Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/701/535 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-29 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/701/535 A sample of candidate radio stars (Kimball+, 2009) *================================================================================ *A sample of candidate radio stars in FIRST and SDSS. * Kimball A.E., Knapp G.R., Ivezic Z., West A.A., Bochanski J.J., * Plotkin R.M., Gordon M.S. * <Astrophys. J., 701, 535-546 (2009)> * =2009ApJ...701..535K C============================================================================= C Internal variables integer*4 i__ c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table1.dat' ! Properties of the radio star candidates sample integer*4 nr__ parameter (nr__=112) ! Number of records character*118 ar__ ! Full-size record C J2000 position composed of: RAdeg DEdeg real*8 RAdeg ! (deg) SDSS Right Ascension in decimal degrees (J2000) real*8 DEdeg ! (deg) SDSS Declination in decimal degrees (J2000) real*8 RAFdeg ! (deg) FIRST Right Ascension in decimal degrees (J2000) real*8 DEFdeg ! (deg) FIRST Declination in decimal degrees (J2000) real*4 Sep ! (arcsec) Separation between SDSS and FIRST positions real*8 Dist ! (pc) Heliocentric distance (1) character*2 Sp ! Visually-confirmed MK spectral type character*1 Ha_ ! [ynm] Spectrum with reliable H{alpha} emission? * (y=yes, n=no, m=maybe) real*4 Speak ! (mJy) FIRST peak 20cm flux density in mJy/beam real*4 Sint ! (mJy) FIRST integrated 20cm flux density real*4 umag ! (mag) SDSS u band model magnitude real*4 gmag ! (mag) SDSS g band model magnitude real*4 rmag ! (mag) SDSS r band model magnitude real*4 imag ! (mag) SDSS i band model magnitude real*4 zmag ! (mag) SDSS z band model magnitude real*4 v4DCD ! Four-dimensional color distance (3) integer*4 v_KI2008_ ! Internal identification number (4) *Note (1): Determined using the photometric parallax relation of * Ivezic et al. (2008ApJ...684..287I); the relation is valid * only for stars on the main sequence. *Note (3): describes the statistical significance of the distance in color * space between a target object and the point on the stellar locus with * the same g–i color as the target; outliers have 4DCD>2, extreme * outliers 4DCD>3. See Section 4.1 of the paper for more details. *Note (4): From the radio catalog of Kimball & Ivezic (2008AJ....136..684K). c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table2.dat' ! Candidate radio stars with resolved radio emission integer*4 nr__1 parameter (nr__1=16) ! Number of records character*118 ar__1 ! Full-size record C J2000 position composed of: RAdeg DEdeg real*8 RAdeg_1 ! (deg) SDSS Right Ascension in decimal degrees (J2000) real*8 DEdeg_1 ! (deg) SDSS Declination in decimal degrees (J2000) real*8 RAFdeg_1 ! (deg) FIRST Right Ascension in decimal degrees (J2000) real*8 DEFdeg_1 ! (deg) FIRST Declination in decimal degrees (J2000) real*4 Sep_1 ! (arcsec) Separation between SDSS and FIRST positions real*8 Dist_1 ! (pc) Heliocentric distance (1) character*2 Sp_1 ! Visually-confirmed MK spectral type character*1 Ha__1 ! [ynm] Spectrum with reliable H{alpha} emission? * (y=yes, n=no, m=maybe) real*4 Speak_1 ! (mJy) FIRST peak 20cm flux density in mJy/beam real*4 Sint_1 ! (mJy) FIRST integrated 20cm flux density real*4 umag_1 ! (mag) SDSS u band model magnitude real*4 gmag_1 ! (mag) SDSS g band model magnitude real*4 rmag_1 ! (mag) SDSS r band model magnitude real*4 imag_1 ! (mag) SDSS i band model magnitude real*4 zmag_1 ! (mag) SDSS z band model magnitude real*4 v4DCD_1 ! Four-dimensional color distance (3) integer*4 v_KI2008__1 ! Internal identification number (4) *Note (1): Determined using the photometric parallax relation of * Ivezic et al. (2008ApJ...684..287I); the relation is valid * only for stars on the main sequence. *Note (3): describes the statistical significance of the distance in color * space between a target object and the point on the stellar locus with * the same g–i color as the target; outliers have 4DCD>2, extreme * outliers 4DCD>3. See Section 4.1 of the paper for more details. *Note (4): From the radio catalog of Kimball & Ivezic (2008AJ....136..684K). c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table3.dat' ! Candidate radio stars with complex radio emission integer*4 nr__2 parameter (nr__2=60) ! Number of records character*118 ar__2 ! Full-size record C J2000 position composed of: RAdeg DEdeg real*8 RAdeg_2 ! (deg) SDSS Right Ascension in decimal degrees (J2000) real*8 DEdeg_2 ! (deg) SDSS Declination in decimal degrees (J2000) real*8 RAFdeg_2 ! (deg) FIRST Right Ascension in decimal degrees (J2000) real*8 DEFdeg_2 ! (deg) FIRST Declination in decimal degrees (J2000) real*4 Sep_2 ! (arcsec) Separation between SDSS and FIRST positions real*8 Dist_2 ! (pc) Heliocentric distance (1) character*2 Sp_2 ! Visually-confirmed MK spectral type character*1 Ha__2 ! [ynm] Spectrum with reliable H{alpha} emission? * (y=yes, n=no, m=maybe) real*4 Speak_2 ! (mJy) FIRST peak 20cm flux density in mJy/beam real*4 Sint_2 ! (mJy) FIRST integrated 20cm flux density real*4 umag_2 ! (mag) SDSS u band model magnitude real*4 gmag_2 ! (mag) SDSS g band model magnitude real*4 rmag_2 ! (mag) SDSS r band model magnitude real*4 imag_2 ! (mag) SDSS i band model magnitude real*4 zmag_2 ! (mag) SDSS z band model magnitude real*4 v4DCD_2 ! Four-dimensional color distance (3) integer*4 v_KI2008__2 ! Internal identification number (4) *Note (1): Determined using the photometric parallax relation of * Ivezic et al. (2008ApJ...684..287I); the relation is valid * only for stars on the main sequence. *Note (3): describes the statistical significance of the distance in color * space between a target object and the point on the stellar locus with * the same g–i color as the target; outliers have 4DCD>2, extreme * outliers 4DCD>3. See Section 4.1 of the paper for more details. *Note (4): From the radio catalog of Kimball & Ivezic (2008AJ....136..684K). C============================================================================= C Loading file 'table1.dat' ! Properties of the radio star candidates sample C Format for file interpretation 1 format( + F11.7,1X,F12.8,1X,F9.5,1X,F9.5,1X,F4.2,1X,F10.3,1X,A2,1X,A1, + 2X,F6.2,1X,F6.2,1X,F4.1,1X,F4.1,1X,F4.1,1X,F4.1,1X,F4.1,1X, + F4.1,1X,I7) C Effective file loading open(unit=1,status='old',file= +'table1.dat') write(6,*) '....Loading file: table1.dat' do i__=1,112 read(1,'(A118)')ar__ read(ar__,1) + RAdeg,DEdeg,RAFdeg,DEFdeg,Sep,Dist,Sp,Ha_,Speak,Sint,umag, + gmag,rmag,imag,zmag,v4DCD,v_KI2008_ c ..............Just test output........... write(6,1) + RAdeg,DEdeg,RAFdeg,DEFdeg,Sep,Dist,Sp,Ha_,Speak,Sint,umag, + gmag,rmag,imag,zmag,v4DCD,v_KI2008_ c .......End.of.Just test output........... end do close(1) C============================================================================= C Loading file 'table2.dat' ! Candidate radio stars with resolved radio emission C Format for file interpretation 2 format( + F11.7,1X,F12.8,1X,F9.5,1X,F9.5,1X,F4.2,1X,F10.3,1X,A2,1X,A1, + 2X,F6.2,1X,F6.2,1X,F4.1,1X,F4.1,1X,F4.1,1X,F4.1,1X,F4.1,1X, + F4.1,1X,I7) C Effective file loading open(unit=1,status='old',file= +'table2.dat') write(6,*) '....Loading file: table2.dat' do i__=1,16 read(1,'(A118)')ar__1 read(ar__1,2) + RAdeg_1,DEdeg_1,RAFdeg_1,DEFdeg_1,Sep_1,Dist_1,Sp_1,Ha__1, + Speak_1,Sint_1,umag_1,gmag_1,rmag_1,imag_1,zmag_1,v4DCD_1, + v_KI2008__1 c ..............Just test output........... write(6,2) + RAdeg_1,DEdeg_1,RAFdeg_1,DEFdeg_1,Sep_1,Dist_1,Sp_1,Ha__1, + Speak_1,Sint_1,umag_1,gmag_1,rmag_1,imag_1,zmag_1,v4DCD_1, + v_KI2008__1 c .......End.of.Just test output........... end do close(1) C============================================================================= C Loading file 'table3.dat' ! Candidate radio stars with complex radio emission C Format for file interpretation 3 format( + F11.7,1X,F12.8,1X,F9.5,1X,F9.5,1X,F4.2,1X,F10.3,1X,A2,1X,A1, + 2X,F6.2,1X,F6.2,1X,F4.1,1X,F4.1,1X,F4.1,1X,F4.1,1X,F4.1,1X, + F4.1,1X,I7) C Effective file loading open(unit=1,status='old',file= +'table3.dat') write(6,*) '....Loading file: table3.dat' do i__=1,60 read(1,'(A118)')ar__2 read(ar__2,3) + RAdeg_2,DEdeg_2,RAFdeg_2,DEFdeg_2,Sep_2,Dist_2,Sp_2,Ha__2, + Speak_2,Sint_2,umag_2,gmag_2,rmag_2,imag_2,zmag_2,v4DCD_2, + v_KI2008__2 c ..............Just test output........... write(6,3) + RAdeg_2,DEdeg_2,RAFdeg_2,DEFdeg_2,Sep_2,Dist_2,Sp_2,Ha__2, + Speak_2,Sint_2,umag_2,gmag_2,rmag_2,imag_2,zmag_2,v4DCD_2, + v_KI2008__2 c .......End.of.Just test output........... end do close(1) C============================================================================= stop end