Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_A/424/79 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-20
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/A+A/424/79 Photometry and Metallicity in ABCG 209 galaxies (Mercurio+, 2004)
*================================================================================
*Transformations of galaxies in the environments of the cluster ABCG 209 at z~0.2
* Mercurio A., Busarello G., Merluzzi P., La Barbera F., Girardi M., Haines C.
* <Astron. Astrophys. 424, 79 (2004)>
* =2004A&A...424...79M
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Photometric parameters for 102 galaxies
integer*4 nr__
parameter (nr__=102) ! Number of records
character*85 ar__ ! Full-size record
C J2000.0 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg (nr__) ! (deg) Right Ascension J2000.0
real*8 DEdeg (nr__) ! (deg) Declination J2000.0
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 Seq (nr__) ! Running number
integer*4 RAh (nr__) ! (h) Right ascension (J2000.0)
integer*4 RAm (nr__) ! (min) Right ascension (J2000.0)
real*4 RAs (nr__) ! (s) Right ascension (J2000.0)
character*1 DE_ (nr__) ! Declination sign (J2000.0)
integer*4 DEd (nr__) ! (deg) Declination (J2000.0)
integer*4 DEm (nr__) ! (arcmin) Declination (J2000.0)
real*4 DEs (nr__) ! (arcsec) Declination (J2000.0)
real*4 Rmag (nr__) ! (mag) R-band Kron magnitude corrected for Galactic
* extinction (1)
real*4 e_Rmag (nr__) ! (mag) rms uncertainty on the R-band Kron magnitude
* determination (2)
real*4 B_R (nr__) ! (mag) B-R colour index
real*4 e_B_R (nr__) ! (mag) rms uncertainty on the color determination (2)
real*4 z (nr__) ! heliocentric corrected redshift
real*4 e_z (nr__) ! rms uncertainty on the redshift
real*4 n (nr__) ! Sersic index
*Note (1): Correction for foreground Galactic extinction according to
* Schlegel et al. (1998ApJ...500..525S) corresponds to the centre of cluster
*Note (2): Uncertainties in magnitudes and colours are rounded to the
* second decimal place.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table4.dat' ! *Spectral indices for 102 galaxies
integer*4 nr__1
parameter (nr__1=102) ! Number of records
character*172 ar__1 ! Full-size record
integer*4 Seq_1 (nr__1) ! Running number
real*4 D4000 (nr__1) ! ? Strength of the 4000{AA} break
real*4 e_D4000 (nr__1) ! ? rms uncertainty on the 4000{AA} break
* measurement
real*4 EW_OII_ (nr__1) ! (0.1nm) ? [OII] equivalent width (1)
real*4 e_EW_OII_ (nr__1) ! (0.1nm) ? rms uncertainty on OII equivalent width
real*4 EWHdA (nr__1) ! (0.1nm) H{delta},A equivalent width
real*4 e_EWHdA (nr__1) ! (0.1nm) rms uncertainty on H{delta},A equivalent width
real*4 EWHgA (nr__1) ! (0.1nm) H{gamma},A equivalent width
real*4 e_EWHgA (nr__1) ! (0.1nm) rms uncertainty on H{gamma},A equivalent width
real*4 EWFe4531 (nr__1) ! (0.1nm) Fe4531 equivalent width
real*4 e_EWFe4531 (nr__1) ! (0.1nm) rms uncertainty on Fe4531 equivalent width
real*4 EWHb (nr__1) ! (0.1nm) H{beta} equivalent width
real*4 e_EWHb (nr__1) ! (0.1nm) rms uncertainty on H_beta equivalent width
real*4 EW_OIII_ (nr__1) ! (0.1nm) Equivalent width of [OIII]
real*4 e_EW_OIII_ (nr__1) ! (0.1nm) rms uncertainty on [OIII] equivalent width
real*4 EWFe5015 (nr__1) ! (0.1nm) Fe5015 equivalent width
real*4 e_EWFe5015 (nr__1) ! (0.1nm) rms uncertainty on Fe5015 equivalent width
real*4 Mg1 (nr__1) ! (mag) Mg1 index
real*4 e_Mg1 (nr__1) ! (mag) rms uncertainty on Mg1 index
real*4 Mg2 (nr__1) ! (mag) Mg2 index
real*4 e_Mg2 (nr__1) ! (mag) rms uncertainty on Mg2 index
real*4 Mgb (nr__1) ! (0.1nm) Mgb index
real*4 e_Mgb (nr__1) ! (0.1nm) rms uncertainty on Mgb index
real*4 EWFe5270 (nr__1) ! (0.1nm) H{beta} equivalent width
real*4 e_EWFe5270 (nr__1) ! (0.1nm) rms uncertainty on Fe5270 equivalent width
real*4 EWFe5335 (nr__1) ! (0.1nm) Fe5335 equivalent width
real*4 e_EWFe5335 (nr__1) ! (0.1nm) rms uncertainty on Fe5335 equivalent width
real*4 EWHa (nr__1) ! (0.1nm) ? H{alpha} equivalent width (1)
real*4 e_EWHa (nr__1) ! (0.1nm) ? rms uncertainty on H_alpha equivalent width
character*9 Class (nr__1) ! Spectral classification (2)
*Note (1): A value of '0.0' for the equivalent width for an emission-line
* indicates that no emission is observed, whereas '---' indicates that
* the equivalent width could not be measured as the line does not lie
* within the available wavelength range.
*Note (2): Spectral classification:
* ELG: emission line galaxies;
* HDS_blue: H{delta} strong galaxies with blue colour;
* HDS_red: H{delta} strong galaxies with red colour;
* P: passive evolving galaxies;
* Ab-spirals: passive evolving disk-dominated galaxies (n_Sersic_<=2).
* Galaxy 62 presents very strong [OII], [OIII] and H{alpha} emission,
* that could suggest the presence of an AGN. However, our data do not
* allow a reliable classification, leading us to exclude this object
* from the analysis..
C=============================================================================
C Loading file 'table1.dat' ! Photometric parameters for 102 galaxies
C Format for file interpretation
1 format(
+ I3,2X,I2,2X,I2,2X,F5.2,3X,A1,I2,2X,I2,2X,F4.1,3X,F5.2,3X,F4.2,
+ 2X,F4.2,3X,F4.2,2X,F6.4,3X,F6.4,2X,F3.1)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,102
read(1,'(A85)')ar__
read(ar__,1)
+ Seq(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),Rmag(i__),e_Rmag(i__),B_R(i__),e_B_R(i__),
+ z(i__),e_z(i__),n(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)
+ Seq(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),Rmag(i__),e_Rmag(i__),B_R(i__),e_B_R(i__),
+ z(i__),e_z(i__),n(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 'table4.dat' ! *Spectral indices for 102 galaxies
C Format for file interpretation
2 format(
+ I3,1X,F4.2,1X,F4.2,1X,F5.1,1X,F3.1,2X,F4.1,1X,F3.1,1X,F5.1,1X,
+ F3.1,2X,F4.1,1X,F3.1,1X,F5.1,1X,F3.1,1X,F5.1,1X,F3.1,1X,F5.1,
+ 1X,F3.1,3X,F4.2,1X,F4.2,2X,F4.2,1X,F4.2,2X,F4.1,1X,F3.1,1X,
+ F5.1,1X,F3.1,2X,F4.1,1X,F3.1,1X,F6.1,1X,F3.1,2X,A9)
C Effective file loading
open(unit=1,status='old',file=
+'table4.dat')
write(6,*) '....Loading file: table4.dat'
do i__=1,102
read(1,'(A172)')ar__1
read(ar__1,2)
+ Seq_1(i__),D4000(i__),e_D4000(i__),EW_OII_(i__),
+ e_EW_OII_(i__),EWHdA(i__),e_EWHdA(i__),EWHgA(i__),
+ e_EWHgA(i__),EWFe4531(i__),e_EWFe4531(i__),EWHb(i__),
+ e_EWHb(i__),EW_OIII_(i__),e_EW_OIII_(i__),EWFe5015(i__),
+ e_EWFe5015(i__),Mg1(i__),e_Mg1(i__),Mg2(i__),e_Mg2(i__),
+ Mgb(i__),e_Mgb(i__),EWFe5270(i__),e_EWFe5270(i__),
+ EWFe5335(i__),e_EWFe5335(i__),EWHa(i__),e_EWHa(i__),Class(i__)
if(ar__1(5:8) .EQ. '') D4000(i__) = rNULL__
if(ar__1(10:13) .EQ. '') e_D4000(i__) = rNULL__
if(ar__1(15:19) .EQ. '') EW_OII_(i__) = rNULL__
if(ar__1(21:23) .EQ. '') e_EW_OII_(i__) = rNULL__
if(ar__1(138:143) .EQ. '') EWHa(i__) = rNULL__
if(ar__1(145:147) .EQ. '') e_EWHa(i__) = rNULL__
c ..............Just test output...........
write(6,2)
+ Seq_1(i__),D4000(i__),e_D4000(i__),EW_OII_(i__),
+ e_EW_OII_(i__),EWHdA(i__),e_EWHdA(i__),EWHgA(i__),
+ e_EWHgA(i__),EWFe4531(i__),e_EWFe4531(i__),EWHb(i__),
+ e_EWHb(i__),EW_OIII_(i__),e_EW_OIII_(i__),EWFe5015(i__),
+ e_EWFe5015(i__),Mg1(i__),e_Mg1(i__),Mg2(i__),e_Mg2(i__),
+ Mgb(i__),e_Mgb(i__),EWFe5270(i__),e_EWFe5270(i__),
+ EWFe5335(i__),e_EWFe5335(i__),EWHa(i__),e_EWHa(i__),Class(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end