Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_A/489/1255 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-Jun-08
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/489/1255 HARPS observations of eight galactic Cepheids (Nardetto+, 2008)
*================================================================================
*High resolution spectroscopy for Cepheids distance determination.
*III. A relation between {gamma}-velocities and {gamma}-asymmetries.
* Nardetto N., Stoekl A., Bersier D., Barnes, T.G.
* <Astron. Astrophys. 489, 1255 (2008)>
* =2008A&A...489.1255N
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Observed sample of Cepheids sorted by increasing
period and main results
integer*4 nr__
parameter (nr__=8) ! Number of records
character*62 ar__ ! Full-size record
character*8 Name (nr__) ! Star name
integer*4 HD (nr__) ! HD number
real*8 Per (nr__) ! (d) Pulsation period (1)
real*4 VgGCD (nr__) ! (km/s) GCD {gamma}-velocities (2)
real*4 a0 (nr__) ! Slope of the relation (3)
real*4 e_a0 (nr__) ! Uncertainty on a0
real*4 b0 (nr__) ! (km/s) Zero-Point of the relation (3)
real*4 e_b0 (nr__) ! (km/s) Uncertainty on b0
integer*4 Chi2 (nr__) ! Reduced Chi^2 of the fit
real*4 VgStar (nr__) ! (km/s) Physically calibrated {gamma}-velocity of
* the star (4)
real*4 e_VgStar (nr__) ! (km/s) Uncertainty on VgStar
*Note (1): The corresponding Julian dates (T0) can be found
* in Nardetto et al., 2007A&A...471..661N (Paper II)
*Note (2): gGCD is the {gamma}-velocity of the Galactic Cepheid Database :
* http://www.astro.utoronto.ca/DDO/research/cepheids/
*Note (3): a0 and b0 are respectively the slope and the zero-point of the
* relation Vg(i)-gGCD=a0*Ag(i)+b0, where i correspond to the metallic
* line considered. Vg(i) and Ag(i) can be found in table2.dat
*Note (4): VgStar is defined as VgGCD+b0
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Gamma-velocities and {gamma}-asymmetries
integer*4 nr__1
parameter (nr__1=136) ! Number of records
character*45 ar__1 ! Full-size record
character*8 Name_1 (nr__1) ! Star name
character*4 Ion (nr__1) ! Species metallic spectral line
real*8 Line (nr__1) ! (0.1nm) Wavelength of the spectral line
real*4 Ag (nr__1) ! (%) Gamma-asymmetry in % of the FWHM (1)
real*4 e_Ag (nr__1) ! (%) Uncertainty on Ag
real*4 Vg (nr__1) ! (km/s) Gamma-velocity
real*4 e_Vg (nr__1) ! (km/s) Uncertainty on Vg
*Note (1): Quantity derived from a bi-Gaussian fit. See paper for more detail.
C=============================================================================
C Loading file 'table1.dat' ! Observed sample of Cepheids sorted by increasing
* period and main results
C Format for file interpretation
1 format(
+ A8,1X,I6,1X,F8.5,1X,F5.1,1X,F5.2,1X,F4.2,1X,F3.1,1X,F3.1,1X,
+ I2,1X,F5.1,1X,F3.1)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,8
read(1,'(A62)')ar__
read(ar__,1)
+ Name(i__),HD(i__),Per(i__),VgGCD(i__),a0(i__),e_a0(i__),
+ b0(i__),e_b0(i__),Chi2(i__),VgStar(i__),e_VgStar(i__)
c ..............Just test output...........
write(6,1)
+ Name(i__),HD(i__),Per(i__),VgGCD(i__),a0(i__),e_a0(i__),
+ b0(i__),e_b0(i__),Chi2(i__),VgStar(i__),e_VgStar(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table2.dat' ! Gamma-velocities and {gamma}-asymmetries
C Format for file interpretation
2 format(A8,1X,A4,1X,F8.3,1X,F5.2,1X,F5.2,1X,F5.2,1X,F4.2)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,136
read(1,'(A45)')ar__1
read(ar__1,2)
+ Name_1(i__),Ion(i__),Line(i__),Ag(i__),e_Ag(i__),Vg(i__),
+ e_Vg(i__)
c ..............Just test output...........
write(6,2)
+ Name_1(i__),Ion(i__),Line(i__),Ag(i__),e_Ag(i__),Vg(i__),
+ e_Vg(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end