Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_A/507/85 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-Apr-18
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/507/85 ESO/VLT 3rd year type Ia supernova data set (Balland+, 2009)
*================================================================================
*The ESO/VLT 3rd year type Ia supernova data set from the supernova legacy
*survey.
* Balland C., Baumont S., Basa S., Mouchet M., Howell D.A., Astier P.,
* Carlberg R.G., Conley A., Fouchez D., Guy J., Hardin D., Hook I.M.,
* Pain R., Perrett K., Pritchet C.J., Regnault N., Rich J., Sullivan M.,
* Antilogus P., Arsenijevic V., Le Du J., Fabbro S., Lidman C., Mourao A.,
* Palanque-Delabrouille N., Pecontal E., Ruhlmann-Kleider V.
* <Astron. Astrophys., 507, 85-103 (2009)>
* =2009A&A...507...85B
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! *List of SNLS 3rd year ESO-VLT SN Ia and SN Ia*
spectra
integer*4 nr__
parameter (nr__=139) ! Number of records
character*73 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*6 SN (nr__) ! SN name (NNANaa)
character*3 n_SN (nr__) ! Individual notes (1)
integer*4 RAh (nr__) ! (h) Right ascension (J2000)
integer*4 RAm (nr__) ! (min) Right ascension (J2000)
real*4 RAs (nr__) ! (s) Right ascension (J2000)
character*1 DE_ (nr__) ! Declination sign (J2000)
integer*4 DEd (nr__) ! (deg) Declination (J2000)
integer*4 DEm (nr__) ! (arcmin) Declination (J2000)
real*4 DEs (nr__) ! (arcsec) Declination (J2000)
character*10 Date (nr__) ! ("YYYY-MM-DD") Spectrum date
character*5 ExpTime (nr__) ! (s) Exposure time
real*4 Seeing (nr__) ! (arcsec) Seeing
real*4 Dsep (nr__) ! (arcsec) ?=- Host-supernova distance (from PHASE
* model) (2)
real*4 Air (nr__) ! Air mass
real*4 i_mag (nr__) ! (mag) SDSS i' magnitude
*Note (1): Notes as follows:
* c = Observed with Grism 300I
* d = SNLS-03D4cy is identified as a SN Ia on the basis of a Gemini
* spectrum published in Howell et al. (2005ApJ...634.1190H).
* The VLT spectrum is shown here for reference
* e = There are two underlying galaxies in the line-of-sight of SNLS-04D1hx
* f = FORS2 spectrum
*Note (2): "---" either denotes cases for which a separate extraction of the
* supernova and the host component was not possible with PHASE or the
* absence of a detectable host.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Results of identifications of the SNLS 3rd year
ESO-VLT SN Ia and SN Ia* spectra
integer*4 nr__1
parameter (nr__1=142) ! Number of records
character*51 ar__1 ! Full-size record
character*6 SN_1 (nr__1) ! SN name (NNANaa)
character*5 SpType (nr__1) ! MK spectral type
real*4 z (nr__1) ! Redshift (of SN or host)
real*4 e_z (nr__1) ! rms uncertainty on z
character*1 n_z (nr__1) ! [HS] Redshift source (H for Host, S for SN)
real*4 Phase (nr__1) ! (d) Phase (time from maximum brightness)
character*8 Mod (nr__1) ! Host model (1)
real*4 Fract (nr__1) ! ? Fraction of host used in best fitting model
real*4 v_S_N_ (nr__1) ! Average signal-to-noise ratio per 5{AA} pixel
*Note (1): Host type of the best fitting model. The number in parenthesis is
* the age of the best fitting PEGASE template (in Gyrs). Two host types
* separated by a dash indicate that the best fitting host model is an
* interpolation between two Kinney et al. (1996ApJ...467...38K)
* templates. The label "NoGalaxy" denotes that the best fitting model
* is obtained with no host model.
C=============================================================================
C Loading file 'table1.dat' ! *List of SNLS 3rd year ESO-VLT SN Ia and SN Ia*
* spectra
C Format for file interpretation
1 format(
+ A6,1X,A3,2X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F5.2,1X,A10,1X,
+ A5,1X,F4.2,1X,F4.2,1X,F4.2,1X,F4.1)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,139
read(1,'(A73)')ar__
read(ar__,1)
+ SN(i__),n_SN(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
+ DEd(i__),DEm(i__),DEs(i__),Date(i__),ExpTime(i__),Seeing(i__),
+ Dsep(i__),Air(i__),i_mag(i__)
if (idig(ar__(60:63)).EQ.0) Dsep(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)
+ SN(i__),n_SN(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
+ DEd(i__),DEm(i__),DEs(i__),Date(i__),ExpTime(i__),Seeing(i__),
+ Dsep(i__),Air(i__),i_mag(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 'table2.dat' ! Results of identifications of the SNLS 3rd year
* ESO-VLT SN Ia and SN Ia* spectra
C Format for file interpretation
2 format(
+ A6,1X,A5,1X,F5.3,1X,F5.3,1X,A1,1X,F4.1,1X,A8,1X,F4.2,1X,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,142
read(1,'(A51)')ar__1
read(ar__1,2)
+ SN_1(i__),SpType(i__),z(i__),e_z(i__),n_z(i__),Phase(i__),
+ Mod(i__),Fract(i__),v_S_N_(i__)
if(ar__1(42:45) .EQ. '') Fract(i__) = rNULL__
c ..............Just test output...........
write(6,2)
+ SN_1(i__),SpType(i__),z(i__),e_z(i__),n_z(i__),Phase(i__),
+ Mod(i__),Fract(i__),v_S_N_(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