Conversion of standardized ReadMe file for
file /./home/cats/J/A_A/525/A149 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 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/525/A149 Red MSX Survey (RMS): bolometric fluxes of YSOs (Mottram+, 2011)
*================================================================================
*The Red MSX Survey survey: the bolometric fluxes and luminosity distributions of
*young massive stars.
* Mottram J.C., Hoare M.G., Urquhart J.S., Lumsden S.L., Oudmaijer R.D.,
* Robitaille T.P., Moore T.J.T, Davies B., Stead J.J.
* <Astron. Astrophys. 525, A149 (2011)>
* =2011A&A...525A.149M
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Bolometric fluxes for sources with far-IR data
using SED fitting
integer*4 nr__
parameter (nr__=1173) ! Number of records
character*103 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*18 MSX6C (nr__) ! Name of target, GLLL.llll+BB.bbbbA
integer*4 RAh (nr__) ! (h) Right Ascension J2000 (hours)
integer*4 RAm (nr__) ! (min) Right Ascension J2000 (minutes)
real*4 RAs (nr__) ! (s) Right Ascension J2000 (seconds)
character*1 DE_ (nr__) ! Declination J2000 (sign)
integer*4 DEd (nr__) ! (deg) Declination J2000 (degrees)
integer*4 DEm (nr__) ! (arcmin) Declination J2000 (minutes)
real*4 DEs (nr__) ! (arcsec) Declination J2000 (seconds)
character*7 Class (nr__) ! RMS classification (G1)
integer*4 Np (nr__) ! Number of detected flux data points used
* for SED fit
character*1 v2M (nr__) ! [Y/N] Flag for inclusion of 2MASS data
character*1 T2 (nr__) ! [Y/N] Flag for inclusion of TIMMI2 data (1)
character*1 far (nr__) ! [I/M] Inclusion of far-IR IRAS Galaxy Atlas
* data (I), or MIPSGAL (M) data (2)
character*1 sc (nr__) ! [Y/N] Flag for inclusion of sub-mm SCUBA data
character*1 mm (nr__) ! [1234N] Flag for 1.2mm data (3)
real*4 chi2b (nr__) ! ? The chi-squared of the best fit
real*4 dchi2 (nr__) ! ? The delta-chi-squared at which at
* least 10 fits exist
integer*4 Nfit (nr__) ! ? The number of fits
real*4 Flux (nr__) ! (10-11W/m2) Measured bolometric flux from the SED
real*4 e_Flux (nr__) ! (10-11W/m2) Error in the measured bolometric flux
character*2 dst (nr__) ! [s nf] Whether the distance ambiguity has
* been solved (s) or not (nf)
real*4 ApC (nr__) ! Aperture correction used for large-beam fluxes
* (apportioning correction, 1=no apportioning)
character*1 ApT (nr__) ! [NGTS] Type of apportioning used:
* N=no (ApC=1), G=GLIMPSE, T=TIMMI2, S=split
*Note (1): Data from Mottram et al. (2007A&A...476.1019M)
*Note (2): Data from Mottram et al. (2010A&A...510A..89M)
*Note (3): Flag for 1.2mm data as follows:
* N = no
* 1 = Beuther et al. (2002ApJ...566..945B),
* 2 = Faundez et al. (2004A&A...426...97F),
* 3 = Hill et al. (2005MNRAS.363..405H),
* 4 = Beltran et al. (2006A&A...447..221B)
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Bolometric fluxes for sources with no far-IR
data using Fbol/F21
integer*4 nr__1
parameter (nr__1=280) ! Number of records
character*96 ar__1 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_1 (nr__1) ! (deg) Right Ascension J2000
real*8 DEdeg_1 (nr__1) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
character*18 MSX6C_1 (nr__1) ! Name of target, GLLL.llll+BB.bbbbA
integer*4 RAh_1 (nr__1) ! (h) Right Ascension J2000 (hours)
integer*4 RAm_1 (nr__1) ! (min) Right Ascension J2000 (minutes)
real*4 RAs_1 (nr__1) ! (s) Right Ascension J2000 (seconds)
character*1 DE__1 (nr__1) ! Declination J2000 (sign)
integer*4 DEd_1 (nr__1) ! (deg) Declination J2000 (degrees)
integer*4 DEm_1 (nr__1) ! (arcmin) Declination J2000 (minutes)
real*4 DEs_1 (nr__1) ! (arcsec) Declination J2000 (seconds)
character*7 Class_1 (nr__1) ! MSX Source classification (G1)
real*8 MSX21 (nr__1) ! (Jy) MSX PSC 21 micron flux
real*4 e_MSX21 (nr__1) ! (Jy) Error in the MSX PSC 21 micron flux
real*8 Flux_1 (nr__1) ! (10-11W/m2) Measured bolometric flux using Fbol/F21
real*8 E_Flux_1 (nr__1) ! (10-11W/m2) Positive error in the measured bolometric flux
real*8 e_Flux_2 (nr__1) ! (10-11W/m2) Negative error in the measured bolometric flux
real*4 ApC_1 (nr__1) ! Aperture correction used for large-beam fluxes
character*1 ApT_1 (nr__1) ! [NGTS] Type of apportioning used:
* N=no (ApC=1), G=GLIMPSE, T=TIMMI2, S=split
C=============================================================================
C Loading file 'table1.dat' ! Bolometric fluxes for sources with far-IR data
* using SED fitting
C Format for file interpretation
1 format(
+ A18,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,A7,1X,I2,1X,
+ A1,1X,A1,1X,A1,1X,A1,1X,A1,1X,F5.1,1X,F4.1,1X,I4,1X,F6.3,1X,
+ F6.3,1X,A2,1X,F4.2,1X,A1)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,1173
read(1,'(A103)')ar__
read(ar__,1)
+ MSX6C(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),Class(i__),Np(i__),v2M(i__),T2(i__),
+ far(i__),sc(i__),mm(i__),chi2b(i__),dchi2(i__),Nfit(i__),
+ Flux(i__),e_Flux(i__),dst(i__),ApC(i__),ApT(i__)
if(ar__(65:69) .EQ. '') chi2b(i__) = rNULL__
if(ar__(71:74) .EQ. '') dchi2(i__) = rNULL__
if(ar__(76:79) .EQ. '') Nfit(i__) = iNULL__
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)
+ MSX6C(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),Class(i__),Np(i__),v2M(i__),T2(i__),
+ far(i__),sc(i__),mm(i__),chi2b(i__),dchi2(i__),Nfit(i__),
+ Flux(i__),e_Flux(i__),dst(i__),ApC(i__),ApT(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' ! Bolometric fluxes for sources with no far-IR
* data using Fbol/F21
C Format for file interpretation
2 format(
+ A18,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,A7,1X,F7.2,
+ 1X,F6.2,1X,F7.3,1X,F7.3,1X,F7.3,1X,F4.2,1X,A1)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,280
read(1,'(A96)')ar__1
read(ar__1,2)
+ MSX6C_1(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),
+ DEd_1(i__),DEm_1(i__),DEs_1(i__),Class_1(i__),MSX21(i__),
+ e_MSX21(i__),Flux_1(i__),E_Flux_1(i__),e_Flux_2(i__),
+ ApC_1(i__),ApT_1(i__)
RAdeg_1(i__) = rNULL__
DEdeg_1(i__) = rNULL__
c Derive coordinates RAdeg_1 and DEdeg_1 from input data
c (RAdeg_1 and DEdeg_1 are set to rNULL__ when unknown)
if(RAh_1(i__) .GT. -180) RAdeg_1(i__)=RAh_1(i__)*15.
if(RAm_1(i__) .GT. -180) RAdeg_1(i__)=RAdeg_1(i__)+RAm_1(i__)/4.
if(RAs_1(i__) .GT. -180) RAdeg_1(i__)=RAdeg_1(i__)+RAs_1(i__)/240.
if(DEd_1(i__) .GE. 0) DEdeg_1(i__)=DEd_1(i__)
if(DEm_1(i__) .GE. 0) DEdeg_1(i__)=DEdeg_1(i__)+DEm_1(i__)/60.
if(DEs_1(i__) .GE. 0) DEdeg_1(i__)=DEdeg_1(i__)+DEs_1(i__)/3600.
if(DE__1(i__).EQ.'-'.AND.DEdeg_1(i__).GE.0) DEdeg_1(i__)=-DEdeg_1(i__)
c ..............Just test output...........
write(6,2)
+ MSX6C_1(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),
+ DEd_1(i__),DEm_1(i__),DEs_1(i__),Class_1(i__),MSX21(i__),
+ e_MSX21(i__),Flux_1(i__),E_Flux_1(i__),e_Flux_2(i__),
+ ApC_1(i__),ApT_1(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_1(i__),DEdeg_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end