Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_A/460/695 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/A+A/460/695 Search for Associations Containing Young stars (Torres+, 2006) *================================================================================ *Search for Associations Containing Young stars (SACY). *I. Sample & Searching Method. * Torres C.A.O., Quast G.R., da Silva L., de la Reza R., Melo C.H.F., * Sterzik M. * <Astron. Astrophys. 460, 695 (2006)> * =2006A&A...460..695T C============================================================================= C Internal variables integer*4 i__ c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table3.dat' ! Astrometric, spectroscopic and photometric data of the SACY sample integer*4 nr__ parameter (nr__=1626) ! Number of records character*228 ar__ ! Full-size record C J2000.0 position composed of: RAh RAm RAs DE- DEd DEm DEs real*8 RAdeg (nr__) ! (deg) Right Ascension J2000.0 real*8 DEdeg (nr__) ! (deg) Declination J2000.0 C ---------------------------------- ! (position vector(s) in degrees) integer*4 Seq (nr__) ! Running number character*16 v1RXS (nr__) ! 1RXS (<IX/10>,<IX/29>) designation (1) character*16 Name (nr__) ! Hipparcos (<I/239>), Tycho-2 (<II/259>) or * UCAC2 (<I/289>) identification (2) character*13 OName (nr__) ! Other identification (HD, DM, other) (3) integer*4 RAh (nr__) ! (h) Right ascension (J2000.0) integer*4 RAm (nr__) ! (min) Right ascension (J2000.0) real*4 RAs (nr__) ! (s) Right ascension (J2000.0) character*1 DE_ (nr__) ! Declination sign (J2000.0) integer*4 DEd (nr__) ! (deg) Declination (J2000.0) integer*4 DEm (nr__) ! (arcmin) Declination (J2000.0) integer*4 DEs (nr__) ! (arcsec) Declination (J2000.0) real*8 pmRA (nr__) ! (mas/yr) Proper motion in RA (pmRA*cosDE) real*8 pmDE (nr__) ! (mas/yr) Proper motion in DE (pmDE) character*3 r_pmRA (nr__) ! Source of proper motions (4) real*4 HRV (nr__) ! (km/s) Heliocentric radial velocity (5) character*1 f_HRV (nr__) ! [:] Quality flag for RV real*4 e_HRV (nr__) ! (km/s) ? rms of the observed RV integer*4 Nobs (nr__) ! ? Number of observations (6) character*1 f_Nobs (nr__) ! [*] *: RV value comes from the literature (7) character*3 r_HRV (nr__) ! ? Source of radial velocity (8) character*5 n_HRV (nr__) ! [D,SB1234 ?] Multiplicity flag (9) real*4 Sep (nr__) ! (arcsec) ? Angular separation of visual binaries (10) real*4 dV (nr__) ! (mag) ? Magnitude difference of components (11) character*1 u_dV (nr__) ! [?] Uncertainty flag on dV real*4 vsini (nr__) ! (km/s) ? Rotational velocity real*4 e_vsini (nr__) ! (km/s) ? rms uncertainty on vsini character*3 r_vsini (nr__) ! ? Source of vsini (8) real*4 Plx (nr__) ! (mas) ? Trigonometric parallax real*4 e_Plx (nr__) ! (mas) ? Standard error in Plx character*3 r_Plx (nr__) ! Source of Plx (8) real*4 Vmag (nr__) ! (mag) Johnson V magnitude character*1 f_Vmag (nr__) ! [V] Quality flag indicating variability (12) real*4 B_V (nr__) ! (mag) ? Johnson B-V colour index real*4 V_I (nr__) ! (mag) ? Cousins V-I colour index character*3 r_Vmag (nr__) ! Source of photometry (13) character*1 n_Vmag (nr__) ! [*] *: photometry corrected for companions (14) character*8 SpType (nr__) ! MK spectral type integer*4 EWLi (nr__) ! (0.1pm) ? LiI equivalent width in milli-Angstroms (15) character*1 f_EWLi (nr__) ! [:?] Quality flag for EWLi real*4 EWHa (nr__) ! (0.1nm) ? H{alpha} line emission in Angstroms character*5 r_EWLi (nr__) ! Source of spectral information (16) *Note (1): * ROSAT All-Sky Survey Catalogue source name, in general from the Bright * Source Catalogue (<IX/10>) but sometimes refers to the Faint Source * Catalogue (<IX/29>). A repeated entry means more than one observed * possible optical counterpart. The same source may have entries in both * Tables 3 and 4, but the best optical candidate may be in any of the * tables. *Note (2): * Order of preference of the identification is Hipparcos, TYCHO-2 or * UCAC2, independently of the astrometric data used. *Note (3): * Order of preference is HD, DM, and other. GSC is only used if there is * no TYCHO-2 identification for the star. *Note (4): * Order of preference of the sources of the proper motions is the same * as of the Name, adding other sources, but in some cases we used the * best value from our judgment. *Note (5): * Radial velocities from SB2 observed once or SB1 are mean values, and * may not represent the systemic velocity. When there is a systemic * velocity from the literature, it is the used value. *Note (6): * Null refers to no published number of observations in the literature * cited in r_HRV. Nobs from SACY includes references N=25 and 26. *Note (7): * The * means that this is the number of spectral observations in the * SACY project, but the systemic HRV value was taken from the literature. * For V1005 Ori the non variable HRV is from literature as our spectrum * was not properly calibrated. *Note (8): * If there is no number, the radial velocity is from this work. *Note (9): * D means visual binary; sometimes the components were observed * separately and there is another entry, designated by A, B, C..., * in Table 3 or Table 4. If the bright component is also a SB the D * is given in the entry of the faint one. * * A ? means possible evidence for radial velocity variations, sometimes * by comparing with published data. In some cases it is difficult to * decide between high rotation (+ spots?) and SB2. For other SB2? with * low rotation and large e_HRV the star should be considered at least * a SB1. For close visual doubles observed together, one of the * spectroscopic components may be also the visual one, mainly in * SB3 cases. For SBn all other data of this line are for the bright * component. In the future we will publish the data for spectroscopic * binaries found in the SACY project. *Note (10): * Separation between the visual components, even if in n_HRV there is a * SBn. This means there is D for a faint companion in n_HRV in another * entry. *Note (11): * Magnitude difference between faint companions and the bright one. A * negative value means that the faint companions together are brighter * than the primary, or the so called primary is a fainter companion with * sharper lines. * * For visual binaries the negative value means that primary is also a * SBn, and the visual difference is given in this entry or the primary * is in the other table. *Note (12): * V: photometric variability. *Note (13): Source of photometry: * H = origin of the photometry from Hipparcos (<I/239>) * T = from TYCHO2 (<I/259>) converted to Johnson * blank = estimated magnitude *Note (14): * for the proposes of the SACY the photometric measures for close visual * doubles and SBs are corrected to take into account the secondaries. As * these values are model dependent they must be used with caution. *Note (15): * For SB2 or SB3 the values are tentatively corrected for the continuum * flux ratios. *Note (16): For observations from this paper: * F = observation with ESO/FEROS * d = observation with the OPD coude spectrograph c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table4.dat' ! Astrometric, spectroscopic and photometric data of other observed stars integer*4 nr__1 parameter (nr__1=165) ! Number of records character*228 ar__1 ! Full-size record C J2000.0 position composed of: RAh RAm RAs DE- DEd DEm DEs real*8 RAdeg_1 (nr__1) ! (deg) Right Ascension J2000.0 real*8 DEdeg_1 (nr__1) ! (deg) Declination J2000.0 C ---------------------------------- ! (position vector(s) in degrees) integer*4 Seq_1 (nr__1) ! Running number character*16 v1RXS_1 (nr__1) ! 1RXS (<IX/10>,<IX/29>) designation (1) character*16 Name_1 (nr__1) ! Hipparcos (<I/239>), Tycho-2 (<II/259>) or * UCAC2 (<I/289>) identification (2) character*13 OName_1 (nr__1) ! Other identification (HD, DM, other) (3) integer*4 RAh_1 (nr__1) ! (h) Right ascension (J2000.0) integer*4 RAm_1 (nr__1) ! (min) Right ascension (J2000.0) real*4 RAs_1 (nr__1) ! (s) Right ascension (J2000.0) character*1 DE__1 (nr__1) ! Declination sign (J2000.0) integer*4 DEd_1 (nr__1) ! (deg) Declination (J2000.0) integer*4 DEm_1 (nr__1) ! (arcmin) Declination (J2000.0) integer*4 DEs_1 (nr__1) ! (arcsec) Declination (J2000.0) real*8 pmRA_1 (nr__1) ! (mas/yr) Proper motion in RA (pmRA*cosDE) real*8 pmDE_1 (nr__1) ! (mas/yr) Proper motion in DE (pmDE) character*3 r_pmRA_1 (nr__1) ! Source of proper motions (4) real*4 HRV_1 (nr__1) ! (km/s) Heliocentric radial velocity (5) character*1 f_HRV_1 (nr__1) ! [:] Quality flag for RV real*4 e_HRV_1 (nr__1) ! (km/s) ? rms of the observed RV integer*4 Nobs_1 (nr__1) ! ? Number of observations (6) character*1 f_Nobs_1 (nr__1) ! [*] *: RV value comes from the literature (7) character*3 r_HRV_1 (nr__1) ! ? Source of radial velocity (8) character*5 n_HRV_1 (nr__1) ! [D,SB1234 ?] Multiplicity flag (9) real*4 Sep_1 (nr__1) ! (arcsec) ? Angular separation of visual binaries (10) real*4 dV_1 (nr__1) ! (mag) ? Magnitude difference of components (11) character*1 u_dV_1 (nr__1) ! [?] Uncertainty flag on dV real*4 vsini_1 (nr__1) ! (km/s) ? Rotational velocity real*4 e_vsini_1 (nr__1) ! (km/s) ? rms uncertainty on vsini character*3 r_vsini_1 (nr__1) ! ? Source of vsini (8) real*4 Plx_1 (nr__1) ! (mas) ? Trigonometric parallax real*4 e_Plx_1 (nr__1) ! (mas) ? Standard error in Plx character*3 r_Plx_1 (nr__1) ! Source of Plx (8) real*4 Vmag_1 (nr__1) ! (mag) Johnson V magnitude character*1 f_Vmag_1 (nr__1) ! [V] Quality flag indicating variability (12) real*4 B_V_1 (nr__1) ! (mag) ? Johnson B-V colour index real*4 V_I_1 (nr__1) ! (mag) ? Cousins V-I colour index character*3 r_Vmag_1 (nr__1) ! Source of photometry (13) character*1 n_Vmag_1 (nr__1) ! [*] *: photometry corrected for companions (14) character*8 SpType_1 (nr__1) ! MK spectral type integer*4 EWLi_1 (nr__1) ! (0.1pm) ? LiI equivalent width in milli-Angstroms (15) character*1 f_EWLi_1 (nr__1) ! [:?] Quality flag for EWLi real*4 EWHa_1 (nr__1) ! (0.1nm) ? H{alpha} line emission in Angstroms character*5 r_EWLi_1 (nr__1) ! Source of spectral information (16) *Note (1): * ROSAT All-Sky Survey Catalogue source name, in general from the Bright * Source Catalogue (<IX/10>) but sometimes refers to the Faint Source * Catalogue (<IX/29>). A repeated entry means more than one observed * possible optical counterpart. The same source may have entries in both * Tables 3 and 4, but the best optical candidate may be in any of the * tables. *Note (2): * Order of preference of the identification is Hipparcos, TYCHO-2 or * UCAC2, independently of the astrometric data used. *Note (3): * Order of preference is HD, DM, and other. GSC is only used if there is * no TYCHO-2 identification for the star. *Note (4): * Order of preference of the sources of the proper motions is the same * as of the Name, adding other sources, but in some cases we used the * best value from our judgment. *Note (5): * Radial velocities from SB2 observed once or SB1 are mean values, and * may not represent the systemic velocity. When there is a systemic * velocity from the literature, it is the used value. *Note (6): * Null refers to no published number of observations in the literature * cited in r_HRV. Nobs from SACY includes references N=25 and 26. *Note (7): * The * means that this is the number of spectral observations in the * SACY project, but the systemic HRV value was taken from the literature. * For V1005 Ori the non variable HRV is from literature as our spectrum * was not properly calibrated. *Note (8): * If there is no number, the radial velocity is from this work. *Note (9): * D means visual binary; sometimes the components were observed * separately and there is another entry, designated by A, B, C..., * in Table 3 or Table 4. If the bright component is also a SB the D * is given in the entry of the faint one. * * A ? means possible evidence for radial velocity variations, sometimes * by comparing with published data. In some cases it is difficult to * decide between high rotation (+ spots?) and SB2. For other SB2? with * low rotation and large e_HRV the star should be considered at least * a SB1. For close visual doubles observed together, one of the * spectroscopic components may be also the visual one, mainly in * SB3 cases. For SBn all other data of this line are for the bright * component. In the future we will publish the data for spectroscopic * binaries found in the SACY project. *Note (10): * Separation between the visual components, even if in n_HRV there is a * SBn. This means there is D for a faint companion in n_HRV in another * entry. *Note (11): * Magnitude difference between faint companions and the bright one. A * negative value means that the faint companions together are brighter * than the primary, or the so called primary is a fainter companion with * sharper lines. * * For visual binaries the negative value means that primary is also a * SBn, and the visual difference is given in this entry or the primary * is in the other table. *Note (12): * V: photometric variability. *Note (13): Source of photometry: * H = origin of the photometry from Hipparcos (<I/239>) * T = from TYCHO2 (<I/259>) converted to Johnson * blank = estimated magnitude *Note (14): * for the proposes of the SACY the photometric measures for close visual * doubles and SBs are corrected to take into account the secondaries. As * these values are model dependent they must be used with caution. *Note (15): * For SB2 or SB3 the values are tentatively corrected for the continuum * flux ratios. *Note (16): For observations from this paper: * F = observation with ESO/FEROS * d = observation with the OPD coude spectrograph c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'refs.dat' ! References (table5 of the paper) integer*4 nr__2 parameter (nr__2=107) ! Number of records character*96 ar__2 ! Full-size record character*3 Ref (nr__2) ! Reference number or letter character*19 BibCode (nr__2) ! BibCode character*24 Aut (nr__2) ! Author's name character*48 Com (nr__2) ! Comments C============================================================================= C Loading file 'table3.dat' ! Astrometric, spectroscopic and photometric data * of the SACY sample C Format for file interpretation 1 format( + I4,2X,A16,2X,A16,1X,A13,1X,I2,1X,I2,1X,F4.1,2X,A1,I2,1X,I2,1X, + I2,2X,F7.1,1X,F7.1,2X,A3,1X,F6.1,A1,1X,F4.1,1X,I3,A1,1X,A3,2X, + A5,1X,F4.1,2X,F4.1,A1,2X,F5.1,1X,F4.1,2X,A3,2X,F5.1,2X,F4.1, + 2X,A3,2X,F5.2,A1,F5.2,1X,F5.2,2X,A3,A1,3X,A8,1X,I3,A1,1X,F5.1, + 2X,A5) C Effective file loading open(unit=1,status='old',file= +'table3.dat') write(6,*) '....Loading file: table3.dat' do i__=1,1626 read(1,'(A228)')ar__ read(ar__,1) + Seq(i__),v1RXS(i__),Name(i__),OName(i__),RAh(i__),RAm(i__), + RAs(i__),DE_(i__),DEd(i__),DEm(i__),DEs(i__),pmRA(i__), + pmDE(i__),r_pmRA(i__),HRV(i__),f_HRV(i__),e_HRV(i__), + Nobs(i__),f_Nobs(i__),r_HRV(i__),n_HRV(i__),Sep(i__),dV(i__), + u_dV(i__),vsini(i__),e_vsini(i__),r_vsini(i__),Plx(i__), + e_Plx(i__),r_Plx(i__),Vmag(i__),f_Vmag(i__),B_V(i__),V_I(i__), + r_Vmag(i__),n_Vmag(i__),SpType(i__),EWLi(i__),f_EWLi(i__), + EWHa(i__),r_EWLi(i__) if(ar__(108:111) .EQ. '') e_HRV(i__) = rNULL__ if(ar__(113:115) .EQ. '') Nobs(i__) = iNULL__ if(ar__(129:132) .EQ. '') Sep(i__) = rNULL__ if(ar__(135:138) .EQ. '') dV(i__) = rNULL__ if(ar__(142:146) .EQ. '') vsini(i__) = rNULL__ if(ar__(148:151) .EQ. '') e_vsini(i__) = rNULL__ if(ar__(159:163) .EQ. '') Plx(i__) = rNULL__ if(ar__(166:169) .EQ. '') e_Plx(i__) = rNULL__ if(ar__(183:187) .EQ. '') B_V(i__) = rNULL__ if(ar__(189:193) .EQ. '') V_I(i__) = rNULL__ if(ar__(212:214) .EQ. '') EWLi(i__) = iNULL__ if(ar__(217:221) .EQ. '') EWHa(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) + Seq(i__),v1RXS(i__),Name(i__),OName(i__),RAh(i__),RAm(i__), + RAs(i__),DE_(i__),DEd(i__),DEm(i__),DEs(i__),pmRA(i__), + pmDE(i__),r_pmRA(i__),HRV(i__),f_HRV(i__),e_HRV(i__), + Nobs(i__),f_Nobs(i__),r_HRV(i__),n_HRV(i__),Sep(i__),dV(i__), + u_dV(i__),vsini(i__),e_vsini(i__),r_vsini(i__),Plx(i__), + e_Plx(i__),r_Plx(i__),Vmag(i__),f_Vmag(i__),B_V(i__),V_I(i__), + r_Vmag(i__),n_Vmag(i__),SpType(i__),EWLi(i__),f_EWLi(i__), + EWHa(i__),r_EWLi(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 'table4.dat' ! Astrometric, spectroscopic and photometric data * of other observed stars C Format for file interpretation 2 format( + I4,2X,A16,2X,A16,1X,A13,1X,I2,1X,I2,1X,F4.1,2X,A1,I2,1X,I2,1X, + I2,2X,F7.1,1X,F7.1,2X,A3,1X,F6.1,A1,1X,F4.1,1X,I3,A1,1X,A3,2X, + A5,1X,F4.1,2X,F4.1,A1,2X,F5.1,1X,F4.1,2X,A3,2X,F5.1,2X,F4.1, + 2X,A3,2X,F5.2,A1,F5.2,1X,F5.2,2X,A3,A1,3X,A8,1X,I3,A1,1X,F5.1, + 2X,A5) C Effective file loading open(unit=1,status='old',file= +'table4.dat') write(6,*) '....Loading file: table4.dat' do i__=1,165 read(1,'(A228)')ar__1 read(ar__1,2) + Seq_1(i__),v1RXS_1(i__),Name_1(i__),OName_1(i__),RAh_1(i__), + RAm_1(i__),RAs_1(i__),DE__1(i__),DEd_1(i__),DEm_1(i__), + DEs_1(i__),pmRA_1(i__),pmDE_1(i__),r_pmRA_1(i__),HRV_1(i__), + f_HRV_1(i__),e_HRV_1(i__),Nobs_1(i__),f_Nobs_1(i__), + r_HRV_1(i__),n_HRV_1(i__),Sep_1(i__),dV_1(i__),u_dV_1(i__), + vsini_1(i__),e_vsini_1(i__),r_vsini_1(i__),Plx_1(i__), + e_Plx_1(i__),r_Plx_1(i__),Vmag_1(i__),f_Vmag_1(i__), + B_V_1(i__),V_I_1(i__),r_Vmag_1(i__),n_Vmag_1(i__), + SpType_1(i__),EWLi_1(i__),f_EWLi_1(i__),EWHa_1(i__), + r_EWLi_1(i__) if(ar__1(108:111) .EQ. '') e_HRV_1(i__) = rNULL__ if(ar__1(113:115) .EQ. '') Nobs_1(i__) = iNULL__ if(ar__1(129:132) .EQ. '') Sep_1(i__) = rNULL__ if(ar__1(135:138) .EQ. '') dV_1(i__) = rNULL__ if(ar__1(142:146) .EQ. '') vsini_1(i__) = rNULL__ if(ar__1(148:151) .EQ. '') e_vsini_1(i__) = rNULL__ if(ar__1(159:163) .EQ. '') Plx_1(i__) = rNULL__ if(ar__1(166:169) .EQ. '') e_Plx_1(i__) = rNULL__ if(ar__1(183:187) .EQ. '') B_V_1(i__) = rNULL__ if(ar__1(189:193) .EQ. '') V_I_1(i__) = rNULL__ if(ar__1(212:214) .EQ. '') EWLi_1(i__) = iNULL__ if(ar__1(217:221) .EQ. '') EWHa_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) + Seq_1(i__),v1RXS_1(i__),Name_1(i__),OName_1(i__),RAh_1(i__), + RAm_1(i__),RAs_1(i__),DE__1(i__),DEd_1(i__),DEm_1(i__), + DEs_1(i__),pmRA_1(i__),pmDE_1(i__),r_pmRA_1(i__),HRV_1(i__), + f_HRV_1(i__),e_HRV_1(i__),Nobs_1(i__),f_Nobs_1(i__), + r_HRV_1(i__),n_HRV_1(i__),Sep_1(i__),dV_1(i__),u_dV_1(i__), + vsini_1(i__),e_vsini_1(i__),r_vsini_1(i__),Plx_1(i__), + e_Plx_1(i__),r_Plx_1(i__),Vmag_1(i__),f_Vmag_1(i__), + B_V_1(i__),V_I_1(i__),r_Vmag_1(i__),n_Vmag_1(i__), + SpType_1(i__),EWLi_1(i__),f_EWLi_1(i__),EWHa_1(i__), + r_EWLi_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 'refs.dat' ! References (table5 of the paper) C Format for file interpretation 3 format(A3,1X,A19,1X,A24,A48) C Effective file loading open(unit=1,status='old',file= +'refs.dat') write(6,*) '....Loading file: refs.dat' do i__=1,107 read(1,'(A96)')ar__2 read(ar__2,3)Ref(i__),BibCode(i__),Aut(i__),Com(i__) c ..............Just test output........... write(6,3)Ref(i__),BibCode(i__),Aut(i__),Com(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= stop end