Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/576/880 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-15
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/576/880 CCD UBV photometry of h and {chi} Per (Slesnick+, 2002)
*================================================================================
*The star formation history and mass function of the double cluster
*h and {chi} Persei.
* Slesnick C.L., Hillenbrand L.A., Massey P.
* <Astrophys. J. 576, 880 (2002)>
* =2002ApJ...576..880S
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Observational Data
integer*4 nr__
parameter (nr__=4528) ! Number of records
character*148 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 SHM (nr__) ! Catalog Number ([SHM2002] in SIMBAD)
integer*4 RAh (nr__) ! (h) Hour of Right Ascension (J2000)
integer*4 RAm (nr__) ! (min) Minute of Right Ascension (J2000)
real*4 RAs (nr__) ! (s) Second of Right Ascension (J2000)
character*1 DE_ (nr__) ! Sign of declination (J2000)
integer*4 DEd (nr__) ! (deg) Degree of Declination (J2000)
integer*4 DEm (nr__) ! (arcmin) Arcminute of of Declination (J2000)
real*4 DEs (nr__) ! (arcsec) Arcsecond of Declination (J2000)
real*4 Vmag (nr__) ! (mag) The visual magnitude
real*4 B_V (nr__) ! (mag) The (B-V) color
real*4 U_B (nr__) ! (mag) The (U-B) color
real*4 D_h (nr__) ! (deg) Distance from the center of h Per
real*4 D_chi (nr__) ! (deg) Distance from the center of Chi Per
character*3 Memb (nr__) ! Cluster membership (1)
character*9 SpType (nr__) ! Adopted MK Spectral Classification (2)
character*21 SpType1 (nr__) ! MK Spectral Classification from the
* Literature (3)
character*45 Onames (nr__) ! Cross identifications from the Litterature (4)
*Note (1): Cluster membership:
* far = not a member
* h = h Per member
* chi = chi Per member
*Note (2): Note on SpType:
* *: indicates that we used a spectral type from the literature in
* our analysis.
*Note (3): Reference code given in parentheses.
* 1 = Schild (1965ApJ...142..979S)
* 2 = Johnson & Morgan (1955ApJ...122..429J)
* 3 = Slettlebak (1968ApJ...154..933S)
* 4 = Appenzeller (1967PASP...79..102A)
* 5 = Bidelman (1947ApJ...105..492B)
* 6 = Morgan, Code & Whitford (1955ApJS....2...41M)
*Note (4): Our cross-identifications are not complete and focus on the
* brighter stars and those for which we have spectral types. When
* available, HD or BD numbers are given. All IDs marked "h-XXX" or
* "chi-XXX" are from Wildey (1964ApJS....8..439W).
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Derived Quantities for Probable Cluster Members
integer*4 nr__1
parameter (nr__1=279) ! Number of records
character*40 ar__1 ! Full-size record
integer*4 SHM_1 (nr__1) ! The SHM catalog number ([SHM2002] in SIMBAD)
character*2 HRD (nr__1) ! [psa ] The HR diagram placement code (1)
real*4 logT (nr__1) ! ([K]) Log of the effective temperature
real*4 E_B_V (nr__1) ! (mag) The (B-V) color excess
real*4 VMag_1 (nr__1) ! (mag) The absolute V band magnitude
real*4 Mbol (nr__1) ! (mag) The bolometric absolute magnitude
real*4 Mass (nr__1) ! (solMass) Mass in solar units
*Note (1): HR diagram placement code:
* p = star placed photometrically
* s = star placed spectroscopically
* a = the mean E(B-V) was adopted
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! Derived Quantities for Probable Field Stars
integer*4 nr__2
parameter (nr__2=411) ! Number of records
character*40 ar__2 ! Full-size record
integer*4 SHM_2 (nr__2) ! The SHM catalog number ([SHM2002] in SIMBAD)
character*2 HRD_1 (nr__2) ! [psa ] The HR diagram placement code (1)
real*4 logT_1 (nr__2) ! ([K]) Log of the effective temperature
real*4 E_B_V_1 (nr__2) ! (mag) The (B-V) color excess
real*4 VMag_2 (nr__2) ! (mag) The absolute V band magnitude
real*4 Mbol_1 (nr__2) ! (mag) The bolometric absolute magnitude
real*4 Mass_1 (nr__2) ! (solMass) Mass in solar units
*Note (1): HR diagram placement code:
* p = star placed photometrically
* s = star placed spectroscopically
* a = the mean E(B-V) was adopted
C=============================================================================
C Loading file 'table1.dat' ! Observational Data
C Format for file interpretation
1 format(
+ I4,1X,I1,1X,I2,1X,F5.2,A1,I2,1X,I2,1X,F4.1,1X,F6.3,2X,F6.3,2X,
+ F6.3,3X,F5.3,3X,F5.3,1X,A3,1X,A9,1X,A21,2X,A45)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,4528
read(1,'(A148)')ar__
read(ar__,1)
+ SHM(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),Vmag(i__),B_V(i__),U_B(i__),D_h(i__),
+ D_chi(i__),Memb(i__),SpType(i__),SpType1(i__),Onames(i__)
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)
+ SHM(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),Vmag(i__),B_V(i__),U_B(i__),D_h(i__),
+ D_chi(i__),Memb(i__),SpType(i__),SpType1(i__),Onames(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' ! Derived Quantities for Probable Cluster Members
C Format for file interpretation
2 format(I4,1X,A2,1X,F5.3,3X,F4.2,2X,F5.2,2X,F5.2,2X,F4.1)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,279
read(1,'(A40)')ar__1
read(ar__1,2)
+ SHM_1(i__),HRD(i__),logT(i__),E_B_V(i__),VMag_1(i__),
+ Mbol(i__),Mass(i__)
c ..............Just test output...........
write(6,2)
+ SHM_1(i__),HRD(i__),logT(i__),E_B_V(i__),VMag_1(i__),
+ Mbol(i__),Mass(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table3.dat' ! Derived Quantities for Probable Field Stars
C Format for file interpretation
3 format(I4,1X,A2,1X,F5.3,3X,F4.2,2X,F5.2,2X,F5.2,2X,F4.1)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,411
read(1,'(A40)')ar__2
read(ar__2,3)
+ SHM_2(i__),HRD_1(i__),logT_1(i__),E_B_V_1(i__),VMag_2(i__),
+ Mbol_1(i__),Mass_1(i__)
c ..............Just test output...........
write(6,3)
+ SHM_2(i__),HRD_1(i__),logT_1(i__),E_B_V_1(i__),VMag_2(i__),
+ Mbol_1(i__),Mass_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end