Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_A/506/1071 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-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/A+A/506/1071 Galaxy morphology in 5 medium redshift clusters (Ascaso+, 2009) *================================================================================ *The bright galaxy population of five medium redshift clusters. *II. Quantitative galaxy morphology. * Ascaso B., Aguerri J.A.L., Moles M., Sanchez-Janssen R., Bettoni D. * <Astron. Astrophys., 506, 1071-1082 (2009)> * =2009A&A...506.1071A C============================================================================= C Internal variables integer*4 i__ c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'tablea1.dat' ! Results of the 2-dimensional surface brightness fit for the galaxies in the NOT sample integer*4 nr__ parameter (nr__=68) ! Number of records character*132 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*5 Cluster ! Cluster name (ANNNN) (1) integer*4 RAh ! (h) Galaxy right ascension (J2000) (2) integer*4 RAm ! (min) Galaxy right ascension (J2000) (2) real*4 RAs ! (s) Galaxy right ascension (J2000) (2) character*1 DE_ ! Galaxy declination sign (J2000) (2) integer*4 DEd ! (deg) Galaxy declination (J2000) (2) integer*4 DEm ! (arcmin) Galaxy declination (J2000) (2) real*4 DEs ! (arcsec) Galaxy declination (J2000) (2) real*4 z ! ? Redshift, when available real*4 B_r ! (mag) Bessel-Gunn B-r' colour index real*4 rMAG ! (mag) Absolute Gunn r' magnitude real*4 mue ! (mag/arcsec2) Effective surface brightness of the bulge real*8 re ! (arcsec) Effective radius of the bulge real*4 eb ! Ellipticity of the bulge real*4 mu0 ! (mag/arcsec2) ?=0 Central surface brightness of the disk real*8 h ! (arcsec) ?=0 Scale length of the disk real*4 ed ! ?=0 Ellipticity of the disk real*4 n ! Shape parameter of the bulge real*8 PAb ! (deg) Position angle of the bulge real*8 PAd ! (deg) Position angle of the disk real*4 B_T ! ?=0 Bulge-to-total luminosity ratio real*4 chi2 ! {chi}^2^ of the fit character*1 col ! [BR] Assigned color (3) character*2 MType ! Visual morphological type extracted from * Paper I (Ascaso et al., Cat. J/A+A/487/453) *Note (1): The five clusters are A1643, A1878, A1952, A2111 and A2658. *Note (2): Galaxies identified in Simbad as * <[AMA2008] ANNNN JHHMMSS.ss+DDMMSS.ss> *Note (3): Red (R) galaxies are located within 0.2mag from the CMR of the * host cluster and Blue (B) galaxies are bluer than 0.2mag the CMR of * the cluster. C============================================================================= C Loading file 'tablea1.dat' ! Results of the 2-dimensional surface brightness * fit for the galaxies in the NOT sample C Format for file interpretation 1 format( + A5,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,2X,F6.4,1X,F5.3, + 1X,F6.2,1X,F5.2,1X,F8.6,1X,F5.3,1X,F5.2,1X,F8.6,1X,F5.3,1X, + F5.3,1X,F7.3,1X,F7.3,1X,F5.3,1X,F6.3,1X,A1,1X,A2) C Effective file loading open(unit=1,status='old',file= +'tablea1.dat') write(6,*) '....Loading file: tablea1.dat' do i__=1,68 read(1,'(A132)')ar__ read(ar__,1) + Cluster,RAh,RAm,RAs,DE_,DEd,DEm,DEs,z,B_r,rMAG,mue,re,eb,mu0, + h,ed,n,PAb,PAd,B_T,chi2,col,MType if(ar__(32:37) .EQ. '') z = rNULL__ 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) + Cluster,RAh,RAm,RAs,DE_,DEd,DEm,DEs,z,B_r,rMAG,mue,re,eb,mu0, + h,ed,n,PAb,PAd,B_T,chi2,col,MType write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg c .......End.of.Just test output........... end do close(1) C============================================================================= stop end