Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/686/127 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-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/ApJ/686/127 Starbursts luminosities based on PAH (Weedman+, 2008)
*================================================================================
*The most luminous starbursts in the Universe.
* Weedman D.W., Houck J.R.
* <Astrophys. J., 686, 127-137 (2008)>
* =2008ApJ...686..127W
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! PAH luminosities for starburst galaxies
integer*4 nr__
parameter (nr__=243) ! Number of records
character*63 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 Seq (nr__) ! Source running number
character*16 Name (nr__) ! Source identification (1)
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__) ! Declination sign (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__) ! Spectroscopic redshift (from Spitzer IRS)
real*8 Fnu (nr__) ! (mJy) ? Spitzer/IRS flux density at 7.7um (2)
real*4 logLnu (nr__) ! ([10-7W]) Rest-frame luminosity {nu}L_{nu}_ at 7.7um (3)
integer*4 Ref (nr__) ! Reference (4)
*Note (1): SST24 objects are named <[WH2008] SST24 JHHMMSS.ss+DDMMSS.s> in Simbad
*Note (2): Observed flux density in mJy at peak of 7.7um PAH feature
* measured from published spectra or from our own extractions. Typical
* uncertainties are +/-5% for sources with F_{nu}_(7.7{mu}m)>~5mJy and
* +/-10% for sources with F_{nu}_(7.7{mu}m)~1mJy. Sources without
* entries have {nu}L_{nu}_(7.7um) determined from other PAH features, as
* explained in note (2).
*Note (3): Rest-frame luminosity {nu}L_{nu}_(7.7um) in ergs/s determined
* using peak F_{nu}_(7.7um) and luminosity distances from E. L. Wright,
* http://www.astro.ucla.edu/~wright/CosmoCalc.html, for H_0_=71km/s/Mpc,
* {Omega}_M_=0.27, and {Omega}_{Lambda}_=0.73.
* * For ULIRGs in reference 12, {nu}L_{nu}_(7.7um) is determined
* using the relation {nu}L_{nu}_(7.7{mu}m)=28L(6.2{mu}m+11.3{mu}m);
* * for ULIRGs in references 13 and 14, {nu}L_{nu}_(7.7um) is determined
* using the relation {nu}L_{nu}_(7.7{mu}m)=50L(6.2{mu}m).
* * For starbursts in reference 1, luminosities also include the
* correction factor FF given in Brandl et al. (2006ApJ...653.1129B)
* for flux from the resolved source which is not included in the IRS
* observing slit.
*Note (4): References (with more details in section 2.1) as follows:
* 1 = Brandl et al. 2006ApJ...653.1129B
* 2 = Houck et al. 2007, Cat. J/ApJ/671/323;
* <[HWL2007] SST24 JHHMMSS.ss+DDMMSS.s> in Simbad
* 3 = new extraction of Bootes source from archival spectra program 20128 (PI:
* G. Lagache) or 20113 (PI: H. Dole)
* 4 = new spectral extraction from program 40038 (D. Weedman & J. Houck,
* 2009, cat J/ApJ/693/370)
* 5 = new extraction of FLS source from archival spectra program 20128
* 6 = Brand et al. 2008ApJ...673..119B;
* <[BWD2008] SST24 JHHMMSS.s+DDMMSS> in Simbad.
* 7 = Weedman et al. 2006ApJ...653..101W
* 8 = Farrah et al. 2008ApJ...677..957F; <SWIRE JHHMMSS.ss+DDMMSS.s> in Simbad
* 9 = new extraction of source in Houck et al. (2005ApJ...622L.105H,
* <[HSW2005] SST24 JHHMMSS.ss+DDMMSS.s> in Simbad) or Weedman et al.
* (2006ApJ...638..613W, <[WLH2006] SST24 JHHMMSS.ss+DDMMSS.s>) using v15
* data products and the 4 pixel extraction technique described in Weedman
* et al. (2006ApJ...653..101W)
* 10 = Yan et al. 2007ApJ...658..778Y;
* <[YSF2007] SST24 JHHMMSS.ss+DDMMSS.s> in Simbad
* 11 = Pope et al. 2008ApJ...675.1171P
* 12 = Farrah et al. 2007ApJ...667..149F
* 13 = Imanishi et al. 2007ApJS..171...72I
* 14 = Sargsyan et al. 2008ApJ...683..114S
C=============================================================================
C Loading file 'table1.dat' ! PAH luminosities for starburst galaxies
C Format for file interpretation
1 format(
+ I3,1X,A16,1X,I2,I2,F5.2,A1,I2,I2,F4.1,1X,F6.4,1X,F7.2,1X,F5.2,
+ 1X,I2)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,243
read(1,'(A63)')ar__
read(ar__,1)
+ Seq(i__),Name(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
+ DEd(i__),DEm(i__),DEs(i__),z(i__),Fnu(i__),logLnu(i__),
+ Ref(i__)
if(ar__(48:54) .EQ. '') Fnu(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)
+ Seq(i__),Name(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
+ DEd(i__),DEm(i__),DEs(i__),z(i__),Fnu(i__),logLnu(i__),
+ Ref(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end