Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/705/32 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/ApJ/705/32 Diffuse interstellar bands from HD 183143 (Hobbs+, 2009) *================================================================================ *Studies of the diffuse interstellar bands. *III. HD 183143. * Hobbs L.M., York D.G., Thorburn J.A., Snow T.P., Bishof M., Friedman S.D., * McCall B.J., Oka T., Rachford B., Sonnentrucker P., Welty D.E. * <Astrophys. J., 705, 32-45 (2009)> * =2009ApJ...705...32H C============================================================================= C Internal variables integer*4 i__ c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table2.dat' ! Diffuse interstellar bands (DIBs) in the spectrum of HD 183143 integer*4 nr__ parameter (nr__=418) ! Number of records character*103 ar__ ! Full-size record real*8 JD94 (nr__) ! (0.1nm) ? Jenniskens & Desert (1994A&AS..106...39J) * central wavelength character*1 f_JD94 (nr__) ! [b] blend (see section 3.2 for details) real*8 GM00 (nr__) ! (0.1nm) ? Galazutdinov et al. (2000PASP..112..648G) * central wavelength real*8 TC00 (nr__) ! (0.1nm) ? Tuairisg et al. (2000A&AS..142..225T) central * wavelength character*1 f_TC00 (nr__) ! [b] blend (see section 3.2 for details) real*8 WS00 (nr__) ! (0.1nm) ? Weselak et al. (2000A&AS..142..239W) central * wavelength character*1 f_WS00 (nr__) ! [b] blend (see section 3.2 for details) real*8 Wc (nr__) ! (0.1nm) Band central wavelength in Angstroms real*4 FWHM (nr__) ! (0.1nm) ? Band Full-Width at Half-Maximum character*1 l_EW (nr__) ! Limit flag on EW real*4 EW (nr__) ! (10-13m) ? Band equivalent width in milli-Angstroms character*1 f_EW (nr__) ! [p] p: present real*4 e_EW (nr__) ! (10-13m) ? Uncertainty in EW character*5 n_EW (nr__) ! Warning note on EW (1) real*8 RWc (nr__) ! (0.1nm) Band central wavelength in stellar rest frame character*1 l_BWc (nr__) ! Limit flag on BWc (2) real*8 BWc (nr__) ! (0.1nm) ? {beta} Ori central wavelength character*1 f_BWc (nr__) ! [P] Indicates BWc shows a P Cygni profile real*4 BEW (nr__) ! (10-13m) ? {beta} Ori equivalent width in milli-Angstroms character*1 f_BEW (nr__) ! [b] blend (3) integer*4 Seq (nr__) ! ? Running index number (only for table 2) *Note (1): Note as follows: * d = blend with another DIB (diffuse interstellar band); * s = blend with stellar line; * t = blend with telluric line; * det = detector artifact; * s1 = blend with stellar NI; * s2 = blend with stellar NII. *Note (2): Indicates more than one (isolated) stellar line interfers, * typically for a broad DIB (diffuse interstellar band). The * corresponding sum of the equivalent widths is given in BEW. *Note (3): * b = the stellar line measured is itself a blend of at least two lines. c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table3.dat' ! 71 possible diffuse interstellar bands in the spectrum of HD 183143 integer*4 nr__1 parameter (nr__1=71) ! Number of records character*103 ar__1 ! Full-size record real*8 JD94_1 (nr__1) ! (0.1nm) ? Jenniskens & Desert (1994A&AS..106...39J) * central wavelength character*1 f_JD94_1 (nr__1) ! [b] blend (see section 3.2 for details) real*8 GM00_1 (nr__1) ! (0.1nm) ? Galazutdinov et al. (2000PASP..112..648G) * central wavelength real*8 TC00_1 (nr__1) ! (0.1nm) ? Tuairisg et al. (2000A&AS..142..225T) central * wavelength character*1 f_TC00_1 (nr__1) ! [b] blend (see section 3.2 for details) real*8 WS00_1 (nr__1) ! (0.1nm) ? Weselak et al. (2000A&AS..142..239W) central * wavelength character*1 f_WS00_1 (nr__1) ! [b] blend (see section 3.2 for details) real*8 Wc_1 (nr__1) ! (0.1nm) Band central wavelength in Angstroms real*4 FWHM_1 (nr__1) ! (0.1nm) ? Band Full-Width at Half-Maximum character*1 l_EW_1 (nr__1) ! Limit flag on EW real*4 EW_1 (nr__1) ! (10-13m) ? Band equivalent width in milli-Angstroms character*1 f_EW_1 (nr__1) ! [p] p: present real*4 e_EW_1 (nr__1) ! (10-13m) ? Uncertainty in EW character*5 n_EW_1 (nr__1) ! Warning note on EW (1) real*8 RWc_1 (nr__1) ! (0.1nm) Band central wavelength in stellar rest frame character*1 l_BWc_1 (nr__1) ! Limit flag on BWc (2) real*8 BWc_1 (nr__1) ! (0.1nm) ? {beta} Ori central wavelength character*1 f_BWc_1 (nr__1) ! [P] Indicates BWc shows a P Cygni profile real*4 BEW_1 (nr__1) ! (10-13m) ? {beta} Ori equivalent width in milli-Angstroms character*1 f_BEW_1 (nr__1) ! [b] blend (3) integer*4 Seq_1 (nr__1) ! ? Running index number (only for table 2) *Note (1): Note as follows: * d = blend with another DIB (diffuse interstellar band); * s = blend with stellar line; * t = blend with telluric line; * det = detector artifact; * s1 = blend with stellar NI; * s2 = blend with stellar NII. *Note (2): Indicates more than one (isolated) stellar line interfers, * typically for a broad DIB (diffuse interstellar band). The * corresponding sum of the equivalent widths is given in BEW. *Note (3): * b = the stellar line measured is itself a blend of at least two lines. C============================================================================= C Loading file 'table2.dat' ! Diffuse interstellar bands (DIBs) in the * spectrum of HD 183143 C Format for file interpretation 1 format( + F7.2,1X,A1,1X,F7.2,1X,F7.2,1X,A1,1X,F7.2,1X,A1,1X,F7.2,1X, + F5.2,1X,A1,F6.1,1X,A1,1X,F4.1,1X,A5,1X,F7.2,1X,A1,F7.2,1X,A1, + 1X,F5.1,1X,A1,1X,I3) C Effective file loading open(unit=1,status='old',file= +'table2.dat') write(6,*) '....Loading file: table2.dat' do i__=1,418 read(1,'(A103)')ar__ read(ar__,1) + JD94(i__),f_JD94(i__),GM00(i__),TC00(i__),f_TC00(i__), + WS00(i__),f_WS00(i__),Wc(i__),FWHM(i__),l_EW(i__),EW(i__), + f_EW(i__),e_EW(i__),n_EW(i__),RWc(i__),l_BWc(i__),BWc(i__), + f_BWc(i__),BEW(i__),f_BEW(i__),Seq(i__) if(ar__(1:7) .EQ. '') JD94(i__) = rNULL__ if(ar__(11:17) .EQ. '') GM00(i__) = rNULL__ if(ar__(19:25) .EQ. '') TC00(i__) = rNULL__ if(ar__(29:35) .EQ. '') WS00(i__) = rNULL__ if(ar__(47:51) .EQ. '') FWHM(i__) = rNULL__ if(ar__(54:59) .EQ. '') EW(i__) = rNULL__ if(ar__(63:66) .EQ. '') e_EW(i__) = rNULL__ if(ar__(83:89) .EQ. '') BWc(i__) = rNULL__ if(ar__(93:97) .EQ. '') BEW(i__) = rNULL__ if(ar__(101:103) .EQ. '') Seq(i__) = iNULL__ c ..............Just test output........... write(6,1) + JD94(i__),f_JD94(i__),GM00(i__),TC00(i__),f_TC00(i__), + WS00(i__),f_WS00(i__),Wc(i__),FWHM(i__),l_EW(i__),EW(i__), + f_EW(i__),e_EW(i__),n_EW(i__),RWc(i__),l_BWc(i__),BWc(i__), + f_BWc(i__),BEW(i__),f_BEW(i__),Seq(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= C Loading file 'table3.dat' ! 71 possible diffuse interstellar bands in the * spectrum of HD 183143 C Format for file interpretation 2 format( + F7.2,1X,A1,1X,F7.2,1X,F7.2,1X,A1,1X,F7.2,1X,A1,1X,F7.2,1X, + F5.2,1X,A1,F6.1,1X,A1,1X,F4.1,1X,A5,1X,F7.2,1X,A1,F7.2,1X,A1, + 1X,F5.1,1X,A1,1X,I3) C Effective file loading open(unit=1,status='old',file= +'table3.dat') write(6,*) '....Loading file: table3.dat' do i__=1,71 read(1,'(A103)')ar__1 read(ar__1,2) + JD94_1(i__),f_JD94_1(i__),GM00_1(i__),TC00_1(i__), + f_TC00_1(i__),WS00_1(i__),f_WS00_1(i__),Wc_1(i__),FWHM_1(i__), + l_EW_1(i__),EW_1(i__),f_EW_1(i__),e_EW_1(i__),n_EW_1(i__), + RWc_1(i__),l_BWc_1(i__),BWc_1(i__),f_BWc_1(i__),BEW_1(i__), + f_BEW_1(i__),Seq_1(i__) if(ar__1(1:7) .EQ. '') JD94_1(i__) = rNULL__ if(ar__1(11:17) .EQ. '') GM00_1(i__) = rNULL__ if(ar__1(19:25) .EQ. '') TC00_1(i__) = rNULL__ if(ar__1(29:35) .EQ. '') WS00_1(i__) = rNULL__ if(ar__1(47:51) .EQ. '') FWHM_1(i__) = rNULL__ if(ar__1(54:59) .EQ. '') EW_1(i__) = rNULL__ if(ar__1(63:66) .EQ. '') e_EW_1(i__) = rNULL__ if(ar__1(83:89) .EQ. '') BWc_1(i__) = rNULL__ if(ar__1(93:97) .EQ. '') BEW_1(i__) = rNULL__ if(ar__1(101:103) .EQ. '') Seq_1(i__) = iNULL__ c ..............Just test output........... write(6,2) + JD94_1(i__),f_JD94_1(i__),GM00_1(i__),TC00_1(i__), + f_TC00_1(i__),WS00_1(i__),f_WS00_1(i__),Wc_1(i__),FWHM_1(i__), + l_EW_1(i__),EW_1(i__),f_EW_1(i__),e_EW_1(i__),n_EW_1(i__), + RWc_1(i__),l_BWc_1(i__),BWc_1(i__),f_BWc_1(i__),BEW_1(i__), + f_BEW_1(i__),Seq_1(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= stop end