Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJS/194/29 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-28 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/194/29 Observations of blazars at 15GHz (Richards+, 2011) *================================================================================ *Blazars in the Fermi era: the OVRO 40m telescope monitoring program. * Richards J.L., Max-Moerbeck W., Pavlidou V., King O.G., Pearson T.J., * Readhead A.C.S., Reeves R., Shepherd M.C., Stevenson M.A., Weintraub L.C., * Fuhrmann L., Angelakis E., Anton Zensus J., Healey S.E., Romani R.W., * Shaw M.S., Grainge K., Birkinshaw M., Lancaster K., Worrall D.M., * Taylor G.B., Cotter G., Bustos R. * <Astrophys. J. Suppl. Ser., 194, 29 (2011)> * =2011ApJS..194...29R C============================================================================= C Internal variables integer*4 i__ c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table4.dat' ! Program source data integer*4 nr__ parameter (nr__=1163) ! Number of records character*85 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*10 Name (nr__) ! Source name (<CGRaBS JHHMM+DDMM> in Simbad for * the 1158 Candidate Gamma-ray Blazar Survey sample) 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 (1) character*6 OType (nr__) ! Optical classification (AGN, BLL, GALAXY, FSRQ * (flat-spectrum radio quasar) or NLRG (narrow-line * radio galaxy)) integer*4 Nobs (nr__) ! Number of observations (2) character*1 v1LAC (nr__) ! [Y/N] Source associated with gamma-ray source in * Fermi 1LAC catalog Abdo et al. 2010, * Cat. J/ApJ/715/429 integer*4 Var (nr__) ! [0,5] Variability analysis flag, 0=variable (3) character*1 V2 (nr__) ! [C/V] Result of 3-{sigma} {chi}^2^ variability * test (4) real*4 S0 (nr__) ! (Jy) ? Intrinsic source mean flux density at 15GHz real*4 e_S0 (nr__) ! (Jy) ? The 1-{sigma} uncertainty in S0 character*1 l_m (nr__) ! Limit flag on m (5) real*4 m (nr__) ! (%) ? Intrinsic modulation index real*4 E_m (nr__) ! (%) ? Upper limit uncertainty in m real*4 e_m_1 (nr__) ! (%) ? Lower limit uncertainty in m *Note (1): For the CGRaBS sample, redshift and optical classifications are * repeated here from Healey et al. (2008, Cat. J/ApJS/175/97) for * convenience. *Note (2): That survived data editing and were used in our variability analysis. *Note (3): Flag as follows: * 0 = a non-zero intrinsic modulation is found; * 1 = the source is non-variable; * 2 = insufficient observations for variability analysis; * 3 = flux density too faint for variability analysis; * 4 = the source was a calibrator used in the spline fit to remove long-term * trends; * 5 = the source was a calibrator not used in the spline fit. *Note (4): C (V) indicates the source is (is not) consistent with a constant * flux density. *Note (5): Values for non-variable sources indicate 3-{sigma} upper limits and * no uncertainties are quoted for S0 and m. c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table5.dat' ! 15 GHz flux densities integer*4 nr__1 parameter (nr__1=149085) ! Number of records character*36 ar__1 ! Full-size record character*10 Name_1 (nr__1) ! Source name (<CGRaBS JHHMM+DDMM> in Simbad for * the 1158 Candidate Gamma-ray Blazar Survey sample) real*8 MJD (nr__1) ! (d) Modified Julian Date of the observation real*4 S15GHz (nr__1) ! (Jy) The 15GHz flux density real*4 e_S15GHz (nr__1) ! (Jy) Uncertainty in S15GHz C============================================================================= C Loading file 'table4.dat' ! Program source data C Format for file interpretation 1 format( + A10,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,F5.3,1X,A6, + 1X,I3,1X,A1,1X,I1,1X,A1,1X,F6.3,1X,F5.3,1X,A1,F5.1,1X,F3.1,1X, + F3.1) C Effective file loading open(unit=1,status='old',file= +'table4.dat') write(6,*) '....Loading file: table4.dat' do i__=1,1163 read(1,'(A85)')ar__ read(ar__,1) + Name(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__), + DEm(i__),DEs(i__),z(i__),OType(i__),Nobs(i__),v1LAC(i__), + Var(i__),V2(i__),S0(i__),e_S0(i__),l_m(i__),m(i__),E_m(i__), + e_m_1(i__) if(ar__(36:40) .EQ. '') z(i__) = rNULL__ if(ar__(59:64) .EQ. '') S0(i__) = rNULL__ if(ar__(66:70) .EQ. '') e_S0(i__) = rNULL__ if(ar__(73:77) .EQ. '') m(i__) = rNULL__ if(ar__(79:81) .EQ. '') E_m(i__) = rNULL__ if(ar__(83:85) .EQ. '') e_m_1(i__) = rNULL__ 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) + Name(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__), + DEm(i__),DEs(i__),z(i__),OType(i__),Nobs(i__),v1LAC(i__), + Var(i__),V2(i__),S0(i__),e_S0(i__),l_m(i__),m(i__),E_m(i__), + e_m_1(i__) write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= C Loading file 'table5.dat' ! 15 GHz flux densities C Format for file interpretation 2 format(A10,1X,F12.6,1X,F6.3,1X,F5.3) C Effective file loading open(unit=1,status='old',file= +'table5.dat') write(6,*) '....Loading file: table5.dat' do i__=1,149085 read(1,'(A36)')ar__1 read(ar__1,2)Name_1(i__),MJD(i__),S15GHz(i__),e_S15GHz(i__) c ..............Just test output........... write(6,2)Name_1(i__),MJD(i__),S15GHz(i__),e_S15GHz(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= stop end