Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_A/700/A187 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/700/A187 Galactic Miras with light-curve asymmetries (Uttenthaler+, 2025)
*================================================================================
*A population analysis of Galactic Miras with light-curve asymmetries.
* Uttenthaler S., Merchan-Benitez P.
* <Astron. Astrophys. 700, A187 (2025)>
* =2025A&A...700A.187U (SIMBAD/NED BibCode)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table.dat' ! Results of the new analysis of Mira light curves
in this paper
integer*4 nr__
parameter (nr__=3100) ! Number of records
character*44 ar__ ! Full-size record
character*20 Name (nr__) ! Object name in Simbad
real*4 Per (nr__) ! (d) Pulsation period
character*2 SpType (nr__) ! Spectral type
character*8 SRV_ (nr__) ! Classification of SRVs or IR according to GCVS
integer*4 Bumps (nr__) ! [0/1] Presence of light-curve bumps
* (0=no, 1=yes)
real*8 DBSL (nr__) ! (mag) ? DBSL parameter in K-[22] vs. P (Sect. 5.2) (1)
*Note (1): We propose a new parameter that we call the distance to the best
* separation line (DBSL), defined as the distance between the observed colour
* index of a Mira from the line that best separates the Group A and S Miras in
* that colour index versus period P (Eqs. 2 and 3), given by the expressions:
*
* Eq. (4): {delta}_K-[22]_=(K-[22])-(0.011xP-1.380) [mag]
* Eq. (5): {delta}_[3.4]-[22]_=([3.4]-[22])-(0.0086xP-1.0093) [mag]
C=============================================================================
C Loading file 'table.dat' ! Results of the new analysis of Mira light curves
* in this paper
C Format for file interpretation
1 format(A20,F6.1,A2,A8,I1,F7.3)
C Effective file loading
open(unit=1,status='old',file=
+'table.dat')
write(6,*) '....Loading file: table.dat'
do i__=1,3100
read(1,'(A44)')ar__
read(ar__,1)
+ Name(i__),Per(i__),SpType(i__),SRV_(i__),Bumps(i__),DBSL(i__)
if(ar__(38:44) .EQ. '') DBSL(i__) = rNULL__
c ..............Just test output...........
write(6,1)
+ Name(i__),Per(i__),SpType(i__),SRV_(i__),Bumps(i__),DBSL(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end