Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_A/538/A100 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-Mar-28 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/538/A100 Abundances red giants in Carina dSph (Lemasle+, 2012) *================================================================================ *VLT/FLAMES spectroscopy of red giant branch stars in the Carina dwarf *spheroidal galaxy. * Lemasle B., Hill V., Tolstoy E., Venn K.A., Shetrone M.D., Irwin M.J., * de Boer T.J.L., Starkenburg E., Salvadori S. * <Astron. Astrophys. 538, A100 (2012)> * =2012A&A...538A.100L C============================================================================= C Internal variables integer*4 i__ c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table3.dat' ! Photometric information for our FLAMES targets integer*4 nr__ parameter (nr__=98) ! Number of records character*88 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*7 Name ! Name MKVNNNN integer*4 RAh ! (h) Right ascension (J2000) integer*4 RAm ! (min) Right ascension (J2000) real*4 RAs ! (s) Right ascension (J2000) character*1 DE_ ! Declination sign (J2000) integer*4 DEd ! (deg) Declination (J2000) integer*4 DEm ! (arcmin) Declination (J2000) real*4 DEs ! (arcsec) Declination (J2000) real*4 Vmag ! (mag) ESO-WFI V magnitude real*4 Imag ! (mag) ESO-WFI I magnitude real*4 Jmag ! (mag) ? ESO-SOFI J magnitude (1) real*4 Hmag ! (mag) ? ESO-SOFI H magnitude (1) real*4 Kmag ! (mag) ? ESO-SOFI K magnitude (1) real*4 HRV ! (km/s) Heliocentric radial velocity (2) real*4 e_HRV ! (km/s) rms uncertainty on HRV (2) character*10 Memb ! Membership *Note (1): From M. Gullieuszik (private communication) *Note (2): our measured radial velocities c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table4.dat' ! List of all spectral lines, their atomic parameters and their measured EWs for all the 35 RGB stars in the Carina dSph integer*4 nr__1 parameter (nr__1=3360) ! Number of records character*36 ar__1 ! Full-size record character*7 Name_1 ! Star name real*8 lambda ! (0.1nm) Wavelength character*3 El ! Element real*4 ExPot ! (eV) Excitation potential real*4 loggf ! ([-]) Oscillator strength integer*4 EW ! (0.1pm) ?=- Equivalent width c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table7.dat' ! The abundances and errors of iron and {alpha}-elements in our sample of RGB stars in the Carina dSph integer*4 nr__2 parameter (nr__2=35) ! Number of records character*86 ar__2 ! Full-size record character*7 Name_2 ! Star name real*4 v_Fe1_H_ ! ([-]) Abundance [FeI/H] real*4 e__Fe1_H_ ! ([-]) rms uncertainty on [FeI/H] integer*4 o__Fe1_H_ ! Number of line used for [FeI/H] real*4 v_Fe2_H_ ! ([-]) ?=- Abundance [FeII/H] real*4 e__Fe2_H_ ! ([-]) ?=- rms uncertainty on [FeII/H] integer*4 o__Fe2_H_ ! ?=- Number of line used for [FeII/H] real*4 v_Mg1_H_ ! ([-]) ?=- Abundance [MgI/H] real*4 e__Mg1_H_ ! ([-]) ?=- rms uncertainty on [MgI/H] integer*4 o__Mg1_H_ ! ?=- Number of line used for [MgI/H] real*4 v_Ca1_H_ ! ([-]) ?=- Abundance [CaI/H] real*4 e__Ca1_H_ ! ([-]) ?=- rms uncertainty on [CaI/H] integer*4 o__Ca1_H_ ! ?=- Number of line used for [CaI/H] real*4 v_Ti1_H_ ! ([-]) ?=- Abundance [TiI/H] real*4 e__Ti1_H_ ! ([-]) ?=- rms uncertainty on [TiI/H] integer*4 o__Ti1_H_ ! ?=- Number of line used for [TiI/H] real*4 v_Ti2_H_ ! ([-]) ?=- Abundance [TiII/H] real*4 e__Ti2_H_ ! ([-]) ?=- rms uncertainty on [TiII/H] integer*4 o__Ti2_H_ ! ?=- Number of line used for [TiII/H] c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table8.dat' ! The abundances and errors of iron-peak and heavy elements in our sample of RGB stars in the Carina dSph integer*4 nr__3 parameter (nr__3=35) ! Number of records character*73 ar__3 ! Full-size record character*7 Name_3 ! Star name real*4 v_Fe1_H__1 ! ([-]) Abundance [FeI/H] real*4 e__Fe1_H__1 ! ([-]) rms uncertainty on [FeI/H] integer*4 o__Fe1_H__1 ! Number of line used for [FeI/H] real*4 v_Cr1_H_ ! ([-]) ?=- Abundance [CrI/H] real*4 e__Cr1_H_ ! ([-]) ?=- rms uncertainty on [CrI/H] integer*4 o__Cr1_H_ ! ?=- Number of line used for [CrI/H] real*4 v_Co1_H_ ! ([-]) ?=- Abundance [CoI/H] real*4 e__Co1_H_ ! ([-]) ?=- rms uncertainty on [CoI/H] integer*4 o__Co1_H_ ! ?=- Number of line used for [CoI/H] real*4 v_Ni1_H_ ! ([-]) ?=- Abundance [NiI/H] real*4 e__Ni1_H_ ! ([-]) ?=- rms uncertainty on [NiI/H] integer*4 o__Ni1_H_ ! ?=- Number of line used for [NiI/H] real*4 v_Ba2_H_ ! ([-]) ?=- Abundance [BaII/H] real*4 e__Ba2_H_ ! ([-]) ?=- rms uncertainty on [BaII/H] integer*4 o__Ba2_H_ ! ?=- Number of line used for [BaII/H] c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table9.dat' ! The abundances and errors for elements that could be measured from single lines in only a handful of stars integer*4 nr__4 parameter (nr__4=8) ! Number of records character*98 ar__4 ! Full-size record character*7 Name_4 ! Star name real*4 v_Na1_H_ ! ([-]) ?=- Abundance [NaI/H] real*4 e__Na1_H_ ! ([-]) ?=- rms uncertainty on [NaI/H] integer*4 o__Na1_H_ ! ?=- Number of line used for [NaI/H] real*4 v_Si1_H_ ! ([-]) ?=- Abundance [SiI/H] real*4 e__Si1_H_ ! ([-]) ?=- rms uncertainty on [SiI/H] integer*4 o__Si1_H_ ! ?=- Number of line used for [SiI/H] real*4 v_Sc2_H_ ! ([-]) ?=- Abundance [ScII/H] real*4 e__Sc2_H_ ! ([-]) ?=- rms uncertainty on [ScII/H] integer*4 o__Sc2_H_ ! ?=- Number of line used for [ScII/H] real*4 v_Y2_H_ ! ([-]) ?=- Abundance [YII/H] real*4 e__Y2_H_ ! ([-]) ?=- rms uncertainty on [YII/H] integer*4 o__Y2_H_ ! ?=- Number of line used for [YII/H] real*4 v_La2_H_ ! ([-]) ?=- Abundance [LaII/H] real*4 e__La2_H_ ! ([-]) ?=- rms uncertainty on [LaII/H] integer*4 o__La2_H_ ! ?=- Number of line used for [LaII/H] real*4 v_Nd2_H_ ! ([-]) ?=- Abundance [NdII/H] real*4 e__Nd2_H_ ! ([-]) ?=- rms uncertainty on [NdII/H] integer*4 o__Nd2_H_ ! ?=- Number of line used for [NdII/H] real*4 v_Eu2_H_ ! ([-]) ?=- Abundance [EuII/H] real*4 e__Eu2_H_ ! ([-]) ?=- rms uncertainty on [EuII/H] integer*4 o__Eu2_H_ ! ?=- Number of line used for [EuII/H] C============================================================================= C Loading file 'table3.dat' ! Photometric information for our FLAMES targets C Format for file interpretation 1 format( + A7,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F5.2,1X,F6.3,1X,F6.3, + 1X,F6.3,1X,F6.3,1X,F6.3,1X,F5.1,1X,F3.1,1X,A10) C Effective file loading open(unit=1,status='old',file= +'table3.dat') write(6,*) '....Loading file: table3.dat' do i__=1,98 read(1,'(A88)')ar__ read(ar__,1) + Name,RAh,RAm,RAs,DE_,DEd,DEm,DEs,Vmag,Imag,Jmag,Hmag,Kmag,HRV, + e_HRV,Memb if(ar__(48:53) .EQ. '') Jmag = rNULL__ if(ar__(55:60) .EQ. '') Hmag = rNULL__ if(ar__(62:67) .EQ. '') Kmag = rNULL__ 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) + Name,RAh,RAm,RAs,DE_,DEd,DEm,DEs,Vmag,Imag,Jmag,Hmag,Kmag,HRV, + e_HRV,Memb write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg c .......End.of.Just test output........... end do close(1) C============================================================================= C Loading file 'table4.dat' ! List of all spectral lines, their atomic * parameters and their measured EWs for all the * 35 RGB stars in the Carina dSph C Format for file interpretation 2 format(A7,1X,F7.2,1X,A3,1X,F5.3,1X,F6.3,1X,I3) C Effective file loading open(unit=1,status='old',file= +'table4.dat') write(6,*) '....Loading file: table4.dat' do i__=1,3360 read(1,'(A36)')ar__1 read(ar__1,2)Name_1,lambda,El,ExPot,loggf,EW if (EW .EQ. 45) EW = iNULL__ c ..............Just test output........... write(6,2)Name_1,lambda,El,ExPot,loggf,EW c .......End.of.Just test output........... end do close(1) C============================================================================= C Loading file 'table7.dat' ! The abundances and errors of iron and * {alpha}-elements in our sample of RGB stars * in the Carina dSph C Format for file interpretation 3 format( + A7,1X,F5.2,1X,F4.2,1X,I2,1X,F5.2,1X,F4.2,1X,I1,1X,F5.2,1X, + F4.2,1X,I1,1X,F5.2,1X,F4.2,1X,I1,1X,F5.2,1X,F4.2,1X,I1,1X, + F5.2,1X,F4.2,1X,I1) C Effective file loading open(unit=1,status='old',file= +'table7.dat') write(6,*) '....Loading file: table7.dat' do i__=1,35 read(1,'(A86)')ar__2 read(ar__2,3) + Name_2,v_Fe1_H_,e__Fe1_H_,o__Fe1_H_,v_Fe2_H_,e__Fe2_H_, + o__Fe2_H_,v_Mg1_H_,e__Mg1_H_,o__Mg1_H_,v_Ca1_H_,e__Ca1_H_, + o__Ca1_H_,v_Ti1_H_,e__Ti1_H_,o__Ti1_H_,v_Ti2_H_,e__Ti2_H_, + o__Ti2_H_ if (idig(ar__2(23:27)).EQ.0) v_Fe2_H_ = rNULL__ if (idig(ar__2(29:32)).EQ.0) e__Fe2_H_ = rNULL__ if (o__Fe2_H_ .EQ. 45) o__Fe2_H_ = iNULL__ if (idig(ar__2(36:40)).EQ.0) v_Mg1_H_ = rNULL__ if (idig(ar__2(42:45)).EQ.0) e__Mg1_H_ = rNULL__ if (o__Mg1_H_ .EQ. 45) o__Mg1_H_ = iNULL__ if (idig(ar__2(49:53)).EQ.0) v_Ca1_H_ = rNULL__ if (idig(ar__2(55:58)).EQ.0) e__Ca1_H_ = rNULL__ if (o__Ca1_H_ .EQ. 45) o__Ca1_H_ = iNULL__ if (idig(ar__2(62:66)).EQ.0) v_Ti1_H_ = rNULL__ if (idig(ar__2(68:71)).EQ.0) e__Ti1_H_ = rNULL__ if (o__Ti1_H_ .EQ. 45) o__Ti1_H_ = iNULL__ if (idig(ar__2(75:79)).EQ.0) v_Ti2_H_ = rNULL__ if (idig(ar__2(81:84)).EQ.0) e__Ti2_H_ = rNULL__ if (o__Ti2_H_ .EQ. 45) o__Ti2_H_ = iNULL__ c ..............Just test output........... write(6,3) + Name_2,v_Fe1_H_,e__Fe1_H_,o__Fe1_H_,v_Fe2_H_,e__Fe2_H_, + o__Fe2_H_,v_Mg1_H_,e__Mg1_H_,o__Mg1_H_,v_Ca1_H_,e__Ca1_H_, + o__Ca1_H_,v_Ti1_H_,e__Ti1_H_,o__Ti1_H_,v_Ti2_H_,e__Ti2_H_, + o__Ti2_H_ c .......End.of.Just test output........... end do close(1) C============================================================================= C Loading file 'table8.dat' ! The abundances and errors of iron-peak and * heavy elements in our sample of RGB stars * in the Carina dSph C Format for file interpretation 4 format( + A7,1X,F5.2,1X,F4.2,1X,I2,1X,F5.2,1X,F4.2,1X,I1,1X,F5.2,1X, + F4.2,1X,I1,1X,F5.2,1X,F4.2,1X,I1,1X,F5.2,1X,F4.2,1X,I1) C Effective file loading open(unit=1,status='old',file= +'table8.dat') write(6,*) '....Loading file: table8.dat' do i__=1,35 read(1,'(A73)')ar__3 read(ar__3,4) + Name_3,v_Fe1_H__1,e__Fe1_H__1,o__Fe1_H__1,v_Cr1_H_,e__Cr1_H_, + o__Cr1_H_,v_Co1_H_,e__Co1_H_,o__Co1_H_,v_Ni1_H_,e__Ni1_H_, + o__Ni1_H_,v_Ba2_H_,e__Ba2_H_,o__Ba2_H_ if (idig(ar__3(23:27)).EQ.0) v_Cr1_H_ = rNULL__ if (idig(ar__3(29:32)).EQ.0) e__Cr1_H_ = rNULL__ if (o__Cr1_H_ .EQ. 45) o__Cr1_H_ = iNULL__ if (idig(ar__3(36:40)).EQ.0) v_Co1_H_ = rNULL__ if (idig(ar__3(42:45)).EQ.0) e__Co1_H_ = rNULL__ if (o__Co1_H_ .EQ. 45) o__Co1_H_ = iNULL__ if (idig(ar__3(49:53)).EQ.0) v_Ni1_H_ = rNULL__ if (idig(ar__3(55:58)).EQ.0) e__Ni1_H_ = rNULL__ if (o__Ni1_H_ .EQ. 45) o__Ni1_H_ = iNULL__ if (idig(ar__3(62:66)).EQ.0) v_Ba2_H_ = rNULL__ if (idig(ar__3(68:71)).EQ.0) e__Ba2_H_ = rNULL__ if (o__Ba2_H_ .EQ. 45) o__Ba2_H_ = iNULL__ c ..............Just test output........... write(6,4) + Name_3,v_Fe1_H__1,e__Fe1_H__1,o__Fe1_H__1,v_Cr1_H_,e__Cr1_H_, + o__Cr1_H_,v_Co1_H_,e__Co1_H_,o__Co1_H_,v_Ni1_H_,e__Ni1_H_, + o__Ni1_H_,v_Ba2_H_,e__Ba2_H_,o__Ba2_H_ c .......End.of.Just test output........... end do close(1) C============================================================================= C Loading file 'table9.dat' ! The abundances and errors for elements that * could be measured from single lines in only * a handful of stars C Format for file interpretation 5 format( + A7,1X,F5.2,1X,F4.2,1X,I1,1X,F5.2,1X,F4.2,1X,I1,1X,F5.2,1X, + F4.2,1X,I1,1X,F5.2,1X,F4.2,1X,I1,1X,F5.2,1X,F4.2,1X,I1,1X, + F5.2,1X,F4.2,1X,I1,1X,F5.2,1X,F4.2,1X,I1) C Effective file loading open(unit=1,status='old',file= +'table9.dat') write(6,*) '....Loading file: table9.dat' do i__=1,8 read(1,'(A98)')ar__4 read(ar__4,5) + Name_4,v_Na1_H_,e__Na1_H_,o__Na1_H_,v_Si1_H_,e__Si1_H_, + o__Si1_H_,v_Sc2_H_,e__Sc2_H_,o__Sc2_H_,v_Y2_H_,e__Y2_H_, + o__Y2_H_,v_La2_H_,e__La2_H_,o__La2_H_,v_Nd2_H_,e__Nd2_H_, + o__Nd2_H_,v_Eu2_H_,e__Eu2_H_,o__Eu2_H_ if (idig(ar__4(9:13)).EQ.0) v_Na1_H_ = rNULL__ if (idig(ar__4(15:18)).EQ.0) e__Na1_H_ = rNULL__ if (o__Na1_H_ .EQ. 45) o__Na1_H_ = iNULL__ if (idig(ar__4(22:26)).EQ.0) v_Si1_H_ = rNULL__ if (idig(ar__4(28:31)).EQ.0) e__Si1_H_ = rNULL__ if (o__Si1_H_ .EQ. 45) o__Si1_H_ = iNULL__ if (idig(ar__4(35:39)).EQ.0) v_Sc2_H_ = rNULL__ if (idig(ar__4(41:44)).EQ.0) e__Sc2_H_ = rNULL__ if (o__Sc2_H_ .EQ. 45) o__Sc2_H_ = iNULL__ if (idig(ar__4(48:52)).EQ.0) v_Y2_H_ = rNULL__ if (idig(ar__4(54:57)).EQ.0) e__Y2_H_ = rNULL__ if (o__Y2_H_ .EQ. 45) o__Y2_H_ = iNULL__ if (idig(ar__4(61:65)).EQ.0) v_La2_H_ = rNULL__ if (idig(ar__4(67:70)).EQ.0) e__La2_H_ = rNULL__ if (o__La2_H_ .EQ. 45) o__La2_H_ = iNULL__ if (idig(ar__4(74:78)).EQ.0) v_Nd2_H_ = rNULL__ if (idig(ar__4(80:83)).EQ.0) e__Nd2_H_ = rNULL__ if (o__Nd2_H_ .EQ. 45) o__Nd2_H_ = iNULL__ if (idig(ar__4(87:91)).EQ.0) v_Eu2_H_ = rNULL__ if (idig(ar__4(93:96)).EQ.0) e__Eu2_H_ = rNULL__ if (o__Eu2_H_ .EQ. 45) o__Eu2_H_ = iNULL__ c ..............Just test output........... write(6,5) + Name_4,v_Na1_H_,e__Na1_H_,o__Na1_H_,v_Si1_H_,e__Si1_H_, + o__Si1_H_,v_Sc2_H_,e__Sc2_H_,o__Sc2_H_,v_Y2_H_,e__Y2_H_, + o__Y2_H_,v_La2_H_,e__La2_H_,o__La2_H_,v_Nd2_H_,e__Nd2_H_, + o__Nd2_H_,v_Eu2_H_,e__Eu2_H_,o__Eu2_H_ 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