Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/641/410 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-Apr-17 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/641/410 XMM and Chandra X-ray sources near 4U 1755-33 (Kaaret+, 2006) *================================================================================ *Evolution of the X-ray jets from 4U 1755-33. * Kaaret P., Corbel S., Tomsick J.A., Lazendic J., Tzioumis A.K., Butt Y., * Wijnands R. * <Astrophys. J., 641, 410-417 (2006)> * =2006ApJ...641..410K C============================================================================= C Internal variables integer*4 i__ c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table1.dat' ! XMM-Newton X-ray sources near 4U 1755-33 integer*4 nr__ parameter (nr__=27) ! Number of records character*82 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) integer*4 v_KCT2006_ (nr__) ! Source number (1) integer*4 RAh (nr__) ! (h) Hour of Right Ascension (J2000) integer*4 RAm (nr__) ! (min) Minute of Right Ascension (J2000) real*4 RAs (nr__) ! (s) Second of Right Ascension (J2000) character*1 DE_ (nr__) ! Sign of the Declination (J2000) integer*4 DEd (nr__) ! (deg) Degree of Declination (J2000) integer*4 DEm (nr__) ! (arcmin) Arcminute of Declination (J2000) real*4 DEs (nr__) ! (arcsec) Arcsecond of Declination (J2000) real*4 ePos (nr__) ! (arcsec) Statistical source position error (2) character*1 n_Flux1 (nr__) ! [A3] Indicates the date of observation * of the first flux (3) real*4 Flux1 (nr__) ! (10-17W/m2) ? First 0.3-10keV flux (4) real*4 e_Flux1 (nr__) ! (10-17W/m2) ? Uncertainty in Flux1 character*1 n_Flux2 (nr__) ! [B4] Indicates the date of observation * of the second flux (3) real*4 Flux2 (nr__) ! (10-17W/m2) ? Second 0.3-10keV flux (4) real*4 e_Flux2 (nr__) ! (10-17W/m2) ? Uncertainty in Flux2 character*17 xID (nr__) ! Counterpart (5) character*5 v2MASS (nr__) ! [2mass] 2MASS counterpart (Cat. II/246) *Note (1): Source number is: * Table 1: [KCT2006] XMM NN in Simbad * Table 3: [KCT2006] Chandra NN in Simbad *Note (2): This does not include errors in the overall astrometry. *Note (3): The date of observation are coded as follows: * A = refers to an XMM-Newton archival observation obtained by Angelini * & White (2003ApJ...586L..71A) beginning on 2001-Mar-08 * with a duration of 19.4ks (ObsID 0032940101) (Table 1 only) * B = refers to an XMM-Newton observation beginning on 2004-Sep-18 * for 45.9ks (ObsID 0203750101) (Table 1 only) * 3 = refers to a 22ks exposure Chandra observation obtained on * 2003-Sep-25 (ObsID 3510; PI S. Murray) (Table 3 only) * 4 = refers to a 45ks exposure Chandra observation obtained on * 2004-Jun-25 (ObsID 4586; PI L. Angelini) (Table 3 only) *Note (4): In units of 10^-14^erg/cm^2^/s and calculated assuming a power * law spectrum with photon index of 1.5 and corrected for the Galactic * absorption column density of 3.1x10^21^cm^-2^. *Note (5): Counterparts in Angelini & White (2003ApJ...586L..71A, * [AW2003] N in Simbad), or the XMM sources in Table 1 (XMM NN). c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table3.dat' ! Chandra X-ray sources near 4U 1755-33 integer*4 nr__1 parameter (nr__1=56) ! Number of records character*82 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) integer*4 v_KCT2006__1(nr__1) ! Source number (1) integer*4 RAh_1 (nr__1) ! (h) Hour of Right Ascension (J2000) integer*4 RAm_1 (nr__1) ! (min) Minute of Right Ascension (J2000) real*4 RAs_1 (nr__1) ! (s) Second of Right Ascension (J2000) character*1 DE__1 (nr__1) ! Sign of the Declination (J2000) integer*4 DEd_1 (nr__1) ! (deg) Degree of Declination (J2000) integer*4 DEm_1 (nr__1) ! (arcmin) Arcminute of Declination (J2000) real*4 DEs_1 (nr__1) ! (arcsec) Arcsecond of Declination (J2000) real*4 ePos_1 (nr__1) ! (arcsec) Statistical source position error (2) character*1 n_Flux1_1 (nr__1) ! [A3] Indicates the date of observation * of the first flux (3) real*4 Flux1_1 (nr__1) ! (10-17W/m2) ? First 0.3-10keV flux (4) real*4 e_Flux1_1 (nr__1) ! (10-17W/m2) ? Uncertainty in Flux1 character*1 n_Flux2_1 (nr__1) ! [B4] Indicates the date of observation * of the second flux (3) real*4 Flux2_1 (nr__1) ! (10-17W/m2) ? Second 0.3-10keV flux (4) real*4 e_Flux2_1 (nr__1) ! (10-17W/m2) ? Uncertainty in Flux2 character*17 xID_1 (nr__1) ! Counterpart (5) character*5 v2MASS_1 (nr__1) ! [2mass] 2MASS counterpart (Cat. II/246) *Note (1): Source number is: * Table 1: [KCT2006] XMM NN in Simbad * Table 3: [KCT2006] Chandra NN in Simbad *Note (2): This does not include errors in the overall astrometry. *Note (3): The date of observation are coded as follows: * A = refers to an XMM-Newton archival observation obtained by Angelini * & White (2003ApJ...586L..71A) beginning on 2001-Mar-08 * with a duration of 19.4ks (ObsID 0032940101) (Table 1 only) * B = refers to an XMM-Newton observation beginning on 2004-Sep-18 * for 45.9ks (ObsID 0203750101) (Table 1 only) * 3 = refers to a 22ks exposure Chandra observation obtained on * 2003-Sep-25 (ObsID 3510; PI S. Murray) (Table 3 only) * 4 = refers to a 45ks exposure Chandra observation obtained on * 2004-Jun-25 (ObsID 4586; PI L. Angelini) (Table 3 only) *Note (4): In units of 10^-14^erg/cm^2^/s and calculated assuming a power * law spectrum with photon index of 1.5 and corrected for the Galactic * absorption column density of 3.1x10^21^cm^-2^. *Note (5): Counterparts in Angelini & White (2003ApJ...586L..71A, * [AW2003] N in Simbad), or the XMM sources in Table 1 (XMM NN). C============================================================================= C Loading file 'table1.dat' ! XMM-Newton X-ray sources near 4U 1755-33 C Format for file interpretation 1 format( + I2,1X,I2,1X,I2,1X,F6.3,1X,A1,I2,1X,I2,1X,F5.2,1X,F3.1,1X,A1, + 1X,F5.1,1X,F4.1,1X,A1,1X,F5.1,1X,F4.1,1X,A17,1X,A5) C Effective file loading open(unit=1,status='old',file= +'table1.dat') write(6,*) '....Loading file: table1.dat' do i__=1,27 read(1,'(A82)')ar__ read(ar__,1) + v_KCT2006_(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__), + DEm(i__),DEs(i__),ePos(i__),n_Flux1(i__),Flux1(i__), + e_Flux1(i__),n_Flux2(i__),Flux2(i__),e_Flux2(i__),xID(i__), + v2MASS(i__) if(ar__(36:40) .EQ. '') Flux1(i__) = rNULL__ if(ar__(42:45) .EQ. '') e_Flux1(i__) = rNULL__ if(ar__(49:53) .EQ. '') Flux2(i__) = rNULL__ if(ar__(55:58) .EQ. '') e_Flux2(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_KCT2006_(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__), + DEm(i__),DEs(i__),ePos(i__),n_Flux1(i__),Flux1(i__), + e_Flux1(i__),n_Flux2(i__),Flux2(i__),e_Flux2(i__),xID(i__), + v2MASS(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 'table3.dat' ! Chandra X-ray sources near 4U 1755-33 C Format for file interpretation 2 format( + I2,1X,I2,1X,I2,1X,F6.3,1X,A1,I2,1X,I2,1X,F5.2,1X,F3.1,1X,A1, + 1X,F5.1,1X,F4.1,1X,A1,1X,F5.1,1X,F4.1,1X,A17,1X,A5) C Effective file loading open(unit=1,status='old',file= +'table3.dat') write(6,*) '....Loading file: table3.dat' do i__=1,56 read(1,'(A82)')ar__1 read(ar__1,2) + v_KCT2006__1(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__), + DEd_1(i__),DEm_1(i__),DEs_1(i__),ePos_1(i__),n_Flux1_1(i__), + Flux1_1(i__),e_Flux1_1(i__),n_Flux2_1(i__),Flux2_1(i__), + e_Flux2_1(i__),xID_1(i__),v2MASS_1(i__) if(ar__1(36:40) .EQ. '') Flux1_1(i__) = rNULL__ if(ar__1(42:45) .EQ. '') e_Flux1_1(i__) = rNULL__ if(ar__1(49:53) .EQ. '') Flux2_1(i__) = rNULL__ if(ar__1(55:58) .EQ. '') e_Flux2_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_KCT2006__1(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__), + DEd_1(i__),DEm_1(i__),DEs_1(i__),ePos_1(i__),n_Flux1_1(i__), + Flux1_1(i__),e_Flux1_1(i__),n_Flux2_1(i__),Flux2_1(i__), + e_Flux2_1(i__),xID_1(i__),v2MASS_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============================================================================= stop end