Conversion of standardized ReadMe file for
file /./ftp/cats/J/MNRAS/306/857 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 2026-Apr-13
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/306/857 ROSAT Brightest Cluster Sample. III. (Crawford+, 1999)
*================================================================================
*The ROSAT Brightest Cluster Sample -
*III. Optical spectra of the central cluster galaxies.
* Crawford C.S., Allen S.W., Ebeling H., Edge A.C., Fabian A.C.
* <Mon. Not. R. Astron. Soc. 306, 857 (1999)>
* =1999MNRAS.306..857C
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Log of the observations - clusters in the BCS
integer*4 nr__
parameter (nr__=215) ! Number of records
character*109 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*15 Cluster (nr__) ! Cluster name
character*7 m_Cluster (nr__) ! Multiplicity index on Cluster
character*1 n_Cluster (nr__) ! [+] indicates a note detailed in notes.dat
integer*4 RAh (nr__) ! (h) Right ascension (J2000) of BCG
integer*4 RAm (nr__) ! (min) Right ascension (J2000) of BCG
real*4 RAs (nr__) ! (s) Right ascension (J2000) of BCG
character*1 DE_ (nr__) ! Declination sign (J2000) of BCG
integer*4 DEd (nr__) ! (deg) Declination (J2000) of BCG
integer*4 DEm (nr__) ! (arcmin) Declination (J2000) of BCG
integer*4 DEs (nr__) ! (arcsec) Declination (J2000) of BCG
real*4 z (nr__) ! Redshift
character*1 u_z (nr__) ! [)] Uncertainty flag on z
character*3 Line (nr__) ! Note on lines presence (1)
integer*4 Exp (nr__) ! (s) ? Exposition time
real*4 AirM (nr__) ! ? Airmass
real*4 A_V (nr__) ! (mag) ? Absorption in V band
integer*4 PA (nr__) ! (deg) ? Position angle
character*1 n_PA (nr__) ! [+] Note on PA (3)
character*3 Ref (nr__) ! Reference of previous study of the cluster (4)
character*25 Notes (nr__) ! Notes
*Note (1): Presence of lines as follows:
* x = Optical H{alpha}-line emission
* / = no H{alpha}-line emission
* [x] = Clusters that show no obvious line emission, but the expected
* H{alpha} and [NII] complex falls within a region of atmospheric
* absorption, and we cannot completely rule out very low level
* [NII]{lambda}{lambda}6548,6584 line emission.
* N = only [NII]{lambda}{lambda}6548,6584 line emission
*Note (3): "+" marks an observation where the position angle of the slit
* is known not to be at the parallactic angle.
*Note (4): References as follows:
* A92 = Allen et al., 1992MNRAS.259...67A
* C95 = Crawford et al., 1995MNRAS.274...75C
* D96 = This paper, observations of December 1996
* M95 = This paper, observations of May 1995
* M98 = This paper, observations of March 1998
* W94 = White et al., 1994MNRAS.269..589W
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Log of the observations - clusters not included
in either the BCS due to their faint X-ray flux,
declination <0, or low Galactic latitude
integer*4 nr__1
parameter (nr__1=41) ! Number of records
character*109 ar__1 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_1 (nr__1) ! (deg) Right Ascension J2000
real*8 DEdeg_1 (nr__1) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
character*15 Cluster_1 (nr__1) ! Cluster name
character*7 m_Cluster_1(nr__1) ! Multiplicity index on Cluster
character*1 n_Cluster_1(nr__1) ! [+] indicates a note detailed in notes.dat
integer*4 RAh_1 (nr__1) ! (h) Right ascension (J2000) of BCG
integer*4 RAm_1 (nr__1) ! (min) Right ascension (J2000) of BCG
real*4 RAs_1 (nr__1) ! (s) Right ascension (J2000) of BCG
character*1 DE__1 (nr__1) ! Declination sign (J2000) of BCG
integer*4 DEd_1 (nr__1) ! (deg) Declination (J2000) of BCG
integer*4 DEm_1 (nr__1) ! (arcmin) Declination (J2000) of BCG
integer*4 DEs_1 (nr__1) ! (arcsec) Declination (J2000) of BCG
real*4 z_1 (nr__1) ! Redshift
character*1 u_z_1 (nr__1) ! [)] Uncertainty flag on z
character*3 Line_1 (nr__1) ! Note on lines presence (1)
integer*4 Exp_1 (nr__1) ! (s) ? Exposition time
real*4 AirM_1 (nr__1) ! ? Airmass
real*4 A_V_1 (nr__1) ! (mag) ? Absorption in V band
integer*4 PA_1 (nr__1) ! (deg) ? Position angle
character*1 n_PA_1 (nr__1) ! [+] Note on PA (3)
character*3 Ref_1 (nr__1) ! Reference of previous study of the cluster (4)
character*25 Notes_1 (nr__1) ! Notes
*Note (1): Presence of lines as follows:
* x = Optical H{alpha}-line emission
* / = no H{alpha}-line emission
* [x] = Clusters that show no obvious line emission, but the expected
* H{alpha} and [NII] complex falls within a region of atmospheric
* absorption, and we cannot completely rule out very low level
* [NII]{lambda}{lambda}6548,6584 line emission.
* N = only [NII]{lambda}{lambda}6548,6584 line emission
*Note (3): "+" marks an observation where the position angle of the slit
* is known not to be at the parallactic angle.
*Note (4): References as follows:
* A92 = Allen et al., 1992MNRAS.259...67A
* C95 = Crawford et al., 1995MNRAS.274...75C
* D96 = This paper, observations of December 1996
* M95 = This paper, observations of May 1995
* M98 = This paper, observations of March 1998
* W94 = White et al., 1994MNRAS.269..589W
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! Clusters in the BCS for which we do not have a
spectrum of the central cluster galaxy
integer*4 nr__2
parameter (nr__2=38) ! Number of records
character*91 ar__2 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_2 (nr__2) ! (deg) Right Ascension J2000
real*8 DEdeg_2 (nr__2) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
character*15 Cluster_2 (nr__2) ! Cluster name
character*7 m_Cluster_2(nr__2) ! Multiplicity index on Cluster
character*1 n_Cluster_2(nr__2) ! [+] indicates a note in notes.dat file
integer*4 RAh_2 (nr__2) ! (h) Right ascension (J2000)
integer*4 RAm_2 (nr__2) ! (min) Right ascension (J2000)
real*4 RAs_2 (nr__2) ! (s) Right ascension (J2000)
character*1 DE__2 (nr__2) ! Declination sign (J2000)
integer*4 DEd_2 (nr__2) ! (deg) Declination (J2000)
integer*4 DEm_2 (nr__2) ! (arcmin) Declination (J2000)
real*4 DEs_2 (nr__2) ! (arcsec) Declination (J2000)
real*4 z_2 (nr__2) ! Redshift
character*1 Line_2 (nr__2) ! Note on lines presence (1)
character*5 Ref_2 (nr__2) ! Reference (2)
character*27 Notes_2 (nr__2) ! Notes
*Note (1): Presence of lines as follows:
* x = Optical H{alpha}-line emission
* / = No H{alpha}-line emission
*Note (2): References as follows:
* DC95 = Davoust & Considere, 1995A&AS..110...19D
* DSG92 = Donahue et al., 1992ApJ...385...49D
* EHM99 = Ebeling, Henry & Mullis, in preparation:
* GB82 = Gregory & Burns 1982ApJ...255..373G
* LM89 = Laurikainen & Moles, 1989ApJ...345..176L
* LPS92 = Le Borgne, Pello & Sanahuja, 1992A&AS...95...87L
* M97 = Maurogordato et al., 1997A&AS..123..411M
* OLK95 = Owen et al., 1995AJ....109...14O
* OWT88 = Owen et al., 1988AJ.....95....1O
* P78 = Peterson, 1978ApJ...223...74P
* S78 = Sandage, 1978AJ.....83..904S
* SR91 = Struble & Rood, 1991, Cat. <VII/177>
* T93 = Tadhunter et al., 1993MNRAS.263..999T
* U76 = Ulrich, 1976ApJ...206..364U
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'notes.dat' ! Individual notes
integer*4 nr__3
parameter (nr__3=353) ! Number of records
character*80 ar__3 ! Full-size record
character*15 Cluster_3 (nr__3) ! Cluster name
character*65 Note (nr__3) ! text of the note
C=============================================================================
C Loading file 'table1.dat' ! Log of the observations - clusters in the BCS
C Format for file interpretation
1 format(
+ A15,1X,A7,A1,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,I2,1X,F6.4,
+ A1,1X,A3,1X,I4,1X,F5.3,1X,F5.3,1X,I3,A1,1X,A3,1X,A25)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,215
read(1,'(A109)')ar__
read(ar__,1)
+ Cluster(i__),m_Cluster(i__),n_Cluster(i__),RAh(i__),RAm(i__),
+ RAs(i__),DE_(i__),DEd(i__),DEm(i__),DEs(i__),z(i__),u_z(i__),
+ Line(i__),Exp(i__),AirM(i__),A_V(i__),PA(i__),n_PA(i__),
+ Ref(i__),Notes(i__)
if(ar__(59:62) .EQ. '') Exp(i__) = iNULL__
if(ar__(64:68) .EQ. '') AirM(i__) = rNULL__
if(ar__(70:74) .EQ. '') A_V(i__) = rNULL__
if(ar__(76:78) .EQ. '') PA(i__) = iNULL__
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)
+ Cluster(i__),m_Cluster(i__),n_Cluster(i__),RAh(i__),RAm(i__),
+ RAs(i__),DE_(i__),DEd(i__),DEm(i__),DEs(i__),z(i__),u_z(i__),
+ Line(i__),Exp(i__),AirM(i__),A_V(i__),PA(i__),n_PA(i__),
+ Ref(i__),Notes(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table2.dat' ! Log of the observations - clusters not included
* in either the BCS due to their faint X-ray flux,
* declination <0, or low Galactic latitude
C Format for file interpretation
2 format(
+ A15,1X,A7,A1,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,I2,1X,F6.4,
+ A1,1X,A3,1X,I4,1X,F5.3,1X,F5.3,1X,I3,A1,1X,A3,1X,A25)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,41
read(1,'(A109)')ar__1
read(ar__1,2)
+ Cluster_1(i__),m_Cluster_1(i__),n_Cluster_1(i__),RAh_1(i__),
+ RAm_1(i__),RAs_1(i__),DE__1(i__),DEd_1(i__),DEm_1(i__),
+ DEs_1(i__),z_1(i__),u_z_1(i__),Line_1(i__),Exp_1(i__),
+ AirM_1(i__),A_V_1(i__),PA_1(i__),n_PA_1(i__),Ref_1(i__),
+ Notes_1(i__)
if(ar__1(59:62) .EQ. '') Exp_1(i__) = iNULL__
if(ar__1(64:68) .EQ. '') AirM_1(i__) = rNULL__
if(ar__1(70:74) .EQ. '') A_V_1(i__) = rNULL__
if(ar__1(76:78) .EQ. '') PA_1(i__) = iNULL__
RAdeg_1(i__) = rNULL__
DEdeg_1(i__) = 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(i__) .GT. -180) RAdeg_1(i__)=RAh_1(i__)*15.
if(RAm_1(i__) .GT. -180) RAdeg_1(i__)=RAdeg_1(i__)+RAm_1(i__)/4.
if(RAs_1(i__) .GT. -180) RAdeg_1(i__)=RAdeg_1(i__)+RAs_1(i__)/240.
if(DEd_1(i__) .GE. 0) DEdeg_1(i__)=DEd_1(i__)
if(DEm_1(i__) .GE. 0) DEdeg_1(i__)=DEdeg_1(i__)+DEm_1(i__)/60.
if(DEs_1(i__) .GE. 0) DEdeg_1(i__)=DEdeg_1(i__)+DEs_1(i__)/3600.
if(DE__1(i__).EQ.'-'.AND.DEdeg_1(i__).GE.0) DEdeg_1(i__)=-DEdeg_1(i__)
c ..............Just test output...........
write(6,2)
+ Cluster_1(i__),m_Cluster_1(i__),n_Cluster_1(i__),RAh_1(i__),
+ RAm_1(i__),RAs_1(i__),DE__1(i__),DEd_1(i__),DEm_1(i__),
+ DEs_1(i__),z_1(i__),u_z_1(i__),Line_1(i__),Exp_1(i__),
+ AirM_1(i__),A_V_1(i__),PA_1(i__),n_PA_1(i__),Ref_1(i__),
+ Notes_1(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_1(i__),DEdeg_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table3.dat' ! Clusters in the BCS for which we do not have a
* spectrum of the central cluster galaxy
C Format for file interpretation
3 format(
+ A15,1X,A7,A1,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,F4.1,1X,
+ F6.4,1X,A1,1X,A5,2X,A27)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,38
read(1,'(A91)')ar__2
read(ar__2,3)
+ Cluster_2(i__),m_Cluster_2(i__),n_Cluster_2(i__),RAh_2(i__),
+ RAm_2(i__),RAs_2(i__),DE__2(i__),DEd_2(i__),DEm_2(i__),
+ DEs_2(i__),z_2(i__),Line_2(i__),Ref_2(i__),Notes_2(i__)
RAdeg_2(i__) = rNULL__
DEdeg_2(i__) = rNULL__
c Derive coordinates RAdeg_2 and DEdeg_2 from input data
c (RAdeg_2 and DEdeg_2 are set to rNULL__ when unknown)
if(RAh_2(i__) .GT. -180) RAdeg_2(i__)=RAh_2(i__)*15.
if(RAm_2(i__) .GT. -180) RAdeg_2(i__)=RAdeg_2(i__)+RAm_2(i__)/4.
if(RAs_2(i__) .GT. -180) RAdeg_2(i__)=RAdeg_2(i__)+RAs_2(i__)/240.
if(DEd_2(i__) .GE. 0) DEdeg_2(i__)=DEd_2(i__)
if(DEm_2(i__) .GE. 0) DEdeg_2(i__)=DEdeg_2(i__)+DEm_2(i__)/60.
if(DEs_2(i__) .GE. 0) DEdeg_2(i__)=DEdeg_2(i__)+DEs_2(i__)/3600.
if(DE__2(i__).EQ.'-'.AND.DEdeg_2(i__).GE.0) DEdeg_2(i__)=-DEdeg_2(i__)
c ..............Just test output...........
write(6,3)
+ Cluster_2(i__),m_Cluster_2(i__),n_Cluster_2(i__),RAh_2(i__),
+ RAm_2(i__),RAs_2(i__),DE__2(i__),DEd_2(i__),DEm_2(i__),
+ DEs_2(i__),z_2(i__),Line_2(i__),Ref_2(i__),Notes_2(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_2(i__),DEdeg_2(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'notes.dat' ! Individual notes
C Format for file interpretation
4 format(A15,A65)
C Effective file loading
open(unit=1,status='old',file=
+'notes.dat')
write(6,*) '....Loading file: notes.dat'
do i__=1,353
read(1,'(A80)')ar__3
read(ar__3,4)Cluster_3(i__),Note(i__)
c ..............Just test output...........
write(6,4)Cluster_3(i__),Note(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end