Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_A/472/241 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-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/472/241 UV Flux distributions of gamma Dor stars (Gerbaldi+, 2007)
*================================================================================
*UV Flux distributions of gamma Dor stars.
* Gerbaldi M., Faraggiana R., Caffau E.
* <Astron. Astrophys. 472, 241 (2007)>
* =2007A&A...472..241G
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Reddening and atmospheric parameters for the
gamma Dor stars
integer*4 nr__
parameter (nr__=40) ! Number of records
character*182 ar__ ! Full-size record
integer*4 HD (nr__) ! HD number (1)
character*2 n_HD (nr__) ! [no] "no" indicates star without Beta-index
* measurement
real*4 E_b_y (nr__) ! (mag) Reddening computed with the Moon program (2)
integer*4 Teff1 (nr__) ! (K) Effective temperature computed with the
* Moon & Dworetsky program (MD) (2)
real*4 logg1 (nr__) ! ([cm/s2]) Surface gravity computed with the
* Moon & Dworetsky program (MD) (2)
integer*4 Teff2 (nr__) ! (K) ? Effective temperature computed with the
* Kunzli et al. program (Gen) (2)
real*4 logg2 (nr__) ! ([cm/s2]) ? Surface gravity computed with the
* Kunzli et al. program (Gen) (2)
real*4 v_M_H_ (nr__) ! ([Sun]) ? Metallicity computed with the
* Kunzli et al. program (Gen) (2)
real*4 VMAG1 (nr__) ! (mag) ? Visual absolute magnitude photometrically
* derived using calibration of uvbyBeta
* photometry adopted by Moon (1985) (2)
real*4 VMAG0 (nr__) ! (mag) ? Visual absolute magnitude derived using
* Hipparcos parallaxes
character*1 Note (nr__) ! [abcd] Note about binarity (3)
character*127 Rem (nr__) ! Remarks (4)
*Note (1):
* In the case of a binary system, the gamma Dor is the A component,
* except for HD 221866 where the gamma Dor star is likely to be the
* B component.
*
* For the SB2 stars, HD 86371 and HD 113867, it is not clear
* which component is the gamma Dor variable (Henry & Fekel,
* 2003AJ....126.3058H); in fact, both components could pulsate
* (Henry et al., 2005, Cat. J/AJ/129/2815)
*Note (2): Program references as follows:
* Moon (1985) = Moon program, 1985, Comm. from the Univ of London Obs.
* 78 and revision in 1985, private comm.
* MD = Moon & Dworetsky, 1985MNRAS.217..305M
* Gen = Kunzli et al., 1997A&AS..122...51K
*Note (3): For the individual components of the SB2 systems the Vmag and
* the spectral types are taken as follows:
* a = Henry & Fekel (2002PASP..114..988H) and Faraggiana & Gerbaldi
* (2004ASPC..318..316F). For HD 108100 there is a controversy on
* its SB2 nature (Henry & Fekel (2002PASP..114..988H) and
* Faraggiana & Gerbaldi (2004ASPC..318..316F).
* b = Henry & Fekel, 2003AJ....126.3058H
* c = Henry et al. (2005AJ....129.2815H)
* d = Kaye et al. (2004PASP..116..558K) and
* Fekel et al. (2003AJ....125.2196F).
*Note (4): The remarks are from Henry et al. (2005, Cat. <J/AJ/129/2815>)
* complemented by duplicity detection from the Hipparcos Catalogue
* (1997, Cat. <I/239>), the Washington Visual Double Star Catalogue
* (WDS, 1997, Cat. <I/237>) and the Fourth catalogue of interferometric
* measurements (Hartkopf et al., 2003,
* http://ad.usno.navy.mil/wds/int4.html). In case of several values of
* the separation taken from WDS, the smallest one is retained.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Reddening and atmospheric parameters for a
sample of reference stars
integer*4 nr__1
parameter (nr__1=41) ! Number of records
character*182 ar__1 ! Full-size record
integer*4 HD_1 (nr__1) ! HD number (1)
character*2 n_HD_1 (nr__1) ! [no] "no" indicates star without Beta-index
* measurement
real*4 E_b_y_1 (nr__1) ! (mag) Reddening computed with the Moon program (2)
integer*4 Teff1_1 (nr__1) ! (K) Effective temperature computed with the
* Moon & Dworetsky program (MD) (2)
real*4 logg1_1 (nr__1) ! ([cm/s2]) Surface gravity computed with the
* Moon & Dworetsky program (MD) (2)
integer*4 Teff2_1 (nr__1) ! (K) ? Effective temperature computed with the
* Kunzli et al. program (Gen) (2)
real*4 logg2_1 (nr__1) ! ([cm/s2]) ? Surface gravity computed with the
* Kunzli et al. program (Gen) (2)
real*4 v_M_H__1 (nr__1) ! ([Sun]) ? Metallicity computed with the
* Kunzli et al. program (Gen) (2)
real*4 VMAG1_1 (nr__1) ! (mag) ? Visual absolute magnitude photometrically
* derived using calibration of uvbyBeta
* photometry adopted by Moon (1985) (2)
real*4 VMAG0_1 (nr__1) ! (mag) ? Visual absolute magnitude derived using
* Hipparcos parallaxes
character*1 Note_1 (nr__1) ! [abcd] Note about binarity (3)
character*127 Rem_1 (nr__1) ! Remarks (4)
*Note (1):
* In the case of a binary system, the gamma Dor is the A component,
* except for HD 221866 where the gamma Dor star is likely to be the
* B component.
*
* For the SB2 stars, HD 86371 and HD 113867, it is not clear
* which component is the gamma Dor variable (Henry & Fekel,
* 2003AJ....126.3058H); in fact, both components could pulsate
* (Henry et al., 2005, Cat. J/AJ/129/2815)
*Note (2): Program references as follows:
* Moon (1985) = Moon program, 1985, Comm. from the Univ of London Obs.
* 78 and revision in 1985, private comm.
* MD = Moon & Dworetsky, 1985MNRAS.217..305M
* Gen = Kunzli et al., 1997A&AS..122...51K
*Note (3): For the individual components of the SB2 systems the Vmag and
* the spectral types are taken as follows:
* a = Henry & Fekel (2002PASP..114..988H) and Faraggiana & Gerbaldi
* (2004ASPC..318..316F). For HD 108100 there is a controversy on
* its SB2 nature (Henry & Fekel (2002PASP..114..988H) and
* Faraggiana & Gerbaldi (2004ASPC..318..316F).
* b = Henry & Fekel, 2003AJ....126.3058H
* c = Henry et al. (2005AJ....129.2815H)
* d = Kaye et al. (2004PASP..116..558K) and
* Fekel et al. (2003AJ....125.2196F).
*Note (4): The remarks are from Henry et al. (2005, Cat. <J/AJ/129/2815>)
* complemented by duplicity detection from the Hipparcos Catalogue
* (1997, Cat. <I/239>), the Washington Visual Double Star Catalogue
* (WDS, 1997, Cat. <I/237>) and the Fourth catalogue of interferometric
* measurements (Hartkopf et al., 2003,
* http://ad.usno.navy.mil/wds/int4.html). In case of several values of
* the separation taken from WDS, the smallest one is retained.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! Visual magnitude for the 10 SB2 or close VB
gamma Dor stars
integer*4 nr__2
parameter (nr__2=10) ! Number of records
character*28 ar__2 ! Full-size record
integer*4 HD_2 (nr__2) ! HD number
real*4 Vmag (nr__2) ! (mag) V-Johnson magnitude from the Hipparcos
* Catalogue (Cat. <I/239>)
real*4 V_A (nr__2) ! (mag) ? V-Johnson magnitude for the component A
real*4 V_B (nr__2) ! (mag) ? V-Johnson magnitude for the component B
character*1 n_HD_2 (nr__2) ! [*] * indicates a note in notes.dat file
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'notes.dat' ! Individual notes
integer*4 nr__3
parameter (nr__3=15) ! Number of records
character*80 ar__3 ! Full-size record
integer*4 HD_3 (nr__3) ! HD number
character*73 Note_2 (nr__3) ! Note
C=============================================================================
C Loading file 'table1.dat' ! Reddening and atmospheric parameters for the
* gamma Dor stars
C Format for file interpretation
1 format(
+ I6,1X,A2,1X,F6.3,1X,I4,1X,F4.2,1X,I4,1X,F4.2,1X,F5.2,1X,F4.2,
+ 1X,F4.2,1X,A1,1X,A127)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,40
read(1,'(A182)')ar__
read(ar__,1)
+ HD(i__),n_HD(i__),E_b_y(i__),Teff1(i__),logg1(i__),Teff2(i__),
+ logg2(i__),v_M_H_(i__),VMAG1(i__),VMAG0(i__),Note(i__),
+ Rem(i__)
if(ar__(28:31) .EQ. '') Teff2(i__) = iNULL__
if(ar__(33:36) .EQ. '') logg2(i__) = rNULL__
if(ar__(38:42) .EQ. '') v_M_H_(i__) = rNULL__
if(ar__(44:47) .EQ. '') VMAG1(i__) = rNULL__
if(ar__(49:52) .EQ. '') VMAG0(i__) = rNULL__
c ..............Just test output...........
write(6,1)
+ HD(i__),n_HD(i__),E_b_y(i__),Teff1(i__),logg1(i__),Teff2(i__),
+ logg2(i__),v_M_H_(i__),VMAG1(i__),VMAG0(i__),Note(i__),
+ Rem(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table2.dat' ! Reddening and atmospheric parameters for a
* sample of reference stars
C Format for file interpretation
2 format(
+ I6,1X,A2,1X,F6.3,1X,I4,1X,F4.2,1X,I4,1X,F4.2,1X,F5.2,1X,F4.2,
+ 1X,F4.2,1X,A1,1X,A127)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,41
read(1,'(A182)')ar__1
read(ar__1,2)
+ HD_1(i__),n_HD_1(i__),E_b_y_1(i__),Teff1_1(i__),logg1_1(i__),
+ Teff2_1(i__),logg2_1(i__),v_M_H__1(i__),VMAG1_1(i__),
+ VMAG0_1(i__),Note_1(i__),Rem_1(i__)
if(ar__1(28:31) .EQ. '') Teff2_1(i__) = iNULL__
if(ar__1(33:36) .EQ. '') logg2_1(i__) = rNULL__
if(ar__1(38:42) .EQ. '') v_M_H__1(i__) = rNULL__
if(ar__1(44:47) .EQ. '') VMAG1_1(i__) = rNULL__
if(ar__1(49:52) .EQ. '') VMAG0_1(i__) = rNULL__
c ..............Just test output...........
write(6,2)
+ HD_1(i__),n_HD_1(i__),E_b_y_1(i__),Teff1_1(i__),logg1_1(i__),
+ Teff2_1(i__),logg2_1(i__),v_M_H__1(i__),VMAG1_1(i__),
+ VMAG0_1(i__),Note_1(i__),Rem_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table3.dat' ! Visual magnitude for the 10 SB2 or close VB
* gamma Dor stars
C Format for file interpretation
3 format(I6,3X,F4.2,2X,F4.2,2X,F5.2,1X,A1)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,10
read(1,'(A28)')ar__2
read(ar__2,3)HD_2(i__),Vmag(i__),V_A(i__),V_B(i__),n_HD_2(i__)
if(ar__2(16:19) .EQ. '') V_A(i__) = rNULL__
if(ar__2(22:26) .EQ. '') V_B(i__) = rNULL__
c ..............Just test output...........
write(6,3)HD_2(i__),Vmag(i__),V_A(i__),V_B(i__),n_HD_2(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'notes.dat' ! Individual notes
C Format for file interpretation
4 format(I6,1X,A73)
C Effective file loading
open(unit=1,status='old',file=
+'notes.dat')
write(6,*) '....Loading file: notes.dat'
do i__=1,15
read(1,'(A80)')ar__3
read(ar__3,4)HD_3(i__),Note_2(i__)
c ..............Just test output...........
write(6,4)HD_3(i__),Note_2(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end