Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/671/323 into FORTRAN code for reading data files line by line.
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-20
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/671/323 Spitzer Spectra of a 10mJy galaxy sample (Houck+, 2007)
*================================================================================
*Spitzer spectra of a 10mJy galaxy sample and the star formation rate in the
*Local universe.
* Houck J.R., Weedman D.W., Le Floc'h E., Hao L.
* <Astrophys. J., 671, 323-332 (2007)>
* =2007ApJ...671..323H
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! The Bootes 10mJy sample
integer*4 nr__
parameter (nr__=50) ! Number of records
character*100 ar__ ! Full-size record
integer*4 v_HWL2007_ ! Sequential number
character*19 SST24 ! Source name (JHHMMSS.ss+DDMMSS.s), in Simbad
* [HWL2007] SST24 JHHMMSS.ss+DDMMSS.s (1)
integer*4 AOR ! ? AOR number (observation number in the
* Spitzer archive)
character*9 Prog ! Program number(s)
integer*4 expSL ! (s) ? Total integration time in IRS Short-Low
* orders 1 and 2
integer*4 expLL ! (s) ? Total integration time in IRS Long-Low
* orders 1 and 2
real*4 F24um ! (mJy) Flux at 24um (2)
character*1 n_F24um ! [r] Note on F24um (3)
real*4 F24um2 ! (mJy) ? Flux at 24um measured independently from
* the extracted IRS spectra (2)
character*1 f_F24um ! [g] Note on F24um (3)
character*1 l_F70um ! Limit flag on 70um
integer*4 F70um ! (mJy) ? Flux at 70um (4)
character*1 u_F70um ! [?] Uncertainty flag on F70um
character*1 n_F70um ! [r] Note on F70um (2)
character*22 Class ! Classification of IRS spectrum (5)
character*1 n_Class ! [*] Note on Class, in notes.dat file
*Note (1): SST24 source name derives from discovery with the MIPS 24um
* images; coordinates listed are J2000.0 24um positions with typical
* 3{sigma} uncertainty of +/-1.2".
*Note (2): Values of f{nu}(24um) are for an unresolved point source measured
* from MIPS images, except that source noted by (r). The mean difference
* of +/-4% between IRS and MIPS values gives an estimate of uncertainties
* in results
*Note (3): Notes as follows:
* g = Spiral galaxy and liner NGC 5656, with SDSS z=0.01055
* r = sources resolved in the same galaxy in the 24um or 70um image,
* and the flux listed is the total flux for all components.
*Note (4): Values of f{nu}(70um) are for an unresolved point source,
* measured from MIPS images; fluxes are uncertain for sources 13 and 14
* because these are two closely interacting galaxies. Sources without
* measured f{nu}(70um) are outside of the field of view for the 70um survey.
*Note (5): Classification of IRS spectrum, whether showing PAH emission,
* emission lines, absorption by the 9.7um Si feature, emission by the
* 9.7um silicate feature, or no features; numerical value gives
* classification according to scheme of Spoon et al. (2007ApJ...654L..49S)
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'notes.dat' ! Individual notes
integer*4 nr__1
parameter (nr__1=17) ! Number of records
character*56 ar__1 ! Full-size record
integer*4 v_HWL2007__1 ! Source number
character*53 Note ! Note
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! Redshifts, luminosities, and star formation
rates of PAH sources
integer*4 nr__2
parameter (nr__2=25) ! Number of records
character*103 ar__2 ! Full-size record
integer*4 v_HWL2007__2 ! Sequential number
character*9 Source ! Source name (HHMM+DDMM) (1)
real*4 z ! IRS redshift (3)
real*4 z2 ! ?=- SDSS redshift (2)
character*15 Class_1 ! SDSS class
integer*4 DL ! (Mpc) Luminosity distance
real*4 EW6_2um ! (um) Equivalent width at 6.2um (4)
real*4 e_EW6_2um ! (um) rms uncertainty on EW6.2um
real*4 F7_7um ! (mJy) Flux density at peak of 7.7um feature
real*4 F7_7um2 ! (mJy) Flux density at peak of 7.7um feature
* after subtraction of underlying
* continuum at 7.7um
real*4 log_nuLnu ! ([10-7W]) Luminosity at 7.7um in source
* rest frame (5)
real*4 log_LIR ! ([solLum]) Infrared luminosity
real*4 SFR ! (Msun/yr) Stellar formation rate (6)
real*4 SFR2 ! (Msun/yr) ? Second value of stellar formation
* rate (7)
real*8 Dens ! (10-5Mpc-3) Space density (8)
real*4 SFRdens ! (10-5Msun/yr/Mpc3) Stellar formation rate density (9)
*Note (1): Source name is truncated name from Table 1.
*Note (2): SDSS redshifts are from optical spectra.
*Note (3): IRS redshifts are determined from PAH emission features, assuming
* rest wavelengths of 6.2, 7.7, 8.6, and 11.3um; mean difference between
* SDSS and IRS redshifts of 0.0012 is estimate of uncertainty in IRS
* redshift.
*Note (4): Equivalent widths listed (EW) are in the observed frame;
* equivalent widths in the rest frame are EW/(1+z).
*Note (5): determined from peak flux density of 7.7um feature without
* continuum subtraction.
*Note (6): SFR for this source as determined from relation
* log(SFR)=log[nuLnu(7.7um)]-42.57.
*Note (7): SFR that would be derived using the f(H{alpha}) for KISS sources
* and the relation log(SFR)=log[L(H{alpha})]-41.1, with no correction for
* extinction.
*Note (8): Space density for this source determined from inverse of comoving
* volume Vmax which source could occupy and remain within sample
* f{nu}(24um)>10mJy; luminosity distances and comoving volumes
* determined by E.L. Wright, for H_0_=71km/s/Mpc, {Omega}_M_=0.27, and
* {Omega}_{Lambda}_=0.73 (http://www.astro.ucla.edu/~wright/CosmoCalc.html)
*Note (9): SFR density produced by this source as determined from
* {nu}L_{nu}_(7.7um).
C=============================================================================
C Loading file 'table1.dat' ! The Bootes 10mJy sample
C Format for file interpretation
1 format(
+ I2,7X,A19,1X,I8,1X,A9,1X,I3,1X,I3,1X,F5.1,A1,1X,F4.1,A1,A1,I4,
+ A1,A1,1X,A22,1X,A1)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,50
read(1,'(A100)')ar__
read(ar__,1)
+ v_HWL2007_,SST24,AOR,Prog,expSL,expLL,F24um,n_F24um,F24um2,
+ f_F24um,l_F70um,F70um,u_F70um,n_F70um,Class,n_Class
if(ar__(30:37) .EQ. '') AOR = iNULL__
if(ar__(49:51) .EQ. '') expSL = iNULL__
if(ar__(53:55) .EQ. '') expLL = iNULL__
if(ar__(64:67) .EQ. '') F24um2 = rNULL__
if(ar__(70:73) .EQ. '') F70um = iNULL__
c ..............Just test output...........
write(6,1)
+ v_HWL2007_,SST24,AOR,Prog,expSL,expLL,F24um,n_F24um,F24um2,
+ f_F24um,l_F70um,F70um,u_F70um,n_F70um,Class,n_Class
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'notes.dat' ! Individual notes
C Format for file interpretation
2 format(I2,1X,A53)
C Effective file loading
open(unit=1,status='old',file=
+'notes.dat')
write(6,*) '....Loading file: notes.dat'
do i__=1,17
read(1,'(A56)')ar__1
read(ar__1,2)v_HWL2007__1,Note
c ..............Just test output...........
write(6,2)v_HWL2007__1,Note
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table3.dat' ! Redshifts, luminosities, and star formation
* rates of PAH sources
C Format for file interpretation
3 format(
+ I2,1X,A9,1X,F6.4,1X,F6.4,1X,A15,I4,1X,F4.2,1X,F4.2,1X,F4.1,1X,
+ F4.1,1X,F5.2,1X,F5.2,1X,F6.2,1X,F4.2,1X,F7.4,1X,F4.1)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,25
read(1,'(A103)')ar__2
read(ar__2,3)
+ v_HWL2007__2,Source,z,z2,Class_1,DL,EW6_2um,e_EW6_2um,F7_7um,
+ F7_7um2,log_nuLnu,log_LIR,SFR,SFR2,Dens,SFRdens
if (idig(ar__2(21:26)).EQ.0) z2 = rNULL__
if(ar__2(87:90) .EQ. '') SFR2 = rNULL__
c ..............Just test output...........
write(6,3)
+ v_HWL2007__2,Source,z,z2,Class_1,DL,EW6_2um,e_EW6_2um,F7_7um,
+ F7_7um2,log_nuLnu,log_LIR,SFR,SFR2,Dens,SFRdens
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