Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/652/458 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 2024-Apr-19 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/ApJ/652/458 BVRH{alpha} photometry of candidates Be stars (Wisniewski+, 2006) *================================================================================ *The role of evolutionary age and metallicity in the formation of classical Be *circumstellar disks. I. New candidate Be stars in the LMC, SMC, and Milky Way. * Wisniewski J.P., Bjorkman K.S. * <Astrophys. J., 652, 458-471 (2006)> * =2006ApJ...652..458W C============================================================================= C Internal variables integer*4 i__ c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table4.dat' ! Photometric properties of the candidate Be stars integer*4 nr__ parameter (nr__=530) ! Number of records character*75 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*9 Cluster (nr__) ! Cluster name integer*4 Star (nr__) ! Star number within the cluster (1) integer*4 RAh (nr__) ! (h) Hour of Right Ascension (J2000) integer*4 RAm (nr__) ! (min) Minute of Right Ascension (J2000) real*4 RAs (nr__) ! (s) Second of Right Ascension (J2000) character*1 DE_ (nr__) ! Sign of the Declination (J2000) integer*4 DEd (nr__) ! (deg) Degree of Declination (J2000) integer*4 DEm (nr__) ! (arcmin) Arcminute of Declination (J2000) real*4 DEs (nr__) ! (arcsec) Arcsecond of Declination (J2000) real*4 Vmag (nr__) ! (mag) The V band magnitude real*4 e_Vmag (nr__) ! (mag) The error in Vmag real*4 B_V (nr__) ! (mag) The (B-V) color index real*4 e_B_V (nr__) ! (mag) The error in B-V real*4 R_Ha (nr__) ! (mag) The (R-H{alpha}) color index real*4 e_R_Ha (nr__) ! (mag) The error in R-Ha character*1 St (nr__) ! [CP] Be star status, as Candidate or Possible *Note (1): Stars identified as WBBe Cluster Star, e.g. * "WBBe Bruck 60 2" for "Bruck 60 WBBe 2". C============================================================================= C Loading file 'table4.dat' ! Photometric properties of the candidate Be stars C Format for file interpretation 1 format( + A9,6X,I3,1X,I1,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,F4.1,1X,F5.2, + 1X,F4.2,1X,F5.2,1X,F4.2,1X,F5.2,1X,F4.2,1X,A1) C Effective file loading open(unit=1,status='old',file= +'table4.dat') write(6,*) '....Loading file: table4.dat' do i__=1,530 read(1,'(A75)')ar__ read(ar__,1) + Cluster(i__),Star(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__), + DEd(i__),DEm(i__),DEs(i__),Vmag(i__),e_Vmag(i__),B_V(i__), + e_B_V(i__),R_Ha(i__),e_R_Ha(i__),St(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) + Cluster(i__),Star(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__), + DEd(i__),DEm(i__),DEs(i__),Vmag(i__),e_Vmag(i__),B_V(i__), + e_B_V(i__),R_Ha(i__),e_R_Ha(i__),St(i__) write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= stop end