Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/542/673 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-18
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/542/673 Morphological types of galaxies in clusters (Fasano+, 2000)
*================================================================================
*The evolution of the galactic morphological types in clusters.
* Fasano G., Poggianti B.M., Couch W.J., Bettoni D., Kjaergaard P., Moles M.
* <Astrophys. J. 542, 673 (2000)>
* =2000ApJ...542..673F
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Cluster parameters
integer*4 nr__
parameter (nr__=10) ! Number of records
character*67 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 Abell (nr__) ! Cluster number
character*1 n_Abell (nr__) ! [ls] Note on Cluster (1)
real*4 z (nr__) ! Redshift
integer*4 RAh (nr__) ! (h) Right ascension (J2000)
integer*4 RAm (nr__) ! (min) Right ascension (J2000)
integer*4 RAs (nr__) ! (s) Right ascension (J2000)
character*1 DE_ (nr__) ! Declination sign (J2000)
integer*4 DEd (nr__) ! (deg) Declination (J2000)
integer*4 DEm (nr__) ! (arcmin) Declination (J2000)
integer*4 DEs (nr__) ! (arcsec) Declination (J2000)
real*4 E_B_V (nr__) ! (mag) Reddening
integer*4 Run (nr__) ! Run number
real*4 Area (nr__) ! (Mpc+2) Cluster area
real*4 Seeing (nr__) ! (arcsec) Seeing in arcsec
real*4 Seeingpc (nr__) ! (kpc) Seeing in kpc
real*4 rmag (nr__) ! (mag) Gunn r magnitude limit
*Note (1): Two entries for A2192:
* l: Data refers to four contiguous Gunn r images covering a quite large area
* s: Data relates to a smaller part of the cluster, for which (B-Gr) colors
* of galaxies are available, thus allowing a more accurate photometric
* calibration.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! Positions and the morphological classifications
of all galaxies in our sample
integer*4 nr__1
parameter (nr__1=383) ! Number of records
character*59 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)
integer*4 Abell_1 (nr__1) ! Abell cluster number (AAAA)
integer*4 Galaxy (nr__1) ! Galaxy number in Abell cluster (NN)
* ([FPC2000] ACO AAAA NN in Simbad)
integer*4 RAh_1 (nr__1) ! (h) Right Ascension (J2000)
integer*4 RAm_1 (nr__1) ! (min) Right Ascension (J2000)
real*4 RAs_1 (nr__1) ! (s) Right Ascension (J2000)
character*1 DE__1 (nr__1) ! Sign of the Declination (J2000)
integer*4 DEd_1 (nr__1) ! (deg) Declination (J2000)
integer*4 DEm_1 (nr__1) ! (arcmin) Declination (J2000)
real*4 DEs_1 (nr__1) ! (arcsec) Declination (J2000)
character*8 Mtype (nr__1) ! Galaxy morphological type (? indicates
* uncertain classification)
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table5.dat' ! Cluster backgrounds
integer*4 nr__2
parameter (nr__2=23) ! Number of records
character*44 ar__2 ! Full-size record
character*8 Cluster (nr__2) ! Abell Cluster Name
character*8 Sample (nr__2) ! Sample from which cluster data was obtained
* from (1)
real*4 z_1 (nr__2) ! Redshift of the cluster
real*4 EField (nr__2) ! Expected number of field Elliptical
* galaxies (2)
real*4 SOField (nr__2) ! Expected number of field SO type galaxies (2)
real*4 SpField (nr__2) ! Expected number of field Spiral galaxies (2)
*Note (1): References
* OUR = This work
* C98 = Couch W.J., Barger A.J., Smail I., Ellis R.S., Sharples R.M.,
* 1998, Cat. <J/ApJ/497/188>
* MORPHS = Dressler A., Oemler A., Couch W.J., Smail I., Ellis R.S.,
* Barger A., Butcher H., Poggianti B.M., Sharples R.M.,
* 1997ApJ...490..577D
*Note (2): The field galaxies have been determined from the galaxy number
* counts given by Metcalfe et al (1995MNRAS.273..257M) and the breakdown
* into morphological classes (E/S0/Sp=18:27:56) was computed for our
* limiting magnitudes at z{~}0.2 from the fits to the differential
* number counts of the Medium Deep Survey.
C=============================================================================
C Loading file 'table2.dat' ! Cluster parameters
C Format for file interpretation
1 format(
+ 6X,I4,1X,A1,2X,F5.3,2X,I2,1X,I2,1X,I2,1X,A1,I2,1X,I2,1X,I2,2X,
+ F4.2,1X,I1,1X,F3.1,1X,F4.2,1X,F4.2,1X,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,10
read(1,'(A67)')ar__
read(ar__,1)
+ Abell(i__),n_Abell(i__),z(i__),RAh(i__),RAm(i__),RAs(i__),
+ DE_(i__),DEd(i__),DEm(i__),DEs(i__),E_B_V(i__),Run(i__),
+ Area(i__),Seeing(i__),Seeingpc(i__),rmag(i__)
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)
+ Abell(i__),n_Abell(i__),z(i__),RAh(i__),RAm(i__),RAs(i__),
+ DE_(i__),DEd(i__),DEm(i__),DEs(i__),E_B_V(i__),Run(i__),
+ Area(i__),Seeing(i__),Seeingpc(i__),rmag(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 'table3.dat' ! Positions and the morphological classifications
* of all galaxies in our sample
C Format for file interpretation
2 format(
+ 6X,I4,5X,I2,4X,I2,1X,I2,1X,F5.2,3X,A1,I2,1X,I2,1X,F5.2,4X,A8)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,383
read(1,'(A59)')ar__1
read(ar__1,2)
+ Abell_1(i__),Galaxy(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),
+ DE__1(i__),DEd_1(i__),DEm_1(i__),DEs_1(i__),Mtype(i__)
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)
+ Abell_1(i__),Galaxy(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),
+ DE__1(i__),DEd_1(i__),DEm_1(i__),DEs_1(i__),Mtype(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 'table5.dat' ! Cluster backgrounds
C Format for file interpretation
3 format(A8,1X,A8,1X,F5.3,2X,F3.1,2X,F3.1,2X,F4.1)
C Effective file loading
open(unit=1,status='old',file=
+'table5.dat')
write(6,*) '....Loading file: table5.dat'
do i__=1,23
read(1,'(A44)')ar__2
read(ar__2,3)
+ Cluster(i__),Sample(i__),z_1(i__),EField(i__),SOField(i__),
+ SpField(i__)
c ..............Just test output...........
write(6,3)
+ Cluster(i__),Sample(i__),z_1(i__),EField(i__),SOField(i__),
+ SpField(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end