Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_A/446/773 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-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/A+A/446/773 GLMP sample of galactic OH/IR stars (Jimenez-Esteban+, 2006)
*================================================================================
*An infrared study of galactic OH/IR stars.
*II. The "GLMP sample" of red oxygen-rich AGB stars
* Jimenez-Esteban F.M., Garcia-Lario P., Engels D., Perea Calderon J.V.
* <Astron. Astrophys. 446, 773 (2006)>
* =2006A&A...446..773J
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! Astrometric information for the sources for
which a near infrared counterpart was found.
integer*4 nr__
parameter (nr__=59) ! Number of records
character*99 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 GLMP (nr__) ! GLMP number (Cat. J/A+AS/126/479)
character*10 IRAS (nr__) ! IRAS name
character*1 v2M (nr__) ! [*] Tentative 2MASS identification
integer*4 RAh (nr__) ! (h) 2MASS right ascension (J2000)
integer*4 RAm (nr__) ! (min) 2MASS right ascension (J2000)
real*4 RAs (nr__) ! (s) 2MASS right ascension (J2000)
character*1 DE_ (nr__) ! 2MASS declination sign (J2000)
integer*4 DEd (nr__) ! (deg) 2MASS declination (J2000)
integer*4 DEm (nr__) ! (arcmin) 2MASS declination (J2000)
real*4 DEs (nr__) ! (arcsec) 2MASS declination (J2000)
integer*4 oRA_2M (nr__) ! (arcsec) Relative distance between 2MASS and IRAS (RA)
integer*4 oDE_2M (nr__) ! (arcsec) Relative distance between 2MASS and IRAS (Dec)
integer*4 oRA_MSX (nr__) ! (arcsec) ? Relative distance between MSX and IRAS (RA)
integer*4 oDE_MSX (nr__) ! (arcsec) ? Relative distance between MSX and IRAS (Dec)
character*16 MSX6CG (nr__) ! MSX name (MSX6C GLLL.llll+BB.bbbb)
character*2 Opt (nr__) ! [**] Shows optical counterpart
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table4.dat' ! Astrometric information for the sources for
which a near infrared counterpart was not found
integer*4 nr__1
parameter (nr__1=35) ! Number of records
character*80 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)
integer*4 GLMP_1 (nr__1) ! GLMP number
character*10 IRAS_1 (nr__1) ! IRAS name
character*1 f_IRAS (nr__1) ! [*] IRAS coordinates
integer*4 RAh_1 (nr__1) ! (h) MSX right ascension (J2000)
integer*4 RAm_1 (nr__1) ! (min) MSX right ascension (J2000)
real*4 RAs_1 (nr__1) ! (s) MSX right ascension (J2000)
character*1 DE__1 (nr__1) ! MSX declination sign (J2000)
integer*4 DEd_1 (nr__1) ! (deg) MSX declination (J2000)
integer*4 DEm_1 (nr__1) ! (arcmin) MSX declination (J2000)
integer*4 DEs_1 (nr__1) ! (arcsec) MSX declination (J2000)
integer*4 oRA_MSX_1 (nr__1) ! (arcsec) ? Relative distance between MSX and IRAS (RA)
integer*4 oDE_MSX_1 (nr__1) ! (arcsec) ? Relative distance between MSX and IRAS (Dec)
character*16 MSX6CG_1 (nr__1) ! MSX name (MSX6C GLLL.llll+BB.bbbb)
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table5.dat' ! Near infrared photometry of the GLMP sources for
which a near infrared counterpart was found
integer*4 nr__2
parameter (nr__2=59) ! Number of records
character*82 ar__2 ! Full-size record
character*10 IRAS_2 (nr__2) ! IRAS name
character*1 n_Jmag (nr__2) ! [* ] Accuracy of the J photometry is affected
* by blending according to 2MASS catalogue
character*2 f_Jmag (nr__2) ! [* ] J photometry obtained from the 2MASS images
character*1 l_Jmag (nr__2) ! Upper or lower limit indicator
real*4 Jmag (nr__2) ! (mag) J magnitude
real*4 e_Jmag (nr__2) ! (mag) ? J magnitude uncertainty
character*1 n_Hmag (nr__2) ! [* ] Accuracy of the H photometry is affected
* by blending according to 2MASS catalogue
character*2 f_Hmag (nr__2) ! [* ] H photometry obtained from the 2MASS images
character*1 l_Hmag (nr__2) ! Upper or lower limit indicator
real*4 Hmag (nr__2) ! (mag) H magnitude
real*4 e_Hmag (nr__2) ! (mag) ? H magnitude uncertainty
character*1 n_Kmag (nr__2) ! [* ] Accuracy of the K photometry is affected
* by blending according to 2MASS catalogue
character*2 f_Kmag (nr__2) ! [* ] K photometry obtained from 2MASS images
character*1 l_Kmag (nr__2) ! Upper or lower limit indicator
real*4 Kmag (nr__2) ! (mag) K magnitude
real*4 e_Kmag (nr__2) ! (mag) ? K magnitude uncertainty
C=============================================================================
C Loading file 'table3.dat' ! Astrometric information for the sources for
* which a near infrared counterpart was found.
C Format for file interpretation
1 format(
+ I3,4X,A10,1X,A1,4X,I2,1X,I2,1X,F5.2,2X,A1,I2,1X,I2,1X,F4.1,4X,
+ I3,3X,I3,3X,I3,3X,I3,5X,A16,3X,A2)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,59
read(1,'(A99)')ar__
read(ar__,1)
+ GLMP(i__),IRAS(i__),v2M(i__),RAh(i__),RAm(i__),RAs(i__),
+ DE_(i__),DEd(i__),DEm(i__),DEs(i__),oRA_2M(i__),oDE_2M(i__),
+ oRA_MSX(i__),oDE_MSX(i__),MSX6CG(i__),Opt(i__)
if(ar__(64:66) .EQ. '') oRA_MSX(i__) = iNULL__
if(ar__(70:72) .EQ. '') oDE_MSX(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)
+ GLMP(i__),IRAS(i__),v2M(i__),RAh(i__),RAm(i__),RAs(i__),
+ DE_(i__),DEd(i__),DEm(i__),DEs(i__),oRA_2M(i__),oDE_2M(i__),
+ oRA_MSX(i__),oDE_MSX(i__),MSX6CG(i__),Opt(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 'table4.dat' ! Astrometric information for the sources for
* which a near infrared counterpart was not found
C Format for file interpretation
2 format(
+ I3,4X,A10,1X,A1,4X,I2,1X,I2,1X,F4.1,3X,A1,I2,1X,I2,1X,I2,6X,
+ I3,3X,I3,3X,A16)
C Effective file loading
open(unit=1,status='old',file=
+'table4.dat')
write(6,*) '....Loading file: table4.dat'
do i__=1,35
read(1,'(A80)')ar__1
read(ar__1,2)
+ GLMP_1(i__),IRAS_1(i__),f_IRAS(i__),RAh_1(i__),RAm_1(i__),
+ RAs_1(i__),DE__1(i__),DEd_1(i__),DEm_1(i__),DEs_1(i__),
+ oRA_MSX_1(i__),oDE_MSX_1(i__),MSX6CG_1(i__)
if(ar__1(52:54) .EQ. '') oRA_MSX_1(i__) = iNULL__
if(ar__1(58:60) .EQ. '') oDE_MSX_1(i__) = iNULL__
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)
+ GLMP_1(i__),IRAS_1(i__),f_IRAS(i__),RAh_1(i__),RAm_1(i__),
+ RAs_1(i__),DE__1(i__),DEd_1(i__),DEm_1(i__),DEs_1(i__),
+ oRA_MSX_1(i__),oDE_MSX_1(i__),MSX6CG_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=============================================================================
C Loading file 'table5.dat' ! Near infrared photometry of the GLMP sources for
* which a near infrared counterpart was found
C Format for file interpretation
3 format(
+ A10,3X,A1,2X,A2,3X,A1,F5.2,3X,F4.2,3X,A1,2X,A2,3X,A1,F5.2,3X,
+ F4.2,3X,A1,2X,A2,3X,A1,F5.2,3X,F4.2)
C Effective file loading
open(unit=1,status='old',file=
+'table5.dat')
write(6,*) '....Loading file: table5.dat'
do i__=1,59
read(1,'(A82)')ar__2
read(ar__2,3)
+ IRAS_2(i__),n_Jmag(i__),f_Jmag(i__),l_Jmag(i__),Jmag(i__),
+ e_Jmag(i__),n_Hmag(i__),f_Hmag(i__),l_Hmag(i__),Hmag(i__),
+ e_Hmag(i__),n_Kmag(i__),f_Kmag(i__),l_Kmag(i__),Kmag(i__),
+ e_Kmag(i__)
if(ar__2(31:34) .EQ. '') e_Jmag(i__) = rNULL__
if(ar__2(55:58) .EQ. '') e_Hmag(i__) = rNULL__
if(ar__2(79:82) .EQ. '') e_Kmag(i__) = rNULL__
c ..............Just test output...........
write(6,3)
+ IRAS_2(i__),n_Jmag(i__),f_Jmag(i__),l_Jmag(i__),Jmag(i__),
+ e_Jmag(i__),n_Hmag(i__),f_Hmag(i__),l_Hmag(i__),Hmag(i__),
+ e_Hmag(i__),n_Kmag(i__),f_Kmag(i__),l_Kmag(i__),Kmag(i__),
+ e_Kmag(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end