Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_A/526/A28 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/A+A/526/A28 SDSS-II supernovae NTT and NOT spectroscopy (Oestman+, 2011) *================================================================================ *NTT and NOT spectroscopy of SDSS-II supernovae. * Oestman L., Nordin J., Goobar A., Amanullah R., Smith M., Sollerman J., * Stanishev V., Stritzinger M.D., Bassett B.A., Davis T.M., Edmondson E., * Frieman J.A., Garnavich P.M., Lampeitl H., Leloudas G., Marriner J., * Nichol R.C., Romer K., Sako M., Schneider D.P., Zheng C. * <Astron. Astrophys., 526, A28 (2011)> * =2011A&A...526A..28O C============================================================================= C Internal variables integer*4 i__ c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'tablea1.dat' ! Information about the observations integer*4 nr__ parameter (nr__=290) ! Number of records character*39 ar__ ! Full-size record integer*4 ID (nr__) ! [12778/22284] Source ID number, * <SDSS-II SNNNNNN> in Simbad integer*4 SPID (nr__) ! Spectrum SPID (1) character*6 SN (nr__) ! IAU name (YYYYaa) character*3 Tel (nr__) ! [NOT NTT] Telescope used real*4 Slit (nr__) ! (arcsec) Slit width integer*4 Texp (nr__) ! (s) Exposure time real*4 Air (nr__) ! Airmass real*4 See (nr__) ! (arcsec) Seeing (2) *Note (1): Most of the spectra in the table that lack IAU names are * photometric SNe without reliable spectroscopic confirmation and * unclassified objects. *Note (2): The FWHM seeing at 5000{AA} for the airmass at which the * observations were conducted. c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'tablea2.dat' ! Spectroscopic typing and redshift determination integer*4 nr__1 parameter (nr__1=290) ! Number of records character*107 ar__1 ! Full-size record integer*4 ID_1 (nr__1) ! [12778/22284] Source ID number integer*4 SPID_1 (nr__1) ! Spectrum SPID number character*13 Type1 (nr__1) ! SDSS SN type (3) character*14 Type2 (nr__1) ! NTT/NOT SN type (4) real*4 LC (nr__1) ! (d) ? Number of days in rest frame from B-band * maximum obtained from the lightcurve (5) real*4 e_LC (nr__1) ! (d) ? Error on LC character*1 n_LC (nr__1) ! [p] Note on LC (6) real*4 SNID (nr__1) ! (d) ? Number of days in rest frame from B-band * maximum obtained from SNID (7) real*4 e_SNID (nr__1) ! (d) ? Error on SNID real*8 ze (nr__1) ! ? SDSS redshift (8) real*8 e_ze (nr__1) ! ? Error on ze real*8 z (nr__1) ! ? SNID redshift real*8 e_z (nr__1) ! ? Error on z character*8 Notes (nr__1) ! Notes (9) *Note (3): The overall SDSS type which is based on the results from the NTT/NOT * analysis in combination with spectra from other telescopes. *Note (4): The typing of the individual spectra in this analysis is based on the * result from SNID in combination with a visual inspection. If a subtype could * be determined, this is given in the table, otherwise only the type. Thus, when * the type is given as solely Ia, this means that SNID could not determine if it * is a normal SN Ia or a non-normal (peculiar, SN 1991T or SN 1991bg). In the * cases where all template spectra which could be matched with the input * spectrum with SNID belong to the same SN, the name of the SN is written within * parenthesis. When the type is NotSN or Gal, this usually means that the * transient was too faint, or the observing conditions were not good enough, so * that the contribution from the host galaxy dominates the spectrum. *Note (5): An age is given when the object has been classified as a SN Ia, as * well as there were enough photometry to build a lightcurve. *Note (6): The sign "p" is added after the lightcurve age when the lightcurve * lacked photometry either before or after maximum brightness. *Note (7): If no error is given, there was only one template fitting the * requirements in SNID. *Note (8): The object redshifts from Zheng et al. (in preparation), which have * their origin in SDSS DR7 redshifts in combination with measurements of * both NTT/NOT spectra and other spectra. *Note (9): Additional information as follows: * s = when the SNID type was determined from the host-galaxy subtracted spectrum * f = if there were few template spectra matching the input spectrum, at which * fewer than 5 spectra were used to determine the type, the redshift * and/or the age * v = when the type obtained from SNID was changed after the visual inspection * zg = when the redshift is not obtained from SDSS DR7, and determined from * galaxy lines * zs = when the redshift is not obtained from SDSS DR7, and determined from * SN features * zt = if the redshift was determined through template fitting c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'tablea3.dat' ! *Spectral quality integer*4 nr__2 parameter (nr__2=290) ! Number of records character*19 ar__2 ! Full-size record integer*4 ID_2 (nr__2) ! [12778/22284] Source ID number integer*4 SPID_2 (nr__2) ! Spectrum ID number real*4 Host (nr__2) ! [0/1]?=- Host contamination (10) character*1 n_Host (nr__2) ! [e] e when estimation based on an * extrapolation of the photometry real*4 Sloss (nr__2) ! [0/1] Estimated maximum differential slit loss * due to atmospheric refraction affecting the SN * light in the wavelength region 4000-8000{AA} * (observed frame) *Note (10): The estimated host-galaxy contamination in the observed spectra, * i.e. before host-galaxy subtraction has been attempted, for * wavelengths corresponding to the g filter in observed frame. C============================================================================= C Loading file 'tablea1.dat' ! Information about the observations C Format for file interpretation 1 format(I5,1X,I4,1X,A6,1X,A3,1X,F3.1,1X,I4,1X,F4.2,1X,F3.1) C Effective file loading open(unit=1,status='old',file= +'tablea1.dat') write(6,*) '....Loading file: tablea1.dat' do i__=1,290 read(1,'(A39)')ar__ read(ar__,1) + ID(i__),SPID(i__),SN(i__),Tel(i__),Slit(i__),Texp(i__), + Air(i__),See(i__) c ..............Just test output........... write(6,1) + ID(i__),SPID(i__),SN(i__),Tel(i__),Slit(i__),Texp(i__), + Air(i__),See(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= C Loading file 'tablea2.dat' ! Spectroscopic typing and redshift determination C Format for file interpretation 2 format( + I5,1X,I4,1X,A13,1X,A14,1X,F6.2,1X,F4.2,A1,1X,F5.1,1X,F5.1,2X, + F7.5,1X,F7.5,2X,F7.5,1X,F7.5,1X,A8) C Effective file loading open(unit=1,status='old',file= +'tablea2.dat') write(6,*) '....Loading file: tablea2.dat' do i__=1,290 read(1,'(A107)')ar__1 read(ar__1,2) + ID_1(i__),SPID_1(i__),Type1(i__),Type2(i__),LC(i__),e_LC(i__), + n_LC(i__),SNID(i__),e_SNID(i__),ze(i__),e_ze(i__),z(i__), + e_z(i__),Notes(i__) if(ar__1(41:46) .EQ. '') LC(i__) = rNULL__ if(ar__1(48:51) .EQ. '') e_LC(i__) = rNULL__ if(ar__1(54:58) .EQ. '') SNID(i__) = rNULL__ if(ar__1(60:64) .EQ. '') e_SNID(i__) = rNULL__ if(ar__1(67:73) .EQ. '') ze(i__) = rNULL__ if(ar__1(75:81) .EQ. '') e_ze(i__) = rNULL__ if(ar__1(84:90) .EQ. '') z(i__) = rNULL__ if(ar__1(92:98) .EQ. '') e_z(i__) = rNULL__ c ..............Just test output........... write(6,2) + ID_1(i__),SPID_1(i__),Type1(i__),Type2(i__),LC(i__),e_LC(i__), + n_LC(i__),SNID(i__),e_SNID(i__),ze(i__),e_ze(i__),z(i__), + e_z(i__),Notes(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= C Loading file 'tablea3.dat' ! *Spectral quality C Format for file interpretation 3 format(I5,1X,I4,1X,F3.1,A1,1X,F3.1) C Effective file loading open(unit=1,status='old',file= +'tablea3.dat') write(6,*) '....Loading file: tablea3.dat' do i__=1,290 read(1,'(A19)')ar__2 read(ar__2,3) + ID_2(i__),SPID_2(i__),Host(i__),n_Host(i__),Sloss(i__) if (idig(ar__2(12:14)).EQ.0) Host(i__) = rNULL__ c ..............Just test output........... write(6,3) + ID_2(i__),SPID_2(i__),Host(i__),n_Host(i__),Sloss(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= stop end C Locate position of first digit in string; or return 0 integer function idig(c) character*(*) c character*1 c1 integer lc,i lc=len(c) idig=0 do i=1,lc if(c(i:i).ne.' ') go to 1 end do 1 if(i.gt.lc) return c1=c(i:i) if(c1.eq.'.'.or.c1.eq.'-'.or.c1.eq.'+') i=i+1 if(i.gt.lc) return c1=c(i:i) if(c1.ge.'0'.and.c1.le.'9') idig=i return end