Conversion of standardized ReadMe file for
file /./ftp/cats/J/AZh/91/382 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-Oct-05
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/AZh/91/382 New variable stars in field SA9 (Sokolovsky+, 2014)
*================================================================================
*New variable stars on digitized plates of the Moscow collection. Field SA9.
* Sokolovsky K.V., Antipin S.V., Zubareva A.M., Kolesnikova D.M.,
* Lebedev A.A., Samus N.N., Sat L.A.
* <Astron. Zh. 91, 382 (2014)>
* =2014AZh....91..382S
* =2014ARep...58..319S
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! New variable stars
integer*4 nr__
parameter (nr__=77) ! Number of records
character*82 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 MDV (nr__) ! [519/595] MDV number
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)
character*4 Type (nr__) ! Variable type
real*4 mMax (nr__) ! (mag) Magnitude at maximum brightness
real*4 mMin (nr__) ! (mag) Magnitude at minimum brightness
character*1 u_mMin (nr__) ! Uncertainty flag on mMin
real*4 mMin2 (nr__) ! (mag) ? Magnitude at second minimum brightness
character*1 u_mMin2 (nr__) ! Uncertainty flag on mMin2
real*8 Epoch (nr__) ! (d) ? Epoch of extremum brightness (JD-2400000)
real*8 Per (nr__) ! (d) ? Period
character*4 Notes (nr__) ! ? Notes (1)
*Note (1): Notes as follows:
* 1 = Type EW with double the period is possible
* 2 = A double star. The eastern star of the pair varies, as confirmed with
* CCD observations. The tabulated coordinates are from the 2MASS catalog
* 3 = Brightness variability and type were confirmed with CCD observations
* 4 = Varies in the NSVS data, which indicate P=9.23d
* 5 = Type RRC with half the period is possible
* 6 = Eccentric orbit; the secondary minimum is at phase 0.465
* 7 = A period of about 8000 days is possible; J-K=0.635 (from 2MASS)
* 8 = Double the period is possible
* 9 = The periods 0.337844d or 0.252442d are possible (type EW in both cases)
* 10 = The period varies. Variable in the NSVS data, which indicate P=1.07213d
* 11 = Probably can be identified with the X-ray source 1RXS J033501.6+623655
* 12 = IRAS 03417+6002. Varies in the NSVS data, which indicate that it may be
* a semi-regular variable (type SR:) with P~92d
C=============================================================================
C Loading file 'table1.dat' ! New variable stars
C Format for file interpretation
1 format(
+ 4X,I3,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,A4,1X,
+ F5.2,1X,F5.2,A1,1X,F5.2,A1,1X,F10.4,1X,F8.6,2X,A4)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,77
read(1,'(A82)')ar__
read(ar__,1)
+ MDV(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),Type(i__),mMax(i__),mMin(i__),u_mMin(i__),
+ mMin2(i__),u_mMin2(i__),Epoch(i__),Per(i__),Notes(i__)
if(ar__(51:55) .EQ. '') mMin2(i__) = rNULL__
if(ar__(58:67) .EQ. '') Epoch(i__) = rNULL__
if(ar__(69:76) .EQ. '') Per(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)
+ MDV(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),Type(i__),mMax(i__),mMin(i__),u_mMin(i__),
+ mMin2(i__),u_mMin2(i__),Epoch(i__),Per(i__),Notes(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end