Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_A/539/A91 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-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/A+A/539/A91 MASSIV I. Sample properties (Contini+, 2012)
*================================================================================
*MASSIV: Mass Assemby Survey with SINFONI in VVDS.
*I. Survey description and global properties of the 0.9 < z < 1.8 galaxy sample.
* Contini T., Garilli B., Le Fevre O., Kissler-Patig M., Amram P., Epinat B.,
* Moultaka J., Paioro L., Queyrel J., Tasca L., Tresse L., Vergani D.,
* Lopez-Sanjuan C., Perez-Montero E.
* <Astron. Astrophys. 539, A91 (2012)>
* =2012A&A...539A..91C
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table5.dat' ! Global properties of the MASSIV sample
integer*4 nr__
parameter (nr__=84) ! Number of records
character*96 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 VVDS (nr__) ! VVDS identification number, Cat. III/250
integer*4 RAh (nr__) ! (h) Right ascension (J2000)
integer*4 RAm (nr__) ! (min) Right ascension (J2000)
real*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)
real*4 DEs (nr__) ! (arcsec) Declination (J2000)
real*4 z (nr__) ! Galaxy redshift as measured in VIMOS spectra
character*1 n_z (nr__) ! [a] redshift from SINFONI (1)
integer*4 q_z (nr__) ! Redshift associated flag (2)
character*2 S (nr__) ! [D W UD] Depth flag of the VVDS parent
* sample: Deep, Wide, or Ultra-Deep.
real*4 logM_ (nr__) ! ([Msun]) Stellar mass
real*4 e_logM_ (nr__) ! ([Msun]) rms uncertainty on logM*
real*4 logSFR (nr__) ! ([Msun/yr]) SED-based star formation rate
real*4 E_logSFR (nr__) ! ([Msun/yr]) Error on logSFR (upper value)
real*4 e_logSFR_1 (nr__) ! ([Msun/yr]) Error on logSFR (lower value)
real*4 W_OII_ (nr__) ! (0.1nm) ? Equivalent width of [OII]3727
real*4 e_W_OII_ (nr__) ! (0.1nm) ? rms uncertainty on W[OII]
real*4 Flux (nr__) ! (10-20W/m2) ? Flux of [OII]3727
real*4 e_Flux (nr__) ! (10-20W/m2) ? rms uncertainty on Flux
*Note (1): a: For this galaxy, we indicate the redshift derived from
* H{alpha} SINFONI data
*Note (2): See Le Fevre et al. 2005, Cat. III/250.
* The last (rightmost) digit characterises the quality of the redshift:
* 2 = 75% confidence in the redshift
* 3 = 95% confidence
* 4 = 100% confidence
* 9 = Single isolated emission line spectra
* +20 = a secondary identified target, i.e. an object which is present
* by chance in the spectral slit in addition of the primary target;
* thus the secondary object is not ensured to be fully centered
* within the slit
C=============================================================================
C Loading file 'table5.dat' ! Global properties of the MASSIV sample
C Format for file interpretation
1 format(
+ I9,1X,I2,1X,I2,1X,F6.3,1X,A1,I1,1X,I2,1X,F6.3,2X,F6.4,A1,I2,
+ 1X,A2,1X,F5.2,1X,F4.2,1X,F4.2,1X,F4.2,1X,F4.2,1X,F6.1,1X,F4.1,
+ 1X,F4.1,1X,F3.1)
C Effective file loading
open(unit=1,status='old',file=
+'table5.dat')
write(6,*) '....Loading file: table5.dat'
do i__=1,84
read(1,'(A96)')ar__
read(ar__,1)
+ VVDS(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),z(i__),n_z(i__),q_z(i__),S(i__),logM_(i__),
+ e_logM_(i__),logSFR(i__),E_logSFR(i__),e_logSFR_1(i__),
+ W_OII_(i__),e_W_OII_(i__),Flux(i__),e_Flux(i__)
if(ar__(77:82) .EQ. '') W_OII_(i__) = rNULL__
if(ar__(84:87) .EQ. '') e_W_OII_(i__) = rNULL__
if(ar__(89:92) .EQ. '') Flux(i__) = rNULL__
if(ar__(94:96) .EQ. '') e_Flux(i__) = rNULL__
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)
+ VVDS(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),z(i__),n_z(i__),q_z(i__),S(i__),logM_(i__),
+ e_logM_(i__),logSFR(i__),E_logSFR(i__),e_logSFR_1(i__),
+ W_OII_(i__),e_W_OII_(i__),Flux(i__),e_Flux(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end