Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJS/203/33 into FORTRAN code for reading data files line by line.
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-16
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/ApJS/203/33 2MASS interferometric calibrator candidates (Richichi+, 2012)
*================================================================================
*A catalog of near-IR sources found to be unresolved with milliarcsecond
*resolution.
* Richichi A., Fors O., Cusano F., Moerchen M.
* <Astrophys. J. Suppl. Ser., 203, 33 (2012)>
* =2012ApJS..203...33R
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! List of sources found unresolved by the lunar
occultation technique
integer*4 nr__
parameter (nr__=556) ! Number of records
character*187 ar__ ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg ! (deg) Right Ascension J2000
real*8 DEdeg ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
character*17 v2MASS ! 2MASS identifier (HHMMSSss+DDMMSSs; J2000)
character*15 OurID ! ESO Period number/sequential identifier (1)
character*1 f_OurID ! [*] * = sources observed with a narrow band
* filter
character*24 Simbad ! Simbad identifier
integer*4 RAh ! (h) Hour of Right Ascension (J2000) (2)
integer*4 RAm ! (min) Minute of Right Ascension (J2000)
real*4 RAs ! (s) Second of Right Ascension (J2000)
character*1 DE_ ! Sign of the Declination (J2000) (2)
integer*4 DEd ! (deg) Degree of Declination (J2000) (2)
integer*4 DEm ! (arcmin) Arcminute of Declination (J2000)
real*4 DEs ! (arcsec) Arcsecond of Declination (J2000)
real*4 Bmag ! (mag) ? Simbad B band magnitude
real*4 Vmag ! (mag) ? Simbad V band magnitude
real*4 Jmag ! (mag) ? 2MASS J band magnitude
real*4 Hmag ! (mag) ? 2MASS H band magnitude
real*4 Kmag ! (mag) ? 2MASS Ks band magnitude
character*9 SpType ! MK spectral type
integer*4 Nref ! [1/106]? Number of ADS references
character*41 OType ! Simbad object type(s)
real*4 SNR ! [10/378.5] Signal-to-noise ratio
real*4 Klim ! (mag) [8.2/12.8] K-band limiting magnitude
real*4 Res ! (mas) [0.25/8.1] Limiting angular resolution; see
* Section 2
character*2 Var ! [FS] Variability flag (3)
*Note (1): Our own ID number, which combines the ESO Period number with the entry
* in our database.
*Note (2): Coordinates, added by CDS, for rows #190 and #268 according to 2MASS
* names.
*Note (3): Flag as follows:
* S = a source belonging to categories such as Miras, emission-line stars,
* RR Lyr or other kind of variables.
* F = a source for which our measured counts differed from the counts
* expected on the basis of the 2MASS K_s_ value by more than 0.6 mag
* (see also Fig. 8).
C=============================================================================
C Loading file 'table1.dat' ! List of sources found unresolved by the lunar
* occultation technique
C Format for file interpretation
1 format(
+ A17,1X,A15,A1,1X,A24,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,
+ F4.1,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,A9,1X,I3,1X,
+ A41,1X,F5.1,1X,F4.1,1X,F4.2,1X,A2)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,556
read(1,'(A187)')ar__
read(ar__,1)
+ v2MASS,OurID,f_OurID,Simbad,RAh,RAm,RAs,DE_,DEd,DEm,DEs,Bmag,
+ Vmag,Jmag,Hmag,Kmag,SpType,Nref,OType,SNR,Klim,Res,Var
if(ar__(84:88) .EQ. '') Bmag = rNULL__
if(ar__(90:94) .EQ. '') Vmag = rNULL__
if(ar__(96:100) .EQ. '') Jmag = rNULL__
if(ar__(102:106) .EQ. '') Hmag = rNULL__
if(ar__(108:112) .EQ. '') Kmag = rNULL__
if(ar__(124:126) .EQ. '') Nref = iNULL__
RAdeg = rNULL__
DEdeg = rNULL__
c Derive coordinates RAdeg and DEdeg from input data
c (RAdeg and DEdeg are set to rNULL__ when unknown)
if(RAh .GT. -180) RAdeg=RAh*15.
if(RAm .GT. -180) RAdeg=RAdeg+RAm/4.
if(RAs .GT. -180) RAdeg=RAdeg+RAs/240.
if(DEd .GE. 0) DEdeg=DEd
if(DEm .GE. 0) DEdeg=DEdeg+DEm/60.
if(DEs .GE. 0) DEdeg=DEdeg+DEs/3600.
if(DE_.EQ.'-'.AND.DEdeg.GE.0) DEdeg=-DEdeg
c ..............Just test output...........
write(6,1)
+ v2MASS,OurID,f_OurID,Simbad,RAh,RAm,RAs,DE_,DEd,DEm,DEs,Bmag,
+ Vmag,Jmag,Hmag,Kmag,SpType,Nref,OType,SNR,Klim,Res,Var
write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end