Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_A/543/A160 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-18
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/543/A160 Normalized spectra of 82 Kepler red giants (Thygesen+, 2012)
*================================================================================
*Atmospheric parameters of 82 red giants in the Kepler field.
* Thygesen A.O., Frandsen, S., Bruntt H., Kallinger T., Andersen M.F.,
* Elsworth Y.E., Hekker S., Karoff C., Stello D., Brogaard K., Burke C.,
* Caldwell D.A., Christiansen J.L.
* <Astron. Astrophys. 543, A160 (2012)>
* =2012A&A...543A.160T
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'stars.dat' ! List of studied giants
integer*4 nr__
parameter (nr__=92) ! Number of records
character*51 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*12 Name (nr__) ! Star name
integer*4 RAh (nr__) ! (h) Right ascension (J2000)
integer*4 RAm (nr__) ! (min) Right ascension (J2000)
real*4 RAs (nr__) ! (s) Right ascension (J2000)
character*1 DE_ (nr__) ! Declination sign (J2000)
integer*4 DEd (nr__) ! (deg) Declination (J2000)
integer*4 DEm (nr__) ! (arcmin) Declination (J2000)
real*4 DEs (nr__) ! (arcsec) Declination (J2000)
character*13 FileName (nr__) ! Name of the spectrum file in subdirectory sp
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'sp/*' ! Individual spectra
integer*4 nr__1
parameter (nr__1=92) ! Number of records
character*23 ar__1 ! Full-size record
real*8 lambda (nr__1) ! (0.1nm) [3999/8850] Wavelength vector
real*8 nFlux (nr__1) ! Normalized flux
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'tablea1.dat' ! Fundamental atmospheric parameters for all red
giants in our sample
integer*4 nr__2
parameter (nr__2=82) ! Number of records
character*94 ar__2 ! Full-size record
integer*4 KIC (nr__2) ! KIC (Cat. V/133) identification
integer*4 Teff1 (nr__2) ! (K) Effective temperature with VWA (+/-80K) (1)
real*4 logg1 (nr__2) ! ([cm/s2]) Surface gravity with VWA (+/-0.2dex) (1)
real*4 xi1 (nr__2) ! (km/s) Microturbulent velocity with VWA (+/-0.15km/s) (1)
real*4 v_Fe_H_1 (nr__2) ! ([Sun]) Metallicity from FeI and FeII (+/-0.15dex) (1)
integer*4 Teff2 (nr__2) ! (K) ?=- Effective temperature with Kepler
* asteroseismic analysis (+/-100K)
real*4 logg2 (nr__2) ! ([cm/s2]) ?=- Surface gravity with Kepler
* asteroseismic analysis (+/-0.1dex)
integer*4 Teff3 (nr__2) ! (K) ?=- Effective temperature with KIC (V/133)
real*4 logg3 (nr__2) ! ([cm/s2]) ?=- Surface gravity with KIC (V/133)
real*4 v_Fe_H_3 (nr__2) ! ([Sun]) ?=- Metallicity with KIC (V/133)
integer*4 Teff (nr__2) ! (K) ?=- VWA + Kepler effective temperature (2)
real*4 v_Fe_H_ (nr__2) ! ([Sun]) ?=- VWA + Kepler metallicity, FeII is used
* as the measure of [Fe/H] (2)
real*4 xi (nr__2) ! (km/s) ?=- VWA + Kepler microturbulent velocity {xi} (2)
real*4 vsini (nr__2) ! (km/s) Projected rotational velocity (+/-1.0km/s)
real*4 vmacro (nr__2) ! (km/s) Macroturbulent velocity (+/-1.0km/s)
real*4 RV (nr__2) ! (km/s) Radial velocity (+/-0.15km/s)
character*3 Type (nr__2) ! Giant type: RGB = red giant branch,
* RC = red clump, SC = secondary clump
*Note (1): VWA software poackage (see Bruntt et al. 2004A&A...425..683B,
* 2008A&A...478..487B, 2010A&A...519A..51B), from spectroscopy.
*Note (2): values are determined with VWA by fixing the gravity from the
* asteroseismic Kepler value.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'tablea2.dat' ! Elemental abundances for all targets where an
asteroseismic logg could be determined
integer*4 nr__3
parameter (nr__3=82) ! Number of records
character*109 ar__3 ! Full-size record
integer*4 KIC_1 (nr__3) ! KIC (Cat. V/133) identification
character*1 R (nr__3) ! [*] (KIC 9574235): abundances based on
* the spectroscopic (VWA) logg
real*4 v_C_H_ (nr__3) ! ([Sun]) ?=- [C/H] abundance (+/-0.5dex)
real*4 v_O_H_ (nr__3) ! ([Sun]) ?=- [O/H] abundance (+/-0.5dex)
real*4 v_Si_H_ (nr__3) ! ([Sun]) ?=- [Si/H] abundance (+/-0.2dex)
real*4 v_Ca_H_ (nr__3) ! ([Sun]) ?=- [Ca/H] abundance (+/-0.2dex)
real*4 v_Sc_H_ (nr__3) ! ([Sun]) ?=- [Sc/H] abundance (+/-0.2dex)
real*4 v_TiI_H_ (nr__3) ! ([Sun]) ?=- [TiI/H] abundance (+/-0.2dex)
real*4 v_TiII_H_ (nr__3) ! ([Sun]) ?=- [TiII/H] abundance (+/-0.2dex)
real*4 v_V_H_ (nr__3) ! ([Sun]) ?=- [V/H] abundance (+/-0.2dex)
real*4 v_CrI_H_ (nr__3) ! ([Sun]) ?=- [CrI/H] abundance (+/-0.2dex)
real*4 v_CrII_H_ (nr__3) ! ([Sun]) ?=- [CrII/H] abundance (+/-0.2dex)
real*4 v_Mn_H_ (nr__3) ! ([Sun]) ?=- [Mn/H] abundance (+/-0.2dex)
real*4 v_FeI_H_ (nr__3) ! ([Sun]) ?=- [FeI/H] abundance (+/-0.15dex)
real*4 v_FeII_H_ (nr__3) ! ([Sun]) ?=- [FeII/H] abundance (+/-0.15dex)
real*4 v_Co_H_ (nr__3) ! ([Sun]) ?=- [Co/H] abundance (+/-0.2dex)
real*4 v_Ni_H_ (nr__3) ! ([Sun]) ?=- [Ni/H] abundance (+/-0.2dex)
real*4 v_Y_H_ (nr__3) ! ([Sun]) ?=- [Y/H] abundance (+/-0.2dex)
C=============================================================================
C Loading file 'stars.dat' ! List of studied giants
C Format for file interpretation
1 format(A12,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F5.2,1X,A13)
C Effective file loading
open(unit=1,status='old',file=
+'stars.dat')
write(6,*) '....Loading file: stars.dat'
do i__=1,92
read(1,'(A51)')ar__
read(ar__,1)
+ Name(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),FileName(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)
+ Name(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),FileName(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 'sp/*' ! Individual spectra
C Format for file interpretation
2 format(1X,F10.5,2X,F10.8)
C Effective file loading
open(unit=1,status='old',file=
+'sp/*')
write(6,*) '....Loading file: sp/*'
do i__=1,92
read(1,'(A23)')ar__1
read(ar__1,2)lambda(i__),nFlux(i__)
c ..............Just test output...........
write(6,2)lambda(i__),nFlux(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'tablea1.dat' ! Fundamental atmospheric parameters for all red
* giants in our sample
C Format for file interpretation
3 format(
+ 4X,I8,1X,I4,1X,F4.2,1X,F4.2,1X,F5.2,1X,I4,1X,F4.2,1X,I4,1X,
+ F4.2,1X,F5.2,1X,I4,1X,F5.2,1X,F4.2,1X,F3.1,1X,F3.1,1X,F6.1,1X,
+ A3)
C Effective file loading
open(unit=1,status='old',file=
+'tablea1.dat')
write(6,*) '....Loading file: tablea1.dat'
do i__=1,82
read(1,'(A94)')ar__2
read(ar__2,3)
+ KIC(i__),Teff1(i__),logg1(i__),xi1(i__),v_Fe_H_1(i__),
+ Teff2(i__),logg2(i__),Teff3(i__),logg3(i__),v_Fe_H_3(i__),
+ Teff(i__),v_Fe_H_(i__),xi(i__),vsini(i__),vmacro(i__),RV(i__),
+ Type(i__)
if (Teff2(i__) .EQ. 45) Teff2(i__) = iNULL__
if (idig(ar__2(40:43)).EQ.0) logg2(i__) = rNULL__
if (Teff3(i__) .EQ. 45) Teff3(i__) = iNULL__
if (idig(ar__2(50:53)).EQ.0) logg3(i__) = rNULL__
if (idig(ar__2(55:59)).EQ.0) v_Fe_H_3(i__) = rNULL__
if (Teff(i__) .EQ. 45) Teff(i__) = iNULL__
if (idig(ar__2(66:70)).EQ.0) v_Fe_H_(i__) = rNULL__
if (idig(ar__2(72:75)).EQ.0) xi(i__) = rNULL__
c ..............Just test output...........
write(6,3)
+ KIC(i__),Teff1(i__),logg1(i__),xi1(i__),v_Fe_H_1(i__),
+ Teff2(i__),logg2(i__),Teff3(i__),logg3(i__),v_Fe_H_3(i__),
+ Teff(i__),v_Fe_H_(i__),xi(i__),vsini(i__),vmacro(i__),RV(i__),
+ Type(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'tablea2.dat' ! Elemental abundances for all targets where an
* asteroseismic logg could be determined
C Format for file interpretation
4 format(
+ 4X,I8,A1,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,
+ F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,
+ 1X,F5.2,1X,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'tablea2.dat')
write(6,*) '....Loading file: tablea2.dat'
do i__=1,82
read(1,'(A109)')ar__3
read(ar__3,4)
+ KIC_1(i__),R(i__),v_C_H_(i__),v_O_H_(i__),v_Si_H_(i__),
+ v_Ca_H_(i__),v_Sc_H_(i__),v_TiI_H_(i__),v_TiII_H_(i__),
+ v_V_H_(i__),v_CrI_H_(i__),v_CrII_H_(i__),v_Mn_H_(i__),
+ v_FeI_H_(i__),v_FeII_H_(i__),v_Co_H_(i__),v_Ni_H_(i__),
+ v_Y_H_(i__)
if (idig(ar__3(15:19)).EQ.0) v_C_H_(i__) = rNULL__
if (idig(ar__3(21:25)).EQ.0) v_O_H_(i__) = rNULL__
if (idig(ar__3(27:31)).EQ.0) v_Si_H_(i__) = rNULL__
if (idig(ar__3(33:37)).EQ.0) v_Ca_H_(i__) = rNULL__
if (idig(ar__3(39:43)).EQ.0) v_Sc_H_(i__) = rNULL__
if (idig(ar__3(45:49)).EQ.0) v_TiI_H_(i__) = rNULL__
if (idig(ar__3(51:55)).EQ.0) v_TiII_H_(i__) = rNULL__
if (idig(ar__3(57:61)).EQ.0) v_V_H_(i__) = rNULL__
if (idig(ar__3(63:67)).EQ.0) v_CrI_H_(i__) = rNULL__
if (idig(ar__3(69:73)).EQ.0) v_CrII_H_(i__) = rNULL__
if (idig(ar__3(75:79)).EQ.0) v_Mn_H_(i__) = rNULL__
if (idig(ar__3(81:85)).EQ.0) v_FeI_H_(i__) = rNULL__
if (idig(ar__3(87:91)).EQ.0) v_FeII_H_(i__) = rNULL__
if (idig(ar__3(93:97)).EQ.0) v_Co_H_(i__) = rNULL__
if (idig(ar__3(99:103)).EQ.0) v_Ni_H_(i__) = rNULL__
if (idig(ar__3(105:109)).EQ.0) v_Y_H_(i__) = rNULL__
c ..............Just test output...........
write(6,4)
+ KIC_1(i__),R(i__),v_C_H_(i__),v_O_H_(i__),v_Si_H_(i__),
+ v_Ca_H_(i__),v_Sc_H_(i__),v_TiI_H_(i__),v_TiII_H_(i__),
+ v_V_H_(i__),v_CrI_H_(i__),v_CrII_H_(i__),v_Mn_H_(i__),
+ v_FeI_H_(i__),v_FeII_H_(i__),v_Co_H_(i__),v_Ni_H_(i__),
+ v_Y_H_(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end
C Locate position of first digit in string; or return 0
integer function idig(c)
character*(*) c
character*1 c1
integer lc,i
lc=len(c)
idig=0
do i=1,lc
if(c(i:i).ne.' ') go to 1
end do
1 if(i.gt.lc) return
c1=c(i:i)
if(c1.eq.'.'.or.c1.eq.'-'.or.c1.eq.'+') i=i+1
if(i.gt.lc) return
c1=c(i:i)
if(c1.ge.'0'.and.c1.le.'9') idig=i
return
end