Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/669/327 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-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/669/327 S3MC: YSOs in N66, in SMC (Simon+, 2007)
*================================================================================
*The Spitzer survey of the Small Magellanic Cloud: discovery of embedded
*protostars in the HII region NGC 346.
* Simon J.D., Bolatto A.D., Whitney B.A., Robitaille T.P., Shah R.Y.,
* Makovoz D., Stanimirovic S., Barba R.H., Rubio M.
* <Astrophys. J., 669, 327-336 (2007)>
* =2007ApJ...669..327S
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Young Stellar Objects in N66
integer*4 nr__
parameter (nr__=111) ! Number of records
character*94 ar__ ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg ! (deg) Right Ascension J2000
real*8 DEdeg ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
character*1 YSO ! [DP] (D)efinite or (P)robable YSOs
integer*4 v_SBW2007b_ ! Sequential number
character*15 SSTS3MC ! SSTS3MC designation (DD.dddd+DD.dddd)
integer*4 RAh ! (h) Right ascension (J2000)
integer*4 RAm ! (min) Right ascension (J2000)
real*4 RAs ! (s) Right ascension (J2000)
character*1 DE_ ! Declination sign (J2000)
integer*4 DEd ! (deg) Declination (J2000)
integer*4 DEm ! (arcmin) Declination (J2000)
real*4 DEs ! (arcsec) Declination (J2000)
integer*4 Lum ! (solLum) Stellar luminosity
integer*4 e_Lum ! (solLum) ?=- rms uncertainty on Lum (1)
real*4 Mass ! (solMass) Stellar mass
real*4 e_Mass ! (solMass) ?=- rms uncertainty on Mass (1)
character*3 Stage ! Stage of YSO (I, II or III)
real*4 e_Stage ! ?=- rms uncertainty on Stage (1)
real*4 chi2 ! {chi}^2^ value (2)
real*4 chi22 ! ?=- {chi}_2_^2^ value (3)
*Note (1): The uncertainties on the luminosities, masses, and stages are
* calculated as the weighted standard deviation of the luminosities,
* masses, and stages of all of the acceptable YSO models. In cases where
* there is only one acceptable model for a given source, or there are
* multiple models but they all produce the same luminosity/mass/stage,
* we cannot calculate an uncertainty in this way, so we fill the
* corresponding space with an ellipsis.
*Note (2): The {chi}^2^ value for the best-fitting SED. Note that these are
* raw {chi}^2^ values, not {chi}^2^ per data point, so a good fit
* ({chi}^2^ per data point <=2.2) can have a {chi}^2^ value as high as 8.8
* (if there are four flux data points for that source) or more.
*Note (3): The {chi}^2^ value for the best-fitting AGB star or background
* galaxy SED.
C=============================================================================
C Loading file 'table1.dat' ! Young Stellar Objects in N66
C Format for file interpretation
1 format(
+ A1,1X,I3,9X,A15,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,
+ I5,1X,I5,1X,F4.1,1X,F3.1,1X,A3,1X,F3.1,1X,F5.2,1X,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,111
read(1,'(A94)')ar__
read(ar__,1)
+ YSO,v_SBW2007b_,SSTS3MC,RAh,RAm,RAs,DE_,DEd,DEm,DEs,Lum,e_Lum,
+ Mass,e_Mass,Stage,e_Stage,chi2,chi22
if (e_Lum .EQ. 45) e_Lum = iNULL__
if (idig(ar__(72:74)).EQ.0) e_Mass = rNULL__
if (idig(ar__(80:82)).EQ.0) e_Stage = rNULL__
if (idig(ar__(90:94)).EQ.0) chi22 = rNULL__
RAdeg = rNULL__
DEdeg = rNULL__
c Derive coordinates RAdeg and DEdeg from input data
c (RAdeg and DEdeg are set to rNULL__ when unknown)
if(RAh .GT. -180) RAdeg=RAh*15.
if(RAm .GT. -180) RAdeg=RAdeg+RAm/4.
if(RAs .GT. -180) RAdeg=RAdeg+RAs/240.
if(DEd .GE. 0) DEdeg=DEd
if(DEm .GE. 0) DEdeg=DEdeg+DEm/60.
if(DEs .GE. 0) DEdeg=DEdeg+DEs/3600.
if(DE_.EQ.'-'.AND.DEdeg.GE.0) DEdeg=-DEdeg
c ..............Just test output...........
write(6,1)
+ YSO,v_SBW2007b_,SSTS3MC,RAh,RAm,RAs,DE_,DEd,DEm,DEs,Lum,e_Lum,
+ Mass,e_Mass,Stage,e_Stage,chi2,chi22
write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
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