Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_A/584/A92 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 2026-May-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/584/A92 Galactic Cold Cores. IV. Cold sub-mm sources (Montillaud+, 2015)
*================================================================================
*Galactic Cold Cores.
*IV. Cold sub-millimetre sources: catalogue and statistical analysis.
* Montillaud J., Juvela M., Rivera-Ingraham A., Malinen J., Pelkonen V.-M.,
* Ristorcelli I., Montier L., Marshall D.J., Marton G., Pagani L., Toth L.V.,
* Zahorecz S., Ysard N., McGehee P., Paladini R., Falgarone E.,
* Bernard J.-P., Motte F., Zavagno A., Doi Y.
* <Astron. Astrophys. 584, A92 (2015)>
* =2015A&A...584A..92M (SIMBAD/NED BibCode)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! General properties of Herschel fields
integer*4 nr__
parameter (nr__=116) ! Number of records
character*265 ar__ ! Full-size record
character*13 Field ! Field name
real*4 Dist ! (kpc) ?=- Adopted distance
real*4 E_Dist ! (kpc) ? Error on Dist (upper value)
real*4 e_Dist_1 ! (kpc) ? Error on Dist (lower value)
character*1 Flag ! [0/2] Reliability flag on Dist (1)
real*4 RG ! (kpc) ?=- Galactic radius (galactocentric distance)
integer*4 AltG ! (pc) ?=- Galactic altitude
real*4 T0_1 ! (K) 0.1th percentile dust temperature in the field
real*4 T90 ! (K) 90th percentile dust temperature in the field
real*4 Nh2 ! (cm-2) Median H_2_ column index in the field
real*4 Mass ! (Msun) ?=- Total mass in the field
real*4 C90 ! (Msun) ?=- Mass at 90% completeness
real*4 C50 ! (Msun) ?=- Mass at 90% completeness
character*176 Assoc ! Associated clouds and masers (2)
*Note (1): Reliability flag as follows:
* 0 = weak
* 1 = medium
* 2 = high level of confidence
*Note (2): the names of clouds from the LDN, MBM and TGU catalogues that lie
* within 1.5 degrees of the field, in order of increasing distance from the
* centre of the field. Known masers are also reported. We added horizontal lines
* to mark the 90, 180 and 270 values of galactic longitude.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'gccscat.dat' ! The GCC source catalogue
integer*4 nr__1
parameter (nr__1=4466) ! Number of records
character*571 ar__1 ! Full-size record
C J2000 position composed of: RAdeg DEdeg
integer*4 ID ! Source number in this catalogue
character*13 Field_1 ! Name of the Herschel field where sources
* were extracted (GLLL.l+BB.bb)
real*4 Dist_1 ! (kpc) Adopted distance
real*4 E_Dist_2 ! (kpc) Upper distance uncertainty
real*4 e_Dist_3 ! (kpc) Lower distance uncertainty
character*1 Dflag ! [0/2] Distance quality flag (1)
real*8 RAdeg ! (deg) Right ascension (J2000)
real*8 DEdeg ! (deg) Declination (J2000)
real*8 GLON ! (deg) Galactic longitude
real*8 GLAT ! (deg) Galactic latitude
real*4 SIGGLO ! Global significance of the source
* extraction (2)
character*1 FG ! [0/3] getsources quality flag (2)(3)
real*4 GOOD ! Goodness of the extraction (2)
real*4 SIGMONO1 ! Monochromatic significance of the source
* extraction at 160 microns (2)
integer*4 FM1 ! ? Monochromatic quality flag for the source
* extraction at 160um (2) (4)
real*4 FXPBEST1 ! (Jy/beam) ?=0 Peak flux value in the source at 160um
* (Jansky/beam) (2) (5)
real*4 e_FXPBEST1 ! (Jy/beam) ?=0 Uncertainty on the peak flux value in
* the source at 160um (Jansky/beam) (2) (5)
real*4 FXTBEST1 ! (Jy) ?=0 Total flux value in the source
* at 160um (2)
real*4 e_FXTBEST1 ! (Jy) ?=0 Uncertainty on the total flux value in
* the source at 160um (2)
real*4 AFWHM1 ! (arcsec) FWHM of the source major axis at 160um (2)
real*4 BFWHM1 ! (arcsec) FWHM of the source minor axis at 160um (2)
real*4 PA1 ! (deg) Position angle of the source major axis at
* 160um (2) (6)
real*4 SIGMONO2 ! Monochromatic significance of the source
* extraction at 250 microns (2)
character*1 FM2 ! [0/2] Monochromatic quality flag for the
* source extraction at 250um (2) (4)
real*4 FXPBEST2 ! (Jy/beam) ?=0 Peak flux value in the source at 250um
* (Jansky/beam) (2) (5)
real*4 e_FXPBEST2 ! (Jy/beam) ?=0 Uncertainty on the peak flux value in
* the source at 250um (Jansky/beam) (2) (5)
real*4 FXTBEST2 ! (Jy) ?=0 Total flux value in the source at
* 250um (2)
real*4 e_FXTBEST2 ! (Jy) ?=0 Uncertainty on the total flux value in
* the source at 250um (2)
real*4 AFWHM2 ! (arcsec) FWHM of the source major axis at 250um (2)
real*4 BFWHM2 ! (arcsec) FWHM of the source minor axis at 250um (2)
real*4 PA2 ! (deg) Position angle of the source major axis
* at 250um (2) (6)
real*4 SIGMONO3 ! Monochromatic significance of the source
* extraction at 350 microns (2)
character*1 FM3 ! [0/1] Monochromatic quality flag for the
* source extraction at 350um (2) (4)
real*4 FXPBEST3 ! (Jy/beam) ?=0 Peak flux value in the source at 350um
* (Jansky/beam) (2) (5)
real*4 e_FXPBEST3 ! (Jy/beam) ?=0 Uncertainty on the peak flux value in
* the source at 350um (Jansky/beam) (2) (5)
real*4 FXTBEST3 ! (Jy) ?=0 Total flux value in the source
* at 350um (2)
real*4 e_FXTBEST3 ! (Jy) ?=0 Uncertainty on the total flux value in
* the source at 350um (2)
real*4 AFWHM3 ! (arcsec) FWHM of the source major axis at 350um (2)
real*4 BFWHM3 ! (arcsec) FWHM of the source minor axis at 350um (2)
real*4 PA3 ! (deg) Position angle of the source major axis
* at 350um (2) (6)
real*4 SIGMONO4 ! Monochromatic significance of the source
* extraction at 500 microns (2)
character*1 FM4 ! [0/1] Monochromatic quality flag for the
* source extraction at 500um (2) (4)
real*4 FXPBEST4 ! (Jy/beam) ?=0 Peak flux value in the source at 500um
* (Jansky/beam) (2) (5)
real*4 e_FXPBEST4 ! (Jy/beam) ?=0 Uncertainty on the peak flux value in
* the source at 500um (Jansky/beam) (2) (5)
real*4 FXTBEST4 ! (Jy) ?=0 Total flux value in the source
* at 500um (2)
real*4 e_FXTBEST4 ! (Jy) ?=0 Uncertainty on the total flux value in
* the source at 500um (2)
real*4 AFWHM4 ! (arcsec) FWHM of the source major axis at 500um (2)
real*4 BFWHM4 ! (arcsec) FWHM of the source minor axis at 500um (2)
real*4 PA4 ! (deg) Position angle of the source major axis at
* 500um (2) (6)
real*4 SIGMONO5 ! Monochromatic significance of the source
* extraction in the opacity map (tau_200) (2)
character*1 FM5 ! [0/2] Monochromatic quality flag for the
* source extraction in the opacity map
* (tau_200) (2) (4)
real*4 FXPBEST5 ! (beam-1) ?=0 Peak flux value in the source in the
* opacity map (tau_200) (beam-1) (2) (5)
real*4 e_FXPBEST5 ! (beam-1) ?=0 Uncertainty on the peak flux value in
* the source in the opacity map (tau_200)
* (beam-1) (2) (5)
real*4 FXTBEST5 ! ?=0 Total flux value in the source in the
* opacity map (tau_200) (2)
real*4 e_FXTBEST5 ! ?=0 Uncertainty on the total flux value in
* the source in the opacity map
* (tau_200) (2)
real*4 AFWHM5 ! (arcsec) FWHM of the source major axis in the opacity
* map (tau_200) (2)
real*4 BFWHM5 ! (arcsec) FWHM of the source minor axis in the opacity
* map (tau_200) (2)
real*4 PA5 ! (deg) Position angle of the source major axis in
* the opacity map (tau_200) (2) (6)
real*4 I200 ! (deg) Calculated surface brightness at 200um (7)
real*4 Tdust ! (K) Dust temperature (7)
real*4 NH2_1 ! (cm-2) Column density (7)
real*4 Lbol ! (Lsun) Bolometric luminosity (7)
real*4 Mass_1 ! (Msun) Source mass (7)
real*8 Chi2 ! Chi2 of the SED fit (7)
real*4 NH2bg ! (cm-2) Background column density (7)
real*8 aBE ! Ratio of Bonnor-Ebert mass to estimated
* mass (7)
character*1 WKGalFlag ! [0/3] Galactic/extragalactic flag using WISE
* data and Koenig et al.
* (2012AAS...21932007K) method (8)
character*1 XgalFlag ! [0/1] Galactic/extragalactic flag after
* combining all methods (9)
character*1 StateNIR ! [0/4] State of evolution derived from
* near-IR data (10)
character*1 Class ! [0/9] Class of the embedded YSO (11)
character*1 StateFIR ! [0/2] State of evolution derived from
* mid-IR data (12)
character*1 State ! [0/4] Final state of evolution (13)
*Note (1): Distance quality flag as follows:
* 0 = unreliable
* 1 = reliable estimate from only one method. Needs to be compared with an
* independent method
* 2 = reliable estimates from several independent methods
*Note (2): getsources output are described in Men'shchikov et al.,
* 2012A&A...542A..81M.
*Note (3): We report here the definition given in the output file of getsources,
* FG: Flag identifying global properties over all wavelengths, as follows:
* 0 = isolated source (not blended with any other source in any waveband)
* 1 = blended source (footprints intersect by more than 20% in at least
* one waveband)
* 2 = sub-structured source (the inner 25% area of its footprint contains
* an entire footprint of at least one source)
* 3 = sub-structuring source (causing a larger source to be flagged as
* sub-structured)
*Note (4): We report here the definition given in the output file of getsources,
* FM: Flag identifying monochromatic properties, as follows:
* 0 = no problems identified for the source at this wavelength
* 1 = substantially larger than its characteristic size:
* AFWHMN>sqrt(2)*SCALEN
* 2 = larger than the desired maximum of [93 120 163 202 184] arcsec:
* AFWHMN>sqrt(2)*max(SRCMAXSIZEN,APERTUREN)
* 3 = larger than both the characteristic size and the desired
* maximum size or aperture
* 10 = peak intensity is not measurable: FXP_BESTN/FXP_ERRON<1.0
* 20 = total flux is not measurable: FXT_BESTN/FXT_ERRON<1.0
* 30 = both total flux and peak intensity are not measurable
* 100 = sub-structured (the inner 25% area of its footprint
* contains an entire footprint of at least one source)
* 200 = significance is low: SIG_MONON<3.5
*Note (5): The beam FWHM are 38.5 arcsec for all 160, 250, 350, and 500 microns
* maps, and 40.0 arcsec for the opacity maps.
*Note (6): East from North
*Note (7): Derived from the modified blackbody fit of the getsources total fluxes
* FXTBEST2, FXTBEST3, FXTBEST4, with a fixed spectral index beta=2.
*Note (8): classification of galactic vs extragalactic sources using only WISE
* data and Koenig et al. (2012AAS...21932007K)'s method (see Sect. 4.3)
* as follows:
* 0 = galactic source
* 1 = source contaminated by galaxies
* 2 = the source is a group of galaxies
* 3 = extragalactic source
*Note (9): final classification of galactic vs extragalactic sources as follows:
* 0 = galactic source
* 1 = extragalactic source
*Note (10): classification of starless vs protostellar sources, using only WISE
* data and Koenig et al. (2012AAS...21932007K)'s method (see Sect. 4.4.2)
* as follows:
* 0 = irrelevant (because the source is extragalactic)
* 1 = undetermined (the method is not conclusive)
* 2 = starless
* 3 = protostellar
* 4 = protostellar, but one WISE source within the Herschel source was
* originally classified as extragalactic (WKGalFlag>1 but XgalFlag=0)
*Note (11): Class (I or II) of the embedded YSO derived using WISE data and
* Koenig et al. (2012AAS...21932007K)'s method.
* Class 0 objects are also reported on the basis of WISE 22 microns and
* AKARI 65 microns observations (Sect. 4.4.2). If several NIR objects are
* classified in the Herschel source, or if the object is eligible to
* several classes, the most advanced class is reported.
* 0 = Class 0
* 1 = Class I
* 2 = Class II
* 9 = undetermined or irrelevant
*Note (12): Classification of starless vs protostellar sources, using only
* Herschel data (see Sect. 4.4.1) as follows:
* 0 = undetermined or irrelevant
* 1 = starless
* 2 = protostellar
*Note (13): Final classification of starless vs protostellar sources, combining
* both methods as follows:
* 0 = undetermined or irrelevant
* 1 = probable starless source (flag 1 in Sect. 4.4.3)
* 2 = reliable starless source (flag 2 in Sect. 4.4.3)
* 3 = probable protostellar source (flag 1 Sect. 4.4.3)
* 4 = reliable protostellar source (flag 2 Sect. 4.4.3)
C=============================================================================
C Loading file 'table1.dat' ! General properties of Herschel fields
C Format for file interpretation
1 format(
+ A13,1X,F5.3,1X,F5.3,1X,F5.3,1X,A1,1X,F5.2,1X,I4,1X,F4.1,1X,
+ F4.1,1X,E7.2,2X,E7.2,1X,E7.2,2X,E7.2,1X,A176)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,116
read(1,'(A265)')ar__
read(ar__,1)
+ Field,Dist,E_Dist,e_Dist_1,Flag,RG,AltG,T0_1,T90,Nh2,Mass,C90,
+ C50,Assoc
if (idig(ar__(15:19)).EQ.0) Dist = rNULL__
if(ar__(21:25) .EQ. '') E_Dist = rNULL__
if(ar__(27:31) .EQ. '') e_Dist_1 = rNULL__
if (idig(ar__(35:39)).EQ.0) RG = rNULL__
if (AltG .EQ. 45) AltG = iNULL__
if (idig(ar__(65:71)).EQ.0) Mass = rNULL__
if (idig(ar__(73:79)).EQ.0) C90 = rNULL__
if (idig(ar__(82:88)).EQ.0) C50 = rNULL__
c ..............Just test output...........
write(6,1)
+ Field,Dist,E_Dist,e_Dist_1,Flag,RG,AltG,T0_1,T90,Nh2,Mass,C90,
+ C50,Assoc
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'gccscat.dat' ! The GCC source catalogue
C Format for file interpretation
2 format(
+ I4,1X,A13,1X,F5.3,1X,F5.3,1X,F5.3,1X,A1,1X,F12.8,1X,F12.8,1X,
+ F12.8,1X,F12.8,1X,E9.3,1X,A1,1X,F4.2,1X,E9.3,1X,I3,1X,E10.3,
+ 1X,E9.3,1X,E10.3,1X,E9.3,1X,F6.2,1X,F6.2,1X,F6.2,1X,E9.3,1X,
+ A1,1X,E9.3,1X,E9.3,1X,E9.3,1X,E9.3,1X,F6.2,1X,F6.2,1X,F6.2,1X,
+ E9.3,1X,A1,1X,E9.3,1X,E9.3,1X,E9.3,1X,E9.3,1X,F6.2,1X,F6.2,1X,
+ F6.2,1X,E9.3,1X,A1,1X,E9.3,1X,E9.3,1X,E9.3,1X,E9.3,1X,F6.2,1X,
+ F6.2,1X,F6.2,1X,E9.3,1X,A1,1X,E9.3,1X,E9.3,1X,E9.3,1X,E9.3,1X,
+ F6.2,1X,F6.2,1X,F6.2,1X,E11.5,1X,F5.2,1X,E11.5,1X,E11.5,1X,
+ E11.5,1X,F7.5,1X,E11.5,1X,F8.2,1X,A1,1X,A1,1X,A1,1X,A1,1X,A1,
+ 1X,A1)
C Effective file loading
open(unit=1,status='old',file=
+'gccscat.dat')
write(6,*) '....Loading file: gccscat.dat'
do i__=1,4466
read(1,'(A571)')ar__1
read(ar__1,2)
+ ID,Field_1,Dist_1,E_Dist_2,e_Dist_3,Dflag,RAdeg,DEdeg,GLON,
+ GLAT,SIGGLO,FG,GOOD,SIGMONO1,FM1,FXPBEST1,e_FXPBEST1,FXTBEST1,
+ e_FXTBEST1,AFWHM1,BFWHM1,PA1,SIGMONO2,FM2,FXPBEST2,e_FXPBEST2,
+ FXTBEST2,e_FXTBEST2,AFWHM2,BFWHM2,PA2,SIGMONO3,FM3,FXPBEST3,
+ e_FXPBEST3,FXTBEST3,e_FXTBEST3,AFWHM3,BFWHM3,PA3,SIGMONO4,FM4,
+ FXPBEST4,e_FXPBEST4,FXTBEST4,e_FXTBEST4,AFWHM4,BFWHM4,PA4,
+ SIGMONO5,FM5,FXPBEST5,e_FXPBEST5,FXTBEST5,e_FXTBEST5,AFWHM5,
+ BFWHM5,PA5,I200,Tdust,NH2_1,Lbol,Mass_1,Chi2,NH2bg,aBE,
+ WKGalFlag,XgalFlag,StateNIR,Class,StateFIR,State
if(ar__1(119:121) .EQ. '') FM1 = iNULL__
c ..............Just test output...........
write(6,2)
+ ID,Field_1,Dist_1,E_Dist_2,e_Dist_3,Dflag,RAdeg,DEdeg,GLON,
+ GLAT,SIGGLO,FG,GOOD,SIGMONO1,FM1,FXPBEST1,e_FXPBEST1,FXTBEST1,
+ e_FXTBEST1,AFWHM1,BFWHM1,PA1,SIGMONO2,FM2,FXPBEST2,e_FXPBEST2,
+ FXTBEST2,e_FXTBEST2,AFWHM2,BFWHM2,PA2,SIGMONO3,FM3,FXPBEST3,
+ e_FXPBEST3,FXTBEST3,e_FXTBEST3,AFWHM3,BFWHM3,PA3,SIGMONO4,FM4,
+ FXPBEST4,e_FXPBEST4,FXTBEST4,e_FXTBEST4,AFWHM4,BFWHM4,PA4,
+ SIGMONO5,FM5,FXPBEST5,e_FXPBEST5,FXTBEST5,e_FXTBEST5,AFWHM5,
+ BFWHM5,PA5,I200,Tdust,NH2_1,Lbol,Mass_1,Chi2,NH2bg,aBE,
+ WKGalFlag,XgalFlag,StateNIR,Class,StateFIR,State
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