Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_A/515/A57 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-17 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/515/A57 Radial velocities in clusters of galaxies. V. (Proust+, 2010) *================================================================================ *New measurements of radial velocities in clusters of galaxies. V. * Proust D., Capelato H.V., Lima Neto G.B., Sodre L. Jr. * <Astron. Astrophys. 515, A57 (2010)> * =2010A&A...515A..57P C============================================================================= C Internal variables integer*4 i__ c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table1.dat' ! Heliocentric redshift, position, and morphological type for galaxies of A376, A970, A1356, and A2244 integer*4 nr__ parameter (nr__=79) ! Number of records character*68 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 integer*4 Gal ! Galaxy number within the cluster (1) integer*4 RAh ! (h) Right ascension (J2000) integer*4 RAm ! (min) Right ascension (J2000) real*4 RAs ! (s) Right ascension (J2000) character*1 DE_ ! Declination sign (J2000) integer*4 DEd ! (deg) Declination (J2000) integer*4 DEm ! (arcmin) Declination (J2000) integer*4 DEs ! (arcsec) Declination (J2000) character*4 MType ! Morphological type (2) integer*4 HRV ! (km/s) Heliocentric radial velocity integer*4 e_HRV ! (km/s) rms uncertainty on HRV real*4 R ! R-value derived from Tonry & Davis * (1979AJ.....84.1511T) integer*4 VNED ! (km/s) ? NED velocity integer*4 Note ! ? Note about emission lines (3) character*7 Rem ! Remarks *Note (1): For A376, this number refers to Dressler (1980, Cat. VII/174, * [D80] ACO NNNN NNN) and for A970 it continues the list of Sodre et al. * (2001, Cat. J/A+A/377/438, [SPC2001] NN) *Note (2): either from Dressler's (1980, Cat. VII/174) catalog for A376 and * from a visual inspection on the Palomar Sky Survey (POSS) for A970. *Note (3): Notes as follows: * 1 = emission line: H{alpha}=40498km/s * 2 = emission line: H{alpha}=39982km/s * 3 = emission line: H{alpha}=13072km/s * 4 = emission line: H{beta}, 2OIII, H{alpha}, S2 * 5 = emission line: H{alpha}=41167km/s * 6 = emission line: H{alpha}=14829km/s * 7 = emission line: OII, H{beta}, 2OIII, H{alpha}, S1 * 8 = emission line: H{alpha}, S2=15478km/s * 9 = emission line: H{alpha}=12066km/s * 10 = emission line: H{alpha}=13267km/s * 11 = emission line: H{alpha}=17652km/s * 12 = emission line: H{alpha}=11058km/s * 13 = emission line: H{alpha} * 14 = emission lines: 2OIII, H{alpha}, S1 * 15 = emission line: H{alpha} * 16 = emission lines: OII, OIII, H{alpha}, N2=21398+/-68km/s * 17 = emission lines: 2OIII, H{alpha}=10684+/-35km/s * 18 = emission lines: H{alpha}, N2 * 19 = emission line: H{alpha} * 20 = emission lines: H{beta}, 2OIII, H{alpha}, N1, N2, S1, S2 C============================================================================= C Loading file 'table1.dat' ! Heliocentric redshift, position, and morphological * type for galaxies of A376, A970, A1356, and A2244 C Format for file interpretation 1 format( + A5,I3,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,I2,1X,A4,2X,I5,1X, + I3,1X,F5.2,1X,I5,1X,I2,1X,A7) C Effective file loading open(unit=1,status='old',file= +'table1.dat') write(6,*) '....Loading file: table1.dat' do i__=1,79 read(1,'(A68)')ar__ read(ar__,1) + Cluster,Gal,RAh,RAm,RAs,DE_,DEd,DEm,DEs,MType,HRV,e_HRV,R, + VNED,Note,Rem if(ar__(53:57) .EQ. '') VNED = iNULL__ if(ar__(59:60) .EQ. '') Note = 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) + Cluster,Gal,RAh,RAm,RAs,DE_,DEd,DEm,DEs,MType,HRV,e_HRV,R, + VNED,Note,Rem write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg c .......End.of.Just test output........... end do close(1) C============================================================================= stop end