm_1 .GT. -180) RAdeg_1=RAdeg_1+RAm_1/4.
if(RAs_1 .GT. -180) RAdeg_1=RAdeg_1+RAs_1/240.
if(DEd_1 .GE. 0) DEdeg_1=DEd_1
if(DEm_1 .GE. 0) DEdeg_1=DEdeg_1+DEm_1/60.
if(DEs_1 .GE. 0) DEdeg_1=DEdeg_1+DEs_1/3600.
if(DE__1.EQ.'-'.AND.DEdeg_1.GE.0) DEdeg_1=-DEdeg_1
c ..............Just test output...........
write(6,2)
+ MOO_1,Seq,RAh_1,RAm_1,RAs_1,DE__1,DEd_1,DEm_1,DEs_1,z,q_z,Type
write(6,'(6H Pos: 2F8.4)') RAdeg_1,DEdeg_1
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end