Conversion of standardized ReadMe file for
file /./ftp/cats/J/AJ/137/3869 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-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/AJ/137/3869 Radio SNRs in 4 irregular galaxies (Chomiuk+, 2009) *================================================================================ *A search for radio supernova remnants in four irregular galaxies. * Chomiuk L., Wilcots E.M. * <Astron. J., 137, 3869-3883 (2009)> * =2009AJ....137.3869C C============================================================================= C Internal variables integer*4 i__ c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table4.dat' ! 20cm sources in NGC 1569 integer*4 nr__ parameter (nr__=46) ! Number of records character*106 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*8 v_CW2009_ (nr__) ! Source name, N1569-NN, N4214-NN, N2366-NN, * or N4449-NN character*1 n__CW2009_ (nr__) ! [*] Variable source (1) 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) real*4 amaj (nr__) ! (arcsec) Major axis real*4 amin (nr__) ! (arcsec) Minor axis real*4 S20cm (nr__) ! (mJy) Flux density at 20cm (1.5GHz) real*4 e_S20cm (nr__) ! (mJy) rms uncertainty on S20cm character*1 l_S6cm (nr__) ! Limit flag on S6cm (5GHz) real*4 S6cm (nr__) ! (mJy) Flux density at 6cm real*4 e_S6cm (nr__) ! (mJy) ? rms uncertainty on S6cm character*1 l_S3_6cm (nr__) ! Limit flag on S3.6cm (8.3GHz) real*4 S3_6cm (nr__) ! (mJy) ?=- Flux density at 3.6cm real*4 e_S3_6cm (nr__) ! (mJy) ? rms uncertainty on S3.6cm character*1 l_alpha (nr__) ! Limit flag on alpha real*4 alpha (nr__) ! Spectral index {alpha} [S{prop.to}nu^{alpha}^] real*4 e_alpha (nr__) ! ? rms uncertainty on alpha character*3 Ha (nr__) ! [Yes/No ] H{alpha} emission? character*11 Class (nr__) ! Classification (2) character*1 n_Class (nr__) ! [ab] Note (1) *Note (1): Notes as follows: * * = The flux of this source is time variable and, therefore, given * the different epochs of the flux measurements, the spectral * index is not trustworthy. * a = This source is actually likely an SNR based on [FeII] and Pabeta * emission in Labrie & Pritchet (2006ApJS..166..188L). * b = Additional data in the literature lend credence to this * characterization; see Section 6. *Note (2): Classification as follows: * Bkg = no apparent H{alpha} emission associated with it * Bkg (>R_25) = no apparent H{alpha} emission associated with it, * source located beyond the galaxy's optical diameter * SNR = has {alpha}<=-0.2 and H{alpha} emission associated with it * H II = has {alpha}>-0.2 and H{alpha} emission associated with it c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table5.dat' ! 20cm sources in NGC 4214 integer*4 nr__1 parameter (nr__1=29) ! Number of records character*106 ar__1 ! Full-size record C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs real*8 RAdeg_1 (nr__1) ! (deg) Right Ascension J2000 real*8 DEdeg_1 (nr__1) ! (deg) Declination J2000 C ---------------------------------- ! (position vector(s) in degrees) character*8 v_CW2009__1(nr__1) ! Source name, N1569-NN, N4214-NN, N2366-NN, * or N4449-NN character*1 n__CW2009__1(nr__1) ! [*] Variable source (1) integer*4 RAh_1 (nr__1) ! (h) Right ascension (J2000) integer*4 RAm_1 (nr__1) ! (min) Right ascension (J2000) real*4 RAs_1 (nr__1) ! (s) Right ascension (J2000) character*1 DE__1 (nr__1) ! Declination sign (J2000) integer*4 DEd_1 (nr__1) ! (deg) Declination (J2000) integer*4 DEm_1 (nr__1) ! (arcmin) Declination (J2000) real*4 DEs_1 (nr__1) ! (arcsec) Declination (J2000) real*4 amaj_1 (nr__1) ! (arcsec) Major axis real*4 amin_1 (nr__1) ! (arcsec) Minor axis real*4 S20cm_1 (nr__1) ! (mJy) Flux density at 20cm (1.5GHz) real*4 e_S20cm_1 (nr__1) ! (mJy) rms uncertainty on S20cm character*1 l_S6cm_1 (nr__1) ! Limit flag on S6cm (5GHz) real*4 S6cm_1 (nr__1) ! (mJy) Flux density at 6cm real*4 e_S6cm_1 (nr__1) ! (mJy) ? rms uncertainty on S6cm character*1 l_S3_6cm_1 (nr__1) ! Limit flag on S3.6cm (8.3GHz) real*4 S3_6cm_1 (nr__1) ! (mJy) ?=- Flux density at 3.6cm real*4 e_S3_6cm_1 (nr__1) ! (mJy) ? rms uncertainty on S3.6cm character*1 l_alpha_1 (nr__1) ! Limit flag on alpha real*4 alpha_1 (nr__1) ! Spectral index {alpha} [S{prop.to}nu^{alpha}^] real*4 e_alpha_1 (nr__1) ! ? rms uncertainty on alpha character*3 Ha_1 (nr__1) ! [Yes/No ] H{alpha} emission? character*11 Class_1 (nr__1) ! Classification (2) character*1 n_Class_1 (nr__1) ! [ab] Note (1) *Note (1): Notes as follows: * * = The flux of this source is time variable and, therefore, given * the different epochs of the flux measurements, the spectral * index is not trustworthy. * a = This source is actually likely an SNR based on [FeII] and Pabeta * emission in Labrie & Pritchet (2006ApJS..166..188L). * b = Additional data in the literature lend credence to this * characterization; see Section 6. *Note (2): Classification as follows: * Bkg = no apparent H{alpha} emission associated with it * Bkg (>R_25) = no apparent H{alpha} emission associated with it, * source located beyond the galaxy's optical diameter * SNR = has {alpha}<=-0.2 and H{alpha} emission associated with it * H II = has {alpha}>-0.2 and H{alpha} emission associated with it c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table6.dat' ! 20cm sources in NGC 2366 integer*4 nr__2 parameter (nr__2=24) ! Number of records character*106 ar__2 ! Full-size record C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs real*8 RAdeg_2 (nr__2) ! (deg) Right Ascension J2000 real*8 DEdeg_2 (nr__2) ! (deg) Declination J2000 C ---------------------------------- ! (position vector(s) in degrees) character*8 v_CW2009__2(nr__2) ! Source name, N1569-NN, N4214-NN, N2366-NN, * or N4449-NN character*1 n__CW2009__2(nr__2) ! [*] Variable source (1) integer*4 RAh_2 (nr__2) ! (h) Right ascension (J2000) integer*4 RAm_2 (nr__2) ! (min) Right ascension (J2000) real*4 RAs_2 (nr__2) ! (s) Right ascension (J2000) character*1 DE__2 (nr__2) ! Declination sign (J2000) integer*4 DEd_2 (nr__2) ! (deg) Declination (J2000) integer*4 DEm_2 (nr__2) ! (arcmin) Declination (J2000) real*4 DEs_2 (nr__2) ! (arcsec) Declination (J2000) real*4 amaj_2 (nr__2) ! (arcsec) Major axis real*4 amin_2 (nr__2) ! (arcsec) Minor axis real*4 S20cm_2 (nr__2) ! (mJy) Flux density at 20cm (1.5GHz) real*4 e_S20cm_2 (nr__2) ! (mJy) rms uncertainty on S20cm character*1 l_S6cm_2 (nr__2) ! Limit flag on S6cm (5GHz) real*4 S6cm_2 (nr__2) ! (mJy) Flux density at 6cm real*4 e_S6cm_2 (nr__2) ! (mJy) ? rms uncertainty on S6cm character*1 l_S3_6cm_2 (nr__2) ! Limit flag on S3.6cm (8.3GHz) real*4 S3_6cm_2 (nr__2) ! (mJy) ?=- Flux density at 3.6cm real*4 e_S3_6cm_2 (nr__2) ! (mJy) ? rms uncertainty on S3.6cm character*1 l_alpha_2 (nr__2) ! Limit flag on alpha real*4 alpha_2 (nr__2) ! Spectral index {alpha} [S{prop.to}nu^{alpha}^] real*4 e_alpha_2 (nr__2) ! ? rms uncertainty on alpha character*3 Ha_2 (nr__2) ! [Yes/No ] H{alpha} emission? character*11 Class_2 (nr__2) ! Classification (2) character*1 n_Class_2 (nr__2) ! [ab] Note (1) *Note (1): Notes as follows: * * = The flux of this source is time variable and, therefore, given * the different epochs of the flux measurements, the spectral * index is not trustworthy. * a = This source is actually likely an SNR based on [FeII] and Pabeta * emission in Labrie & Pritchet (2006ApJS..166..188L). * b = Additional data in the literature lend credence to this * characterization; see Section 6. *Note (2): Classification as follows: * Bkg = no apparent H{alpha} emission associated with it * Bkg (>R_25) = no apparent H{alpha} emission associated with it, * source located beyond the galaxy's optical diameter * SNR = has {alpha}<=-0.2 and H{alpha} emission associated with it * H II = has {alpha}>-0.2 and H{alpha} emission associated with it c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table7.dat' ! 20cm sources in NGC 4449 integer*4 nr__3 parameter (nr__3=30) ! Number of records character*106 ar__3 ! Full-size record C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs real*8 RAdeg_3 (nr__3) ! (deg) Right Ascension J2000 real*8 DEdeg_3 (nr__3) ! (deg) Declination J2000 C ---------------------------------- ! (position vector(s) in degrees) character*8 v_CW2009__3(nr__3) ! Source name, N1569-NN, N4214-NN, N2366-NN, * or N4449-NN character*1 n__CW2009__3(nr__3) ! [*] Variable source (1) integer*4 RAh_3 (nr__3) ! (h) Right ascension (J2000) integer*4 RAm_3 (nr__3) ! (min) Right ascension (J2000) real*4 RAs_3 (nr__3) ! (s) Right ascension (J2000) character*1 DE__3 (nr__3) ! Declination sign (J2000) integer*4 DEd_3 (nr__3) ! (deg) Declination (J2000) integer*4 DEm_3 (nr__3) ! (arcmin) Declination (J2000) real*4 DEs_3 (nr__3) ! (arcsec) Declination (J2000) real*4 amaj_3 (nr__3) ! (arcsec) Major axis real*4 amin_3 (nr__3) ! (arcsec) Minor axis real*4 S20cm_3 (nr__3) ! (mJy) Flux density at 20cm (1.5GHz) real*4 e_S20cm_3 (nr__3) ! (mJy) rms uncertainty on S20cm character*1 l_S6cm_3 (nr__3) ! Limit flag on S6cm (5GHz) real*4 S6cm_3 (nr__3) ! (mJy) Flux density at 6cm real*4 e_S6cm_3 (nr__3) ! (mJy) ? rms uncertainty on S6cm character*1 l_S3_6cm_3 (nr__3) ! Limit flag on S3.6cm (8.3GHz) real*4 S3_6cm_3 (nr__3) ! (mJy) ?=- Flux density at 3.6cm real*4 e_S3_6cm_3 (nr__3) ! (mJy) ? rms uncertainty on S3.6cm character*1 l_alpha_3 (nr__3) ! Limit flag on alpha real*4 alpha_3 (nr__3) ! Spectral index {alpha} [S{prop.to}nu^{alpha}^] real*4 e_alpha_3 (nr__3) ! ? rms uncertainty on alpha character*3 Ha_3 (nr__3) ! [Yes/No ] H{alpha} emission? character*11 Class_3 (nr__3) ! Classification (2) character*1 n_Class_3 (nr__3) ! [ab] Note (1) *Note (1): Notes as follows: * * = The flux of this source is time variable and, therefore, given * the different epochs of the flux measurements, the spectral * index is not trustworthy. * a = This source is actually likely an SNR based on [FeII] and Pabeta * emission in Labrie & Pritchet (2006ApJS..166..188L). * b = Additional data in the literature lend credence to this * characterization; see Section 6. *Note (2): Classification as follows: * Bkg = no apparent H{alpha} emission associated with it * Bkg (>R_25) = no apparent H{alpha} emission associated with it, * source located beyond the galaxy's optical diameter * SNR = has {alpha}<=-0.2 and H{alpha} emission associated with it * H II = has {alpha}>-0.2 and H{alpha} emission associated with it C============================================================================= C Loading file 'table4.dat' ! 20cm sources in NGC 1569 C Format for file interpretation 1 format( + A8,A1,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,F4.1,1X, + F4.1,1X,F5.2,1X,F4.2,1X,A1,F4.2,1X,F4.2,1X,A1,F4.2,1X,F5.3,1X, + A1,F5.2,1X,F4.2,1X,A3,1X,A11,A1) C Effective file loading open(unit=1,status='old',file= +'table4.dat') write(6,*) '....Loading file: table4.dat' do i__=1,46 read(1,'(A106)')ar__ read(ar__,1) + v_CW2009_(i__),n__CW2009_(i__),RAh(i__),RAm(i__),RAs(i__), + DE_(i__),DEd(i__),DEm(i__),DEs(i__),amaj(i__),amin(i__), + S20cm(i__),e_S20cm(i__),l_S6cm(i__),S6cm(i__),e_S6cm(i__), + l_S3_6cm(i__),S3_6cm(i__),e_S3_6cm(i__),l_alpha(i__), + alpha(i__),e_alpha(i__),Ha(i__),Class(i__),n_Class(i__) if(ar__(62:65) .EQ. '') e_S6cm(i__) = rNULL__ if (idig(ar__(68:71)).EQ.0) S3_6cm(i__) = rNULL__ if(ar__(73:77) .EQ. '') e_S3_6cm(i__) = rNULL__ if(ar__(86:89) .EQ. '') e_alpha(i__) = rNULL__ 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) + v_CW2009_(i__),n__CW2009_(i__),RAh(i__),RAm(i__),RAs(i__), + DE_(i__),DEd(i__),DEm(i__),DEs(i__),amaj(i__),amin(i__), + S20cm(i__),e_S20cm(i__),l_S6cm(i__),S6cm(i__),e_S6cm(i__), + l_S3_6cm(i__),S3_6cm(i__),e_S3_6cm(i__),l_alpha(i__), + alpha(i__),e_alpha(i__),Ha(i__),Class(i__),n_Class(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 'table5.dat' ! 20cm sources in NGC 4214 C Format for file interpretation 2 format( + A8,A1,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,F4.1,1X, + F4.1,1X,F5.2,1X,F4.2,1X,A1,F4.2,1X,F4.2,1X,A1,F4.2,1X,F5.3,1X, + A1,F5.2,1X,F4.2,1X,A3,1X,A11,A1) C Effective file loading open(unit=1,status='old',file= +'table5.dat') write(6,*) '....Loading file: table5.dat' do i__=1,29 read(1,'(A106)')ar__1 read(ar__1,2) + v_CW2009__1(i__),n__CW2009__1(i__),RAh_1(i__),RAm_1(i__), + RAs_1(i__),DE__1(i__),DEd_1(i__),DEm_1(i__),DEs_1(i__), + amaj_1(i__),amin_1(i__),S20cm_1(i__),e_S20cm_1(i__), + l_S6cm_1(i__),S6cm_1(i__),e_S6cm_1(i__),l_S3_6cm_1(i__), + S3_6cm_1(i__),e_S3_6cm_1(i__),l_alpha_1(i__),alpha_1(i__), + e_alpha_1(i__),Ha_1(i__),Class_1(i__),n_Class_1(i__) if(ar__1(62:65) .EQ. '') e_S6cm_1(i__) = rNULL__ if (idig(ar__1(68:71)).EQ.0) S3_6cm_1(i__) = rNULL__ if(ar__1(73:77) .EQ. '') e_S3_6cm_1(i__) = rNULL__ if(ar__1(86:89) .EQ. '') e_alpha_1(i__) = rNULL__ RAdeg_1(i__) = rNULL__ DEdeg_1(i__) = rNULL__ c Derive coordinates RAdeg_1 and DEdeg_1 from input data c (RAdeg_1 and DEdeg_1 are set to rNULL__ when unknown) if(RAh_1(i__) .GT. -180) RAdeg_1(i__)=RAh_1(i__)*15. if(RAm_1(i__) .GT. -180) RAdeg_1(i__)=RAdeg_1(i__)+RAm_1(i__)/4. if(RAs_1(i__) .GT. -180) RAdeg_1(i__)=RAdeg_1(i__)+RAs_1(i__)/240. if(DEd_1(i__) .GE. 0) DEdeg_1(i__)=DEd_1(i__) if(DEm_1(i__) .GE. 0) DEdeg_1(i__)=DEdeg_1(i__)+DEm_1(i__)/60. if(DEs_1(i__) .GE. 0) DEdeg_1(i__)=DEdeg_1(i__)+DEs_1(i__)/3600. if(DE__1(i__).EQ.'-'.AND.DEdeg_1(i__).GE.0) DEdeg_1(i__)=-DEdeg_1(i__) c ..............Just test output........... write(6,2) + v_CW2009__1(i__),n__CW2009__1(i__),RAh_1(i__),RAm_1(i__), + RAs_1(i__),DE__1(i__),DEd_1(i__),DEm_1(i__),DEs_1(i__), + amaj_1(i__),amin_1(i__),S20cm_1(i__),e_S20cm_1(i__), + l_S6cm_1(i__),S6cm_1(i__),e_S6cm_1(i__),l_S3_6cm_1(i__), + S3_6cm_1(i__),e_S3_6cm_1(i__),l_alpha_1(i__),alpha_1(i__), + e_alpha_1(i__),Ha_1(i__),Class_1(i__),n_Class_1(i__) write(6,'(6H Pos: 2F8.4)') RAdeg_1(i__),DEdeg_1(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= C Loading file 'table6.dat' ! 20cm sources in NGC 2366 C Format for file interpretation 3 format( + A8,A1,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,F4.1,1X, + F4.1,1X,F5.2,1X,F4.2,1X,A1,F4.2,1X,F4.2,1X,A1,F4.2,1X,F5.3,1X, + A1,F5.2,1X,F4.2,1X,A3,1X,A11,A1) C Effective file loading open(unit=1,status='old',file= +'table6.dat') write(6,*) '....Loading file: table6.dat' do i__=1,24 read(1,'(A106)')ar__2 read(ar__2,3) + v_CW2009__2(i__),n__CW2009__2(i__),RAh_2(i__),RAm_2(i__), + RAs_2(i__),DE__2(i__),DEd_2(i__),DEm_2(i__),DEs_2(i__), + amaj_2(i__),amin_2(i__),S20cm_2(i__),e_S20cm_2(i__), + l_S6cm_2(i__),S6cm_2(i__),e_S6cm_2(i__),l_S3_6cm_2(i__), + S3_6cm_2(i__),e_S3_6cm_2(i__),l_alpha_2(i__),alpha_2(i__), + e_alpha_2(i__),Ha_2(i__),Class_2(i__),n_Class_2(i__) if(ar__2(62:65) .EQ. '') e_S6cm_2(i__) = rNULL__ if (idig(ar__2(68:71)).EQ.0) S3_6cm_2(i__) = rNULL__ if(ar__2(73:77) .EQ. '') e_S3_6cm_2(i__) = rNULL__ if(ar__2(86:89) .EQ. '') e_alpha_2(i__) = rNULL__ RAdeg_2(i__) = rNULL__ DEdeg_2(i__) = rNULL__ c Derive coordinates RAdeg_2 and DEdeg_2 from input data c (RAdeg_2 and DEdeg_2 are set to rNULL__ when unknown) if(RAh_2(i__) .GT. -180) RAdeg_2(i__)=RAh_2(i__)*15. if(RAm_2(i__) .GT. -180) RAdeg_2(i__)=RAdeg_2(i__)+RAm_2(i__)/4. if(RAs_2(i__) .GT. -180) RAdeg_2(i__)=RAdeg_2(i__)+RAs_2(i__)/240. if(DEd_2(i__) .GE. 0) DEdeg_2(i__)=DEd_2(i__) if(DEm_2(i__) .GE. 0) DEdeg_2(i__)=DEdeg_2(i__)+DEm_2(i__)/60. if(DEs_2(i__) .GE. 0) DEdeg_2(i__)=DEdeg_2(i__)+DEs_2(i__)/3600. if(DE__2(i__).EQ.'-'.AND.DEdeg_2(i__).GE.0) DEdeg_2(i__)=-DEdeg_2(i__) c ..............Just test output........... write(6,3) + v_CW2009__2(i__),n__CW2009__2(i__),RAh_2(i__),RAm_2(i__), + RAs_2(i__),DE__2(i__),DEd_2(i__),DEm_2(i__),DEs_2(i__), + amaj_2(i__),amin_2(i__),S20cm_2(i__),e_S20cm_2(i__), + l_S6cm_2(i__),S6cm_2(i__),e_S6cm_2(i__),l_S3_6cm_2(i__), + S3_6cm_2(i__),e_S3_6cm_2(i__),l_alpha_2(i__),alpha_2(i__), + e_alpha_2(i__),Ha_2(i__),Class_2(i__),n_Class_2(i__) write(6,'(6H Pos: 2F8.4)') RAdeg_2(i__),DEdeg_2(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= C Loading file 'table7.dat' ! 20cm sources in NGC 4449 C Format for file interpretation 4 format( + A8,A1,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,F4.1,1X, + F4.1,1X,F5.2,1X,F4.2,1X,A1,F4.2,1X,F4.2,1X,A1,F4.2,1X,F5.3,1X, + A1,F5.2,1X,F4.2,1X,A3,1X,A11,A1) C Effective file loading open(unit=1,status='old',file= +'table7.dat') write(6,*) '....Loading file: table7.dat' do i__=1,30 read(1,'(A106)')ar__3 read(ar__3,4) + v_CW2009__3(i__),n__CW2009__3(i__),RAh_3(i__),RAm_3(i__), + RAs_3(i__),DE__3(i__),DEd_3(i__),DEm_3(i__),DEs_3(i__), + amaj_3(i__),amin_3(i__),S20cm_3(i__),e_S20cm_3(i__), + l_S6cm_3(i__),S6cm_3(i__),e_S6cm_3(i__),l_S3_6cm_3(i__), + S3_6cm_3(i__),e_S3_6cm_3(i__),l_alpha_3(i__),alpha_3(i__), + e_alpha_3(i__),Ha_3(i__),Class_3(i__),n_Class_3(i__) if(ar__3(62:65) .EQ. '') e_S6cm_3(i__) = rNULL__ if (idig(ar__3(68:71)).EQ.0) S3_6cm_3(i__) = rNULL__ if(ar__3(73:77) .EQ. '') e_S3_6cm_3(i__) = rNULL__ if(ar__3(86:89) .EQ. '') e_alpha_3(i__) = rNULL__ RAdeg_3(i__) = rNULL__ DEdeg_3(i__) = rNULL__ c Derive coordinates RAdeg_3 and DEdeg_3 from input data c (RAdeg_3 and DEdeg_3 are set to rNULL__ when unknown) if(RAh_3(i__) .GT. -180) RAdeg_3(i__)=RAh_3(i__)*15. if(RAm_3(i__) .GT. -180) RAdeg_3(i__)=RAdeg_3(i__)+RAm_3(i__)/4. if(RAs_3(i__) .GT. -180) RAdeg_3(i__)=RAdeg_3(i__)+RAs_3(i__)/240. if(DEd_3(i__) .GE. 0) DEdeg_3(i__)=DEd_3(i__) if(DEm_3(i__) .GE. 0) DEdeg_3(i__)=DEdeg_3(i__)+DEm_3(i__)/60. if(DEs_3(i__) .GE. 0) DEdeg_3(i__)=DEdeg_3(i__)+DEs_3(i__)/3600. if(DE__3(i__).EQ.'-'.AND.DEdeg_3(i__).GE.0) DEdeg_3(i__)=-DEdeg_3(i__) c ..............Just test output........... write(6,4) + v_CW2009__3(i__),n__CW2009__3(i__),RAh_3(i__),RAm_3(i__), + RAs_3(i__),DE__3(i__),DEd_3(i__),DEm_3(i__),DEs_3(i__), + amaj_3(i__),amin_3(i__),S20cm_3(i__),e_S20cm_3(i__), + l_S6cm_3(i__),S6cm_3(i__),e_S6cm_3(i__),l_S3_6cm_3(i__), + S3_6cm_3(i__),e_S3_6cm_3(i__),l_alpha_3(i__),alpha_3(i__), + e_alpha_3(i__),Ha_3(i__),Class_3(i__),n_Class_3(i__) write(6,'(6H Pos: 2F8.4)') RAdeg_3(i__),DEdeg_3(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