Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_A/635/A73 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-Sep-12
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/635/A73 Multiplicity study of transiting exoplanet hosts. I. (Bohn+, 2020)
*================================================================================
*A multiplicity study of transiting exoplanet host stars.
*I. High-contrast imaging with VLT/SPHERE .
* Bohn A.J., Southworth, J., Ginski, C., Kenworthy M.A., Maxted P.F.L.,
* Evans D.F.
* <Astron. Astrophys. 635, A73 (2020)>
* =2020A&A...635A..73B (SIMBAD/NED BibCode)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'stars.dat' ! List of studied stars
integer*4 nr__
parameter (nr__=23) ! Number of records
character*95 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)
character*8 Star (nr__) ! Star name
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)
integer*4 Nx (nr__) ! Number of pixels along X-axis
integer*4 Ny (nr__) ! Number of pixels along Y-axis
integer*4 size (nr__) ! (Kibyte) Size of FITS file
character*18 FileName (nr__) ! Name of FITS file, in subdirectory fits
character*31 Title (nr__) ! Title of the FITS file
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Astrometry, photometry, background probability
and derived masses and effective temperatures
of identified candidate companions
integer*4 nr__1
parameter (nr__1=29) ! Number of records
character*101 ar__1 ! Full-size record
character*8 Star_1 (nr__1) ! Host star name around which the companion
* was detected
integer*4 CCID (nr__1) ! ID of the companion candidate
character*10 Date (nr__1) ! ("date") Date of the observation
real*4 Sep (nr__1) ! (arcsec) Separation of the CC
real*4 e_Sep (nr__1) ! (arcsec) Uncertainty of CC separation
real*4 PA (nr__1) ! (deg) Position angle of the CC
real*4 e_PA (nr__1) ! (deg) Uncertainty of the CC PA
real*4 Kmag (nr__1) ! (mag) K band magnitude of the host star,
* corrected for contribution of the CCs
real*4 DeltaK (nr__1) ! (mag) Magnitude difference between primary and CC
real*4 e_DeltaK (nr__1) ! (mag) Uncertainty in magnitude difference between
* primary and CC
character*1 Status (nr__1) ! [ABC] Status of the CC (1)
real*8 pbg (nr__1) ! Probability that CC is background object
real*4 Mass (nr__1) ! (Msun) ? Mass of the CC (2)
real*4 B_Mass (nr__1) ! (Msun) ? Upper threshold for CC mass
real*4 b_Mass_1 (nr__1) ! (Msun) ? Lower threshold for CC mass
integer*4 Teff (nr__1) ! (K) ? Effective temperature of the CC (2)
integer*4 B_Teff (nr__1) ! (K) ? Upper threshold for CC temperature
integer*4 b_Teff_1 (nr__1) ! (K) ? Lower threshold for CC temperature
*Note (1): Status of the CC as follows:
* C = companion
* B = background
* A = ambiguous
*Note (2): No mass and Teff are provided for background objects.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'det-lim.dat' ! Contrast limits of our data reduction for
all targets
integer*4 nr__2
parameter (nr__2=4815) ! Number of records
character*46 ar__2 ! Full-size record
character*8 Star_2 (nr__2) ! Star name
real*4 Sep_1 (nr__2) ! (arcsec) Projected separation
real*4 DeltaKs (nr__2) ! (mag) Magnitude contrast Ks band
real*4 e_DeltaKs (nr__2) ! (mag) Uncertainty of magnitude contrast Ks band
real*4 Masslimit (nr__2) ! (Mjup) Average mass limit
real*4 E_Masslimit(nr__2) ! (Mjup) Upper mass limit
real*4 e_Masslimit_1(nr__2) ! (Mjup) Lower mass limit
C=============================================================================
C Loading file 'stars.dat' ! List of studied stars
C Format for file interpretation
1 format(
+ A8,1X,I2,1X,I2,1X,F5.2,A1,I2,1X,I2,1X,F4.1,1X,I3,1X,I3,1X,I4,
+ 1X,A18,1X,A31)
C Effective file loading
open(unit=1,status='old',file=
+'stars.dat')
write(6,*) '....Loading file: stars.dat'
do i__=1,23
read(1,'(A95)')ar__
read(ar__,1)
+ Star(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),Nx(i__),Ny(i__),size(i__),FileName(i__),
+ Title(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)
+ Star(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),Nx(i__),Ny(i__),size(i__),FileName(i__),
+ Title(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 'table2.dat' ! Astrometry, photometry, background probability
* and derived masses and effective temperatures
* of identified candidate companions
C Format for file interpretation
2 format(
+ A8,1X,I1,1X,A10,1X,F5.3,1X,F5.3,1X,F5.1,1X,F5.1,1X,F5.2,1X,
+ F4.2,1X,F4.2,1X,A1,1X,F7.5,1X,F4.2,1X,F4.2,1X,F4.2,1X,I4,1X,
+ I4,1X,I4)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,29
read(1,'(A101)')ar__1
read(ar__1,2)
+ Star_1(i__),CCID(i__),Date(i__),Sep(i__),e_Sep(i__),PA(i__),
+ e_PA(i__),Kmag(i__),DeltaK(i__),e_DeltaK(i__),Status(i__),
+ pbg(i__),Mass(i__),B_Mass(i__),b_Mass_1(i__),Teff(i__),
+ B_Teff(i__),b_Teff_1(i__)
if(ar__1(73:76) .EQ. '') Mass(i__) = rNULL__
if(ar__1(78:81) .EQ. '') B_Mass(i__) = rNULL__
if(ar__1(83:86) .EQ. '') b_Mass_1(i__) = rNULL__
if(ar__1(88:91) .EQ. '') Teff(i__) = iNULL__
if(ar__1(93:96) .EQ. '') B_Teff(i__) = iNULL__
if(ar__1(98:101) .EQ. '') b_Teff_1(i__) = iNULL__
c ..............Just test output...........
write(6,2)
+ Star_1(i__),CCID(i__),Date(i__),Sep(i__),e_Sep(i__),PA(i__),
+ e_PA(i__),Kmag(i__),DeltaK(i__),e_DeltaK(i__),Status(i__),
+ pbg(i__),Mass(i__),B_Mass(i__),b_Mass_1(i__),Teff(i__),
+ B_Teff(i__),b_Teff_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'det-lim.dat' ! Contrast limits of our data reduction for
* all targets
C Format for file interpretation
3 format(A8,1X,F4.2,1X,F5.2,1X,F5.2,1X,F6.2,1X,F6.2,1X,F6.2)
C Effective file loading
open(unit=1,status='old',file=
+'det-lim.dat')
write(6,*) '....Loading file: det-lim.dat'
do i__=1,4815
read(1,'(A46)')ar__2
read(ar__2,3)
+ Star_2(i__),Sep_1(i__),DeltaKs(i__),e_DeltaKs(i__),
+ Masslimit(i__),E_Masslimit(i__),e_Masslimit_1(i__)
c ..............Just test output...........
write(6,3)
+ Star_2(i__),Sep_1(i__),DeltaKs(i__),e_DeltaKs(i__),
+ Masslimit(i__),E_Masslimit(i__),e_Masslimit_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end