Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJS/176/355 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-Mar-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/ApJS/176/355 AGN X-Ray emission and black holes (Kelly+, 2008) *================================================================================ *Observational constraints on the dependence of radio-quiet quasar X-ray emission *on black hole mass and accretion rate. * Kelly B.C., Bechtold J., Trump J.R., Vestergaard M., Siemiginowska A. * <Astrophys. J. Suppl. Ser., 176, 355-373 (2008)> * =2008ApJS..176..355K C============================================================================= C Internal variables integer*4 i__ c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table1.dat' ! Black Hole Parameters of the Sample integer*4 nr__ parameter (nr__=318) ! Number of records character*61 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) 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 z (nr__) ! Redshift real*4 logMBL (nr__) ! ([solMass]) Log of broad line mass estimate real*4 e_logMBL (nr__) ! ([solMass]) Uncertainty in logMBL real*4 logLX (nr__) ! ([-]) Log of 2keV to Eddington * luminosity ratio (1) real*4 e_logLX (nr__) ! ([-]) Uncertainty in logLX real*4 logLUV (nr__) ! ([-]) Log of 2500{AA} to Eddington * luminosity ratio (1) real*4 e_logLUV (nr__) ! ([-]) Uncertainty in LogLUV *Note (1): Where L_Eddington_ is calculated from the broad emission line * estimate of M_Blackhole_, M_BL_. C============================================================================= C Loading file 'table1.dat' ! Black Hole Parameters of the Sample C Format for file interpretation 1 format( + I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,F4.1,1X,F5.3,1X,F5.2,1X, + F4.2,1X,F5.2,1X,F4.2,1X,F5.2,1X,F4.2) C Effective file loading open(unit=1,status='old',file= +'table1.dat') write(6,*) '....Loading file: table1.dat' do i__=1,318 read(1,'(A61)')ar__ read(ar__,1) + RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),DEm(i__), + DEs(i__),z(i__),logMBL(i__),e_logMBL(i__),logLX(i__), + e_logLX(i__),logLUV(i__),e_logLUV(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) + RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),DEm(i__), + DEs(i__),z(i__),logMBL(i__),e_logMBL(i__),logLX(i__), + e_logLX(i__),logLUV(i__),e_logLUV(i__) write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= stop end