Conversion of standardized ReadMe file for
file /./ftp/cats/J/other/NewA/56.28 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/other/NewA/56.28 Be stars in MC star clusters NIR properties (Paul+, 2017)
*================================================================================
*NIR properties of Be stars in star clusters in the Magellanic Clouds.
* Paul K.T., Annapurni S., Blesson M., Shruthi S.B.
* <New Astron., 56, 28-49 (2017)>
* =2017NewA...56...28P (SIMBAD/NED BibCode)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table5.dat' ! Optical and NIR photometric magnitudes of Be
candidate stars identified in the LMC and SMC
clusters
integer*4 nr__
parameter (nr__=235) ! Number of records
character*104 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*9 Cluster ! Cluster name (1)
integer*4 Star ! Star number within the cluster,
* WBBe Cluster Star in Simbad (1)
integer*4 RAh ! (h) Right ascension (J2000) (1)
integer*4 RAm ! (min) Right ascension (J2000) (1)
real*4 RAs ! (s) Right ascension (J2000) (1)
character*1 DE_ ! Declination sign (J2000) (1)
integer*4 DEd ! (deg) Declination (J2000) (1)
integer*4 DEm ! (arcmin) Declination (J2000) (1)
real*4 DEs ! (arcsec) Declination (J2000) (1)
real*4 Vmag ! (mag) V magnitude (1)
real*4 e_Vmag ! (mag) rms uncertainty on Vmag (1)
real*4 B_V ! (mag) B-V colour index (1)
real*4 e_B_V ! (mag) rms uncertainty on B-V (1)
real*4 R_Ha ! (mag) R-H{alpha} colour index (1)
real*4 e_R_Ha ! (mag) rms uncertainty on R-Ha (1)
real*4 Jmag ! (mag) J magnitude (2)
real*4 e_Jmag ! (mag) rms uncertainty on Jmag
real*4 Hmag ! (mag) H magnitude (2)
real*4 e_Hmag ! (mag) rms uncertainty on Hmag (2)
real*4 Kmag ! (mag) K magnitude (2)
real*4 e_Kmag ! (mag) rms uncertainty on Kmag
*Note (1): from Wisniewski & Bjorkman (2006, Cat. J/ApJ/652/458).
*Note (2): J, H and K magnitudes are obtained by cross-matching with the
* IRSF-MCPSC catalog (Kato et al., 2007, Cat. II/288).
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table6.dat' ! Optical and NIR photometric magnitudes of Be
candidate stars identified in the LMC and SMC
clusters
integer*4 nr__1
parameter (nr__1=153) ! Number of records
character*93 ar__1 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_1 ! (deg) Right Ascension J2000
real*8 DEdeg_1 ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
character*18 Name ! Star name (Cluster KWBBe NNNN),
* Cl* Cluster KWBBe NNNN in Simbad (1)
integer*4 RAh_1 ! (h) Right ascension (J2000) (1)
integer*4 RAm_1 ! (min) Right ascension (J2000) (1)
real*4 RAs_1 ! (s) Right ascension (J2000) (1)
character*1 DE__1 ! Declination sign (J2000) (1)
integer*4 DEd_1 ! (deg) Declination (J2000) (1)
integer*4 DEm_1 ! (arcmin) Declination (J2000) (1)
real*4 DEs_1 ! (arcsec) Declination (J2000) (1)
real*4 Vmag_1 ! (mag) V magnitude (1)
real*4 V_I ! (mag) V-I colour index (1)
real*4 R_Ha_1 ! (mag) R-H{alpha} colour index (1)
real*4 Jmag_1 ! (mag) J magnitude (2)
real*4 e_Jmag_1 ! (mag) rms uncertainty on Jmag
real*4 Hmag_1 ! (mag) H magnitude (2)
real*4 e_Hmag_1 ! (mag) rms uncertainty on Hmag (2)
real*4 Kmag_1 ! (mag) K magnitude (2)
real*4 e_Kmag_1 ! (mag) rms uncertainty on Kmag
*Note (1): from Keller et al. (1999, Cat. J/A+AS/134/489).
*Note (2): J, H and K magnitudes are obtained by cross-matching with the
* IRSF-MCPSC catalog (Kato et al., 2007, Cat. II/288).
C=============================================================================
C Loading file 'table5.dat' ! Optical and NIR photometric magnitudes of Be
* candidate stars identified in the LMC and SMC
* clusters
C Format for file interpretation
1 format(
+ A9,1X,I3,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F5.2,1X,F5.2,
+ 1X,F4.2,1X,F5.2,1X,F4.2,1X,F5.2,1X,F4.2,1X,F5.2,1X,F4.2,1X,
+ F5.2,1X,F4.2,1X,F5.2,1X,F4.2)
C Effective file loading
open(unit=1,status='old',file=
+'table5.dat')
write(6,*) '....Loading file: table5.dat'
do i__=1,235
read(1,'(A104)')ar__
read(ar__,1)
+ Cluster,Star,RAh,RAm,RAs,DE_,DEd,DEm,DEs,Vmag,e_Vmag,B_V,
+ e_B_V,R_Ha,e_R_Ha,Jmag,e_Jmag,Hmag,e_Hmag,Kmag,e_Kmag
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)
+ Cluster,Star,RAh,RAm,RAs,DE_,DEd,DEm,DEs,Vmag,e_Vmag,B_V,
+ e_B_V,R_Ha,e_R_Ha,Jmag,e_Jmag,Hmag,e_Hmag,Kmag,e_Kmag
write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table6.dat' ! Optical and NIR photometric magnitudes of Be
* candidate stars identified in the LMC and SMC
* clusters
C Format for file interpretation
2 format(
+ A18,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F5.2,1X,F5.2,1X,
+ F5.2,1X,F4.2,1X,F5.2,1X,F4.2,1X,F5.2,1X,F4.2,1X,F5.2,1X,F4.2)
C Effective file loading
open(unit=1,status='old',file=
+'table6.dat')
write(6,*) '....Loading file: table6.dat'
do i__=1,153
read(1,'(A93)')ar__1
read(ar__1,2)
+ Name,RAh_1,RAm_1,RAs_1,DE__1,DEd_1,DEm_1,DEs_1,Vmag_1,V_I,
+ R_Ha_1,Jmag_1,e_Jmag_1,Hmag_1,e_Hmag_1,Kmag_1,e_Kmag_1
RAdeg_1 = rNULL__
DEdeg_1 = 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 .GT. -180) RAdeg_1=RAh_1*15.
if(RAm_1 .GT. -180) RAdeg_1=RAdeg_1+RAm_1/4.
if(RAs_1 .GT. -180) RAdeg_1=RAdeg_1+RAs_1/240.
if(DEd_1 .GE. 0) DEdeg_1=DEd_1
if(DEm_1 .GE. 0) DEdeg_1=DEdeg_1+DEm_1/60.
if(DEs_1 .GE. 0) DEdeg_1=DEdeg_1+DEs_1/3600.
if(DE__1.EQ.'-'.AND.DEdeg_1.GE.0) DEdeg_1=-DEdeg_1
c ..............Just test output...........
write(6,2)
+ Name,RAh_1,RAm_1,RAs_1,DE__1,DEd_1,DEm_1,DEs_1,Vmag_1,V_I,
+ R_Ha_1,Jmag_1,e_Jmag_1,Hmag_1,e_Hmag_1,Kmag_1,e_Kmag_1
write(6,'(6H Pos: 2F8.4)') RAdeg_1,DEdeg_1
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end