Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_A/447/685 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-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/447/685 Elemental abundance analyses. XXIX. (Adelman+, 2006) *================================================================================ *Elemental abundance analyses with DAO spectrograms *XXIX. The Mercury-Manganese stars 53 Tau, beta Tau, gamma Crv, and upsilon Her. * Adelman S.J., Caliskan H., Gulliver A.F., Teker A. * <Astron. Astrophys. 447, 685 (2006)> * =2006A&A...447..685A C============================================================================= C Internal variables integer*4 i__ c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table4.dat' ! He/H determinations integer*4 nr__ parameter (nr__=26) ! Number of records character*20 ar__ ! Full-size record character*9 Name (nr__) ! Star name integer*4 lambda (nr__) ! (0.1nm) Wavelength real*4 He_H (nr__) ! He/H abundace value (1) *Note (1): Average values: * 53 Tau : He/H = 0.042+/-0.008 * beta Tau : He/H = 0.070+/-0.010 * gamma Crv : He/H = 0.067+/-0.010 c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'tab567.dat' ! Abundances for {beta} Tau, {gamma} Crv, 53 Tau and from newly measured lines of {upsilon} Her integer*4 nr__1 parameter (nr__1=667) ! Number of records character*54 ar__1 ! Full-size record character*9 Name_1 (nr__1) ! Star name character*6 Ion (nr__1) ! Ion character*5 Mult (nr__1) ! Multiplet number (1) real*8 lambda_1 (nr__1) ! (0.1nm) Laboratory wavelength real*4 log_gf (nr__1) ! log gf value character*2 r_log_gf (nr__1) ! Reference for log(gf) (2) integer*4 EWlambda (nr__1) ! (0.1pm) ?=- Equivalent width real*4 log_Nel_Ntot(nr__1) ! ?=- Derived abundance *Note (1): Multiplet number from Moore 1945 if first line of multiplet; * if not from Moore an initial indicating the paper *Note (2): gf value references are as follows: * BG = Biemont et al. (1981ApJ...248..867B) * GB = Grevesse et al. (1981, Upper Main Sequence CP Stars, 23rd. * Liege Astrophys. Coll., 211) * DW = Dworetsky (1980A&A....84..350D) * FW = Fuhr & Wiese (1990, in Lide, D. R. ed, CRC Handbook of Chemistry * and Physics, CRC Press, Cleveland, OH) * HL = Hannaford et al. (1982ApJ...261..736H) * KX = Kurucz & Bell (1995, Kurucz CD-Rom No. 23) * LA = Lanz & Artru (1985PhyS...32..115L) * LD = Lawler & Dakin (1989, JOSA B, 6, 1457) * MF = Fuhr, Martin & Wiese, 1988, and Martin, Fuhr & Wiese, 1988, Cat. VI/72 * N4 = Fuhr & Wiese (2005, "A Critical Compilation of Atomic Transition * Probabilities for Neutral and Singly-Ionized Iron", * J. Phys. Chem. Ref. Data, in press) * SG = Schulz-Gulde (1969, JQSRT, 9, 13) * WF = Wiese, Fuhr & Deters (1996, Atomic transition probabilities of * carbon, nitrogen, and oxygen : a critical data compilation. * Edited by W.L. Wiese, J.R. Fuhr, and T.M. Deters. Washington, DC) * WM = Wiese & Martin (1980, NSRDS-NBS 68. Part 2, US Government * Printing Office, Washington, DC) * WS = Wiese, Smith & Glennon (1966, NSRDS-NBS 4, US Governement * Printing Office, Washington) and Wiese, Smith & Miles (1969, * NSRDS-NBS, D.C.: US Department of Commerce, National Bureau * of Standards) c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'abund.dat' ! Atomic abundances integer*4 nr__2 parameter (nr__2=73) ! Number of records character*32 ar__2 ! Full-size record character*9 Name_2 (nr__2) ! Star name character*6 Ion_1 (nr__2) ! Ion character*2 Element (nr__2) ! Element (identical to bytes 11-12) real*4 log_Nel_Ntot_1(nr__2) ! Derived abundance of element (1) real*4 e_log_Nel_Ntot(nr__2) ! ? rms uncertainty on (Nel/Ntot) *Note (1): Ratio of number of atoms to the total number of atoms per unit volume c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table8.dat' ! Comparison of Results (logN/H) for 53 Tau, {gamma} Crv, and {upsilon} Her last analysis with this paper integer*4 nr__3 parameter (nr__3=56) ! Number of records character*32 ar__3 ! Full-size record character*9 Name_3 (nr__3) ! Star name character*6 Ion_2 (nr__3) ! Ion real*4 log_Nel_H_old(nr__3) ! Previous relative abundance (1) real*4 log_Nel_H (nr__3) ! This Paper relative abundance *Note (1): Previous log(Nel/H) values are from * Paper II (Adelman, 1987MNRAS.228..573A) for 53 Tau, * Fremat & Houziaux ( 1997A&A...320..580F) for {gamma} Crv, * Paper XXIV (Adelman et al., 2001, Cat. <J/A+A/367/597> for {upsilon} Her C============================================================================= C Loading file 'table4.dat' ! He/H determinations C Format for file interpretation 1 format(A9,2X,I4,1X,F4.2) C Effective file loading open(unit=1,status='old',file= +'table4.dat') write(6,*) '....Loading file: table4.dat' do i__=1,26 read(1,'(A20)')ar__ read(ar__,1)Name(i__),lambda(i__),He_H(i__) c ..............Just test output........... write(6,1)Name(i__),lambda(i__),He_H(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= C Loading file 'tab567.dat' ! Abundances for {beta} Tau, {gamma} Crv, 53 Tau * and from newly measured lines of {upsilon} Her C Format for file interpretation 2 format(A9,1X,A6,2X,A5,1X,F7.2,2X,F5.2,2X,A2,2X,I3,2X,F5.2) C Effective file loading open(unit=1,status='old',file= +'tab567.dat') write(6,*) '....Loading file: tab567.dat' do i__=1,667 read(1,'(A54)')ar__1 read(ar__1,2) + Name_1(i__),Ion(i__),Mult(i__),lambda_1(i__),log_gf(i__), + r_log_gf(i__),EWlambda(i__),log_Nel_Ntot(i__) if (EWlambda(i__) .EQ. 45) EWlambda(i__) = iNULL__ if (idig(ar__1(50:54)).EQ.0) log_Nel_Ntot(i__) = rNULL__ c ..............Just test output........... write(6,2) + Name_1(i__),Ion(i__),Mult(i__),lambda_1(i__),log_gf(i__), + r_log_gf(i__),EWlambda(i__),log_Nel_Ntot(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= C Loading file 'abund.dat' ! Atomic abundances C Format for file interpretation 3 format(A9,1X,A6,2X,A2,2X,F5.2,1X,F4.2) C Effective file loading open(unit=1,status='old',file= +'abund.dat') write(6,*) '....Loading file: abund.dat' do i__=1,73 read(1,'(A32)')ar__2 read(ar__2,3) + Name_2(i__),Ion_1(i__),Element(i__),log_Nel_Ntot_1(i__), + e_log_Nel_Ntot(i__) if(ar__2(29:32) .EQ. '') e_log_Nel_Ntot(i__) = rNULL__ c ..............Just test output........... write(6,3) + Name_2(i__),Ion_1(i__),Element(i__),log_Nel_Ntot_1(i__), + e_log_Nel_Ntot(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= C Loading file 'table8.dat' ! Comparison of Results (logN/H) for 53 Tau, {gamma} * Crv, and {upsilon} Her last analysis with this paper C Format for file interpretation 4 format(A9,2X,A6,3X,F5.2,2X,F5.2) C Effective file loading open(unit=1,status='old',file= +'table8.dat') write(6,*) '....Loading file: table8.dat' do i__=1,56 read(1,'(A32)')ar__3 read(ar__3,4) + Name_3(i__),Ion_2(i__),log_Nel_H_old(i__),log_Nel_H(i__) c ..............Just test output........... write(6,4) + Name_3(i__),Ion_2(i__),log_Nel_H_old(i__),log_Nel_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