Conversion of standardized ReadMe file for
file /./ftp/cats/III/198 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-18
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. III/198 Palomar/MSU nearby star spectroscopic survey (Hawley+ 1997)
*================================================================================
*The Palomar/MSU nearby star spectroscopic survey.
*I. The northern M dwarfs-band strengths and kinematics.
* Reid I.N., Hawley S.L., Gizis J.E.
* <Astron. J. 110, 1838 (1995) ; Erratum Vol. 111, 2469 (1996)>
* =1995AJ....110.1838R
*II. The southern M dwarfs and investigations of magnetic activity.
* Hawley S.L., Gizis J.E., Reid I.N.
* <Astron. J. 112, 2799 (1996) ; Erratum Vol. 113, 1458 (1997)>
* =1996AJ....112.2799H
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'main.dat' ! Basic data (tables 1a of both papers, and table 1d
from paper I for Star numbers 3804-3810)
integer*4 nr__
parameter (nr__=1971) ! Number of records
character*80 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*1 Sam (nr__) ! [ns] n=North (paper I), s=South (paper II)
integer*4 CNS3 (nr__) ! [1/3810]+= Star number (row in CNS3) (8)
character*13 Name (nr__) ! Star name (1)
character*2 n_Name (nr__) ! [abc eghijk*] Individual Note (2)
character*1 Bin (nr__) ! [ps] Primary or secondary binary comp. (3)
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
integer*4 DEd (nr__) ! (deg) Declination, J2000
integer*4 DEm (nr__) ! (arcmin) Declination, J2000
integer*4 DEs (nr__) ! (arcsec) Declination, J2000
integer*4 Src (nr__) ! [0/4] Source of positional data (G1)
real*4 VMag (nr__) ! (mag) Absolute V magnitude
character*1 n_VMag (nr__) ! [ab] Note about ptg/ptm origin of VMag (5)
real*4 r (nr__) ! (pc) Distance (6)
integer*4 e_r (nr__) ! (%) Distance uncertainty (6)
character*1 Dist (nr__) ! [CSp ] Origin of r & M_V_ (9)
integer*4 wPi (nr__) ! (%) ? Weight for trigonometric parallax
integer*4 wSp (nr__) ! (%) ? Weight for spectroscopic parallax
character*1 f_Sp (nr__) ! Limit sign (<>) on Sp, or sd luminosity class
character*5 Sp (nr__) ! Spectral type (may include sd luminosity class)
character*1 n_Sp (nr__) ! [cdfk] Note about the spectrum (7)
*Note (1): Lists are abbreviated as:
* Gl = Gliese (1969, Veroff. Astr. Rechen-Instituts, Heidelberg, Nr. 22)
* GJ = Gliese & Jahreiss =1979A&AS...38..423G
* Wo = Woolley et al (1970, R. Obs. Ann., No. 5) =Cat. <V/32>
* LHS = Luyten Half-Second Catalogue =Cat. <I/87>
* LTT = Luyten Two-Tenths Catalogue
* LP = Luyten Palomar proper-motion catalogue
* G = Giclas et al (1971, Lowell Proper Motion Survey) =Cat. <I/79>
* GR = Giclas et al (1971) red star (see =1980LowOB...8..157G)
* GH = Giclas et al (1971) Hyades star (see =1962LowOB...5..257G)
* (Nomenclature note: should be named "HG")
* Rob = Robertson (should be named RBTS) =1984AJ.....89.1229R
* Steph = Stephenson (1986, AJ, 91, 137) =Cat. <III/123>
* (Nomenclature note: should be named "StKM")
* PS = Pesch & Sanduleak =1978AJ.....83.1090P
* San = Sanduleak =1976AJ.....81..350S
* vA = van Altena =1969AJ.....74....2V
* V = Vyssotsky (1963, Stars and Stellar Systems III, Basic Astronomical Data,
* edited by K. Aa Strand; University of Chicago Press, Chicago; p. 192)
* (Nomemclature Note: should be named MCC =Cat. <III/13>)
*Note (2): Flags as follows:
* a = Low quality trigonometric parallax
* b = Poor photometry
* c = Accurate parallax and good photometry. Both components of Gl 799
* lie above the main-sequence.
* e = 629 (Hy 207) appears twice in the preliminary version of the CNS3
* g = 2172: This star is not listed as double in the LHS
* h = 2426 (GJ 2112 A): Eggen (1980ApJS...43..457E) notes that this
* star appears to be a double in good seeing, but there are no
* confirming observations.
* i = 2805 (GSC036B-821) is listed in the CNS3 as a companion of V796,
* but the authors find that the radial velocity differs by 50km/s
* j = star from Brosch & Goldberg (1994MNRAS.268L..27B)
* k = star from Irwin et al. (1991MNRAS.252p..61I)
* * = star position corrected at CDS (see also the file "errata.htx")
*Note (3): Components in a binary system are identified as
* p (primary) or s (secondary, tertiary).
*Note (5): Flag as follows:
* a = CNS3 lists a photographic magnitude - the authors assumed an
* (m(pg)-V) colour of 1.5 magnitudes
* b = CNS3 lists a `photometric' magnitude for this star
*Note (6): Distance and estimated uncertainty (%) from the authors' data, using
* a weighted combination of trigonometric and spectroscopic parallaxes.
*Note (7): Flag as follows:
* c = Spectral type from Kirkpatrick et al (1995AJ....109..797K)
* d = Strong CaH - probable metal-poor disk dwarf or halo subdwarf
* f = 1752: Leggett & Hawkins (1988MNRAS.234.1065L) suggest, on the
* basis of JHK colours, that this star might be a giant, but our
* spectra are consistent with classification as a dwarf. Note that
* the V magnitude listed by LH88 is 8.07, while the CNS3 magnitude
* is 11.4 (photometric estimate). The authors observed a star of
* the latter magnitude. There is a nearby 8th magnitude SAO star
* (SAO 7382) - listed as K5, luminosity class unknown but {mu}~0"/yr
* which Leggett & Hawkins may have observed by mistake.
* k = Spectral type from Kirkpatrick et al. (1995AJ....109..797K)
*Note (8): Numbers 3804 to 3810 are the additional stars from
* table 1d in paper I.
*Note (9): Origin of distance and absolute magnitude as follows:
* C = distance and absolute magnitude from CNS3
* S = distance estimate is based on the authors' spectroscopic data
* p = Distance estimate is based on trigonometric parallax
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'binary.dat' ! Inaccessible binary companions (tables 1b)
integer*4 nr__1
parameter (nr__1=142) ! Number of records
character*70 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*1 Sam_1 (nr__1) ! [ns] n=North (paper I), s=South (paper II)
integer*4 CNS3_1 (nr__1) ! [1/3803]+= Star number (row number in CNS3)
character*10 Name_1 (nr__1) ! Star name, references same as main.dat
character*1 n_Name_1 (nr__1) ! [cdef] Individual Note (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
integer*4 DEd_1 (nr__1) ! (deg) Declination, J2000
integer*4 DEm_1 (nr__1) ! (arcmin) Declination, J2000
integer*4 DEs_1 (nr__1) ! (arcsec) Declination, J2000
integer*4 Src_1 (nr__1) ! [0/4] Source of position, as in main.dat (G1)
real*4 VMag_1 (nr__1) ! (mag) Absolute V magnitude (2)
character*1 n_VMag_1 (nr__1) ! [ab] a=ptg, b=ptm VMag estimate (3)
real*4 r_1 (nr__1) ! (pc) Distance (4)
integer*4 e_r_1 (nr__1) ! (%) Distance uncertainty (4)
real*4 Vmag1 (nr__1) ! (mag) Magnitude of primary star in the system
real*4 dV (nr__1) ! (mag) Magnitude difference
character*1 l_dP (nr__1) ! [~] Limit flag on dP
real*4 dP (nr__1) ! (arcsec) Separation
*Note (1): Flag as follows:
* c = Gl 452B (1863) is listed as an f-type companion to Gl 452A, 7.5
* magnitudes fainter and ~15 arcseconds distant. We were unable to
* locate this star on the TV guider (r_lim_ ~21) of the Keck telescope.
* d = The companion to LHS 2789 (2172) is listed in the LTT, but not in
* the LHS and may not exist
* e = Known VLM companion - Forrest et al., (1988ApJ...330L.119F)
* f = Eggen (1980ApJS...43..457E) noted that the primary star appeared
* double in good seeing, but there is no strong evidence for a
* binary companion.
*Note (2): Absolute magnitudes have been calculated using the magnitudes
* listed in the CNS3 and the distance estimate to the primary star
* (either from CNS3 or main file)
*Note (3):
* a = CNS3 lists a photographic magnitude
* b = CNS3 lists a 'photometric' magnitude estimate
*Note (4): Distance and estimated uncertainty (%) from the authors' data,
* using a weighted combination of trigonometric and spectroscopic parallaxes.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'notobs.dat' ! Stars not observed (table 1d, paper II)
integer*4 nr__2
parameter (nr__2=21) ! Number of records
character*55 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)
integer*4 CNS3_2 (nr__2) ! [1/3803] Star number (row number in CNS3)
character*9 Name_2 (nr__2) ! Star name
character*1 n_Name_2 (nr__2) ! [ab] Individual note (1)
character*1 Bin_1 (nr__2) ! [ps] Primary or secondary binary component
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
integer*4 DEd_2 (nr__2) ! (deg) Declination, J2000
integer*4 DEm_2 (nr__2) ! (arcmin) Declination, J2000
integer*4 DEs_2 (nr__2) ! (arcsec) Declination, J2000
integer*4 Src_2 (nr__2) ! [0/4] Source of position, as in main.dat (G1)
real*4 VMag_2 (nr__2) ! (mag) Absolute V magnitude
real*4 r_2 (nr__2) ! (pc) Distance
integer*4 e_r_2 (nr__2) ! (%) Distance uncertainty
*Note (1): Flag as follows:
* a = Gl 127.1B probably does not exist. Gliese (1969, Veroff. Astr.
* Rechen-Instituts, Heidelberg, Nr. 22) lists a 'red companion at 8
* arcseconds', but no companion brighter than R~17 was visible with the
* LCO Du Pont telescope. Bessell (1990A&AS...83..357B) lists colours of
* (B-V)=0.615, (V-I)=0.70, suggesting either a white dwarf companion or
* observations of a background star.
* b = Our spectrum indicates that this star is an M-dwarf, but the
* 6th magnitude primary, CP-73 2192, at 8 arcseconds distance prevents
* accurate bandstrength measurements.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'early.dat' ! Early-type stars, giants and degenerates (tables 1c)
integer*4 nr__3
parameter (nr__3=98) ! Number of records
character*74 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*1 Sam_2 (nr__3) ! [ns] n=North (paper I), s=South (paper II)
integer*4 CNS3_3 (nr__3) ! [1/3803]+ Star number (row number in CNS3)
character*14 Name_3 (nr__3) ! Star name, references same as main.dat
character*1 f_Name (nr__3) ! [e] Possible error flag (4)
character*1 Bin_2 (nr__3) ! [ps] Primary or secondary binary comp. (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
integer*4 DEd_3 (nr__3) ! (deg) Declination, J2000
integer*4 DEm_3 (nr__3) ! (arcmin) Declination, J2000
integer*4 DEs_3 (nr__3) ! (arcsec) Declination, J2000
integer*4 Src_3 (nr__3) ! [0/4] Source of position, as in main.dat (G1)
real*4 Vmag_3 (nr__3) ! (mag) V magnitude from the CNS3
real*4 VMag_4 (nr__3) ! (mag) Absolute V magnitude (2)
character*3 n_r (nr__3) ! [abcd fg] Note about distance (4)
integer*4 r_3 (nr__3) ! (pc) Distance
character*7 Sp_1 (nr__3) ! Spectral type
character*1 Note (nr__3) ! [def] Additional notes (5)
*Note (1): Components in a binary system are identified as
* p (primary) or s (secondary, tertiary).
*Note (2): absolute magnitudes are derived:
* * In North, using Reid & Murray's (1992AJ....103..514R) (M_V_, (B-V))
* relation unless otherwise indicated.
* * In South, from (B-V) colours listed in the CNS3 unless otherwise indicated.
*Note (4): Flag as follows:
* a = distance estimated from spectral type;
* b = distance estimated based on companion star;
* c = spectral types suggest that these stars are not associated
* with the nominal primary star.
* d = distance from CNS3
* e = listed in the LHS as proper motion companion to LHS 2405
* (I/87 main file); it is possible that we have observed the wrong star
* f = FS Comae: distance based on Jura & Kleinmann's (1992ApJS...83..329J) M_K_
* g = distance from McCook & Sion (1987ApJS...65..603M) (M_V_, B-V) relations
*Note (5): Flag as follows:
* d = 757: foreground reddening probably present
* e = Gl 288B is the well-known low-luminosity white dwarf, van Biesbroeck 3
* f = Gl 432B is the well-known low-luminosity white dwarf, van Biesbroeck 4
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'spectro.dat' ! Bandstrengths (table 3 of paper I and
table 2 of paper II)
integer*4 nr__4
parameter (nr__4=2008) ! Number of records
character*57 ar__4 ! Full-size record
character*1 Sam_3 (nr__4) ! [ns] n=North (paper I), s=South (paper II)
integer*4 CNS3_4 (nr__4) ! [1/3810]+= Star number (row number in CNS3)
character*1 m_CNS3 (nr__4) ! Multiplicity index on star
real*4 TiO1 (nr__4) ! ? TiO1 index: F(6718-6723)/F(6703-6708)
real*4 TiO2 (nr__4) ! ? TiO2 index: F(7058-7061)/F(7043-7046)
real*4 TiO3 (nr__4) ! ? TiO3 index: F(7092-7097)/F(7079-7084)
real*4 TiO4 (nr__4) ! ? TiO4 index: F(7130-7135)/F(7115-7120)
real*4 TiO5 (nr__4) ! ? TiO5 index: F(7126-7135)/F(7042-7046)
real*4 CaH1 (nr__4) ! ? CaH1 index: F(6380-6390)/F(6345-6355,6410-6420))
real*4 CaH2 (nr__4) ! ? CaH2 index: F(6814-6846)/F(7042-7046)
real*4 CaH3 (nr__4) ! ? CaH3 index: F(6960-6990)/F(7042-7046)
real*4 CaOH (nr__4) ! ? CaOH index: F(6230-6240)/F(6345-6354)
real*4 Halpha (nr__4) ! ? H-{alpha} index: F(6560-6566)/F(6545-6555)
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'vel.dat' ! Radial velocities and space motions
(table 5 of paper I and table 3 of paper II)
integer*4 nr__5
parameter (nr__5=1971) ! Number of records
character*51 ar__5 ! Full-size record
character*1 Sam_4 (nr__5) ! [ns] n=North (paper I), s=South (paper II)
integer*4 CNS3_5 (nr__5) ! [1/3810]+= Star number (row number in CNS3)
character*1 m_CNS3_1 (nr__5) ! Multiplicity index on star
real*4 pmRA (nr__5) ! (arcsec/yr) ? Proper motion in right ascension, from CNS3
real*4 pmDE (nr__5) ! (arcsec/yr) ? Proper motion in declination, from CNS3
real*8 RV (nr__5) ! (km/s) ? Radial velocity
character*1 Note_1 (nr__5) ! [*] If no proper motions are available
integer*4 U (nr__5) ! (km/s) ? U space velocity
integer*4 V (nr__5) ! (km/s) ? V space velocity
integer*4 W (nr__5) ! (km/s) ? W space velocity
real*4 VMag_5 (nr__5) ! (mag) Absolute V magnitude (from main.dat)
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'dmestar.dat' ! Photometric and spectroscopic data for dMe stars
(table 4a of paper II)
integer*4 nr__6
parameter (nr__6=321) ! Number of records
character*83 ar__6 ! Full-size record
integer*4 CNS3_6 (nr__6) ! [1/3803]+ Star number (row number in CNS3)
real*4 Halp (nr__6) ! ? H-{alpha} index: F(6560-6566)/F(6545-6555)
real*4 TiO2_1 (nr__6) ! ? TiO2 index: F(7058-7061)/F(7043-7046)
real*4 TiO4_1 (nr__6) ! ? TiO4 index: F(7130-7135)/F(7115-7120)
real*4 TiO5_1 (nr__6) ! ? TiO5 index: F(7126-7135)/F(7042-7046)
real*4 Sp_2 (nr__6) ! Spectral type
real*4 Mv (nr__6) ! (mag) Absolute V magnitude
real*4 Vmag_6 (nr__6) ! (mag) V magnitude
real*4 R_I (nr__6) ! (mag) ? R-I colour index
real*4 V_I (nr__6) ! (mag) ? V-I colour index
integer*4 r_V_I (nr__6) ! ? Reference for VRI photometry
real*4 V_K (nr__6) ! (mag) ? V-K colour index
real*4 S_Hb (nr__6) ! (10-13mW/m2) ? H{beta} flux
real*4 S_Ha__S_Hb (nr__6) ! ? H{alpha} versus H{beta} flux ratio
real*4 log_L_Ha__Lbol(nr__6) ! ? H{alpha} vs. bolometric luminosity ratio
real*4 Mbol (nr__6) ! (mag) ? Bolometric magnitude
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'hyades.dat' ! Photometric and spectroscopic data for
Hyades stars (table 4b of paper II)
integer*4 nr__7
parameter (nr__7=25) ! Number of records
character*68 ar__7 ! Full-size record
integer*4 CNS3_7 (nr__7) ! [1/3803]+ Star number (row number in CNS3)
real*4 Halp_1 (nr__7) ! ? H-{alpha} index: F(6560-6566)/F(6545-6555)
real*4 TiO2_2 (nr__7) ! ? TiO2 index: F(7058-7061)/F(7043-7046)
real*4 TiO4_2 (nr__7) ! ? TiO4 index: F(7130-7135)/F(7115-7120)
real*4 TiO5_2 (nr__7) ! ? TiO5 index: F(7126-7135)/F(7042-7046)
real*4 Sp_3 (nr__7) ! Spectral type
real*4 Mv_1 (nr__7) ! (mag) Absolute V magnitude
real*4 Vmag_7 (nr__7) ! (mag) V magnitude
real*4 V_I_1 (nr__7) ! (mag) ? V-I colour index
real*4 log_L_Ha__Lbol_1(nr__7) ! ? H{alpha} versus bolometric luminosity ratio
real*4 log_LX_Lbol(nr__7) ! ? X-ray versus bolometric luminosity ratio
real*4 Mbol_1 (nr__7) ! (mag) ? Bolometric magnitude
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'ic2602.dat' ! Photometric and spectroscopic data for
IC 2602 stars (table 4c of paper II)
integer*4 nr__8
parameter (nr__8=26) ! Number of records
character*68 ar__8 ! Full-size record
integer*4 CNS3_8 (nr__8) ! [1/3803]+ Star number (row number in CNS3)
real*4 Halp_2 (nr__8) ! ? H-{alpha} index: F(6560-6566)/F(6545-6555)
real*4 TiO2_3 (nr__8) ! ? TiO2 index: F(7058-7061)/F(7043-7046)
real*4 TiO4_3 (nr__8) ! ? TiO4 index: F(7130-7135)/F(7115-7120)
real*4 TiO5_3 (nr__8) ! ? TiO5 index: F(7126-7135)/F(7042-7046)
real*4 Sp_4 (nr__8) ! Spectral type
real*4 Mv_2 (nr__8) ! (mag) Absolute V magnitude
real*4 Vmag_8 (nr__8) ! (mag) V magnitude
real*4 V_I_2 (nr__8) ! (mag) ? V-I colour index
real*4 log_L_Ha__Lbol_1(nr__8) ! ? H{alpha} versus bolometric luminosity ratio
real*4 log_LX_Lbol_1(nr__8) ! ? X-ray versus bolometric luminosity ratio
real*4 Mbol_2 (nr__8) ! (mag) ? Bolometric magnitude
C=============================================================================
C Loading file 'main.dat' ! Basic data (tables 1a of both papers, and table 1d
* from paper I for Star numbers 3804-3810)
C Format for file interpretation
1 format(
+ A1,I4,1X,A13,2X,A2,1X,A1,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,
+ 1X,I2,1X,I1,1X,F5.2,A1,F5.1,1X,I2,A1,I3,1X,I3,2X,A1,A5,A1)
C Effective file loading
open(unit=1,status='old',file=
+'main.dat')
write(6,*) '....Loading file: main.dat'
do i__=1,1971
read(1,'(A80)')ar__
read(ar__,1)
+ Sam(i__),CNS3(i__),Name(i__),n_Name(i__),Bin(i__),RAh(i__),
+ RAm(i__),RAs(i__),DE_(i__),DEd(i__),DEm(i__),DEs(i__),
+ Src(i__),VMag(i__),n_VMag(i__),r(i__),e_r(i__),Dist(i__),
+ wPi(i__),wSp(i__),f_Sp(i__),Sp(i__),n_Sp(i__)
if(ar__(65:67) .EQ. '') wPi(i__) = iNULL__
if(ar__(69:71) .EQ. '') wSp(i__) = iNULL__
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)
+ Sam(i__),CNS3(i__),Name(i__),n_Name(i__),Bin(i__),RAh(i__),
+ RAm(i__),RAs(i__),DE_(i__),DEd(i__),DEm(i__),DEs(i__),
+ Src(i__),VMag(i__),n_VMag(i__),r(i__),e_r(i__),Dist(i__),
+ wPi(i__),wSp(i__),f_Sp(i__),Sp(i__),n_Sp(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 'binary.dat' ! Inaccessible binary companions (tables 1b)
C Format for file interpretation
2 format(
+ A1,I4,1X,A10,1X,A1,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,I2,
+ 1X,I1,1X,F4.1,A1,1X,F4.1,1X,I2,1X,F4.1,1X,F4.1,A1,F4.1)
C Effective file loading
open(unit=1,status='old',file=
+'binary.dat')
write(6,*) '....Loading file: binary.dat'
do i__=1,142
read(1,'(A70)')ar__1
read(ar__1,2)
+ Sam_1(i__),CNS3_1(i__),Name_1(i__),n_Name_1(i__),RAh_1(i__),
+ RAm_1(i__),RAs_1(i__),DE__1(i__),DEd_1(i__),DEm_1(i__),
+ DEs_1(i__),Src_1(i__),VMag_1(i__),n_VMag_1(i__),r_1(i__),
+ e_r_1(i__),Vmag1(i__),dV(i__),l_dP(i__),dP(i__)
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)
+ Sam_1(i__),CNS3_1(i__),Name_1(i__),n_Name_1(i__),RAh_1(i__),
+ RAm_1(i__),RAs_1(i__),DE__1(i__),DEd_1(i__),DEm_1(i__),
+ DEs_1(i__),Src_1(i__),VMag_1(i__),n_VMag_1(i__),r_1(i__),
+ e_r_1(i__),Vmag1(i__),dV(i__),l_dP(i__),dP(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 'notobs.dat' ! Stars not observed (table 1d, paper II)
C Format for file interpretation
3 format(
+ I4,1X,A9,1X,A1,1X,A1,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,I2,
+ 1X,I1,1X,F5.2,1X,F4.1,1X,I2)
C Effective file loading
open(unit=1,status='old',file=
+'notobs.dat')
write(6,*) '....Loading file: notobs.dat'
do i__=1,21
read(1,'(A55)')ar__2
read(ar__2,3)
+ CNS3_2(i__),Name_2(i__),n_Name_2(i__),Bin_1(i__),RAh_2(i__),
+ RAm_2(i__),RAs_2(i__),DE__2(i__),DEd_2(i__),DEm_2(i__),
+ DEs_2(i__),Src_2(i__),VMag_2(i__),r_2(i__),e_r_2(i__)
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)
+ CNS3_2(i__),Name_2(i__),n_Name_2(i__),Bin_1(i__),RAh_2(i__),
+ RAm_2(i__),RAs_2(i__),DE__2(i__),DEd_2(i__),DEm_2(i__),
+ DEs_2(i__),Src_2(i__),VMag_2(i__),r_2(i__),e_r_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 'early.dat' ! Early-type stars, giants and degenerates (tables 1c)
C Format for file interpretation
4 format(
+ A1,I4,1X,A14,A1,A1,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,I2,
+ 1X,I1,1X,F5.2,1X,F5.2,A3,1X,I4,1X,A7,A1)
C Effective file loading
open(unit=1,status='old',file=
+'early.dat')
write(6,*) '....Loading file: early.dat'
do i__=1,98
read(1,'(A74)')ar__3
read(ar__3,4)
+ Sam_2(i__),CNS3_3(i__),Name_3(i__),f_Name(i__),Bin_2(i__),
+ RAh_3(i__),RAm_3(i__),RAs_3(i__),DE__3(i__),DEd_3(i__),
+ DEm_3(i__),DEs_3(i__),Src_3(i__),Vmag_3(i__),VMag_4(i__),
+ n_r(i__),r_3(i__),Sp_1(i__),Note(i__)
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)
+ Sam_2(i__),CNS3_3(i__),Name_3(i__),f_Name(i__),Bin_2(i__),
+ RAh_3(i__),RAm_3(i__),RAs_3(i__),DE__3(i__),DEd_3(i__),
+ DEm_3(i__),DEs_3(i__),Src_3(i__),Vmag_3(i__),VMag_4(i__),
+ n_r(i__),r_3(i__),Sp_1(i__),Note(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_3(i__),DEdeg_3(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'spectro.dat' ! Bandstrengths (table 3 of paper I and
* table 2 of paper II)
C Format for file interpretation
5 format(
+ A1,I4,A1,1X,F4.2,1X,F4.2,1X,F4.2,1X,F4.2,1X,F4.2,1X,F4.2,1X,
+ F4.2,1X,F4.2,1X,F4.2,1X,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'spectro.dat')
write(6,*) '....Loading file: spectro.dat'
do i__=1,2008
read(1,'(A57)')ar__4
read(ar__4,5)
+ Sam_3(i__),CNS3_4(i__),m_CNS3(i__),TiO1(i__),TiO2(i__),
+ TiO3(i__),TiO4(i__),TiO5(i__),CaH1(i__),CaH2(i__),CaH3(i__),
+ CaOH(i__),Halpha(i__)
if(ar__4(8:11) .EQ. '') TiO1(i__) = rNULL__
if(ar__4(13:16) .EQ. '') TiO2(i__) = rNULL__
if(ar__4(18:21) .EQ. '') TiO3(i__) = rNULL__
if(ar__4(23:26) .EQ. '') TiO4(i__) = rNULL__
if(ar__4(28:31) .EQ. '') TiO5(i__) = rNULL__
if(ar__4(33:36) .EQ. '') CaH1(i__) = rNULL__
if(ar__4(38:41) .EQ. '') CaH2(i__) = rNULL__
if(ar__4(43:46) .EQ. '') CaH3(i__) = rNULL__
if(ar__4(48:51) .EQ. '') CaOH(i__) = rNULL__
if(ar__4(53:57) .EQ. '') Halpha(i__) = rNULL__
c ..............Just test output...........
write(6,5)
+ Sam_3(i__),CNS3_4(i__),m_CNS3(i__),TiO1(i__),TiO2(i__),
+ TiO3(i__),TiO4(i__),TiO5(i__),CaH1(i__),CaH2(i__),CaH3(i__),
+ CaOH(i__),Halpha(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'vel.dat' ! Radial velocities and space motions
* (table 5 of paper I and table 3 of paper II)
C Format for file interpretation
6 format(
+ A1,I4,A1,1X,F6.3,1X,F6.3,1X,F7.1,1X,A1,I5,1X,I4,1X,I4,1X,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'vel.dat')
write(6,*) '....Loading file: vel.dat'
do i__=1,1971
read(1,'(A51)')ar__5
read(ar__5,6)
+ Sam_4(i__),CNS3_5(i__),m_CNS3_1(i__),pmRA(i__),pmDE(i__),
+ RV(i__),Note_1(i__),U(i__),V(i__),W(i__),VMag_5(i__)
if(ar__5(8:13) .EQ. '') pmRA(i__) = rNULL__
if(ar__5(15:20) .EQ. '') pmDE(i__) = rNULL__
if(ar__5(22:28) .EQ. '') RV(i__) = rNULL__
if(ar__5(31:35) .EQ. '') U(i__) = iNULL__
if(ar__5(37:40) .EQ. '') V(i__) = iNULL__
if(ar__5(42:45) .EQ. '') W(i__) = iNULL__
c ..............Just test output...........
write(6,6)
+ Sam_4(i__),CNS3_5(i__),m_CNS3_1(i__),pmRA(i__),pmDE(i__),
+ RV(i__),Note_1(i__),U(i__),V(i__),W(i__),VMag_5(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'dmestar.dat' ! Photometric and spectroscopic data for dMe stars
* (table 4a of paper II)
C Format for file interpretation
7 format(
+ I4,1X,F5.2,1X,F4.2,1X,F4.2,1X,F4.2,1X,F4.1,1X,F5.2,1X,F5.2,1X,
+ F4.2,1X,F4.2,1X,I1,1X,F4.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'dmestar.dat')
write(6,*) '....Loading file: dmestar.dat'
do i__=1,321
read(1,'(A83)')ar__6
read(ar__6,7)
+ CNS3_6(i__),Halp(i__),TiO2_1(i__),TiO4_1(i__),TiO5_1(i__),
+ Sp_2(i__),Mv(i__),Vmag_6(i__),R_I(i__),V_I(i__),r_V_I(i__),
+ V_K(i__),S_Hb(i__),S_Ha__S_Hb(i__),log_L_Ha__Lbol(i__),
+ Mbol(i__)
if(ar__6(6:10) .EQ. '') Halp(i__) = rNULL__
if(ar__6(12:15) .EQ. '') TiO2_1(i__) = rNULL__
if(ar__6(17:20) .EQ. '') TiO4_1(i__) = rNULL__
if(ar__6(22:25) .EQ. '') TiO5_1(i__) = rNULL__
if(ar__6(44:47) .EQ. '') R_I(i__) = rNULL__
if(ar__6(49:52) .EQ. '') V_I(i__) = rNULL__
if(ar__6(54:54) .EQ. '') r_V_I(i__) = iNULL__
if(ar__6(56:59) .EQ. '') V_K(i__) = rNULL__
if(ar__6(61:65) .EQ. '') S_Hb(i__) = rNULL__
if(ar__6(67:71) .EQ. '') S_Ha__S_Hb(i__) = rNULL__
if(ar__6(73:77) .EQ. '') log_L_Ha__Lbol(i__) = rNULL__
if(ar__6(79:83) .EQ. '') Mbol(i__) = rNULL__
c ..............Just test output...........
write(6,7)
+ CNS3_6(i__),Halp(i__),TiO2_1(i__),TiO4_1(i__),TiO5_1(i__),
+ Sp_2(i__),Mv(i__),Vmag_6(i__),R_I(i__),V_I(i__),r_V_I(i__),
+ V_K(i__),S_Hb(i__),S_Ha__S_Hb(i__),log_L_Ha__Lbol(i__),
+ Mbol(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'hyades.dat' ! Photometric and spectroscopic data for
* Hyades stars (table 4b of paper II)
C Format for file interpretation
8 format(
+ I4,1X,F5.2,1X,F5.3,1X,F5.3,1X,F5.3,1X,F4.1,1X,F5.2,1X,F5.2,1X,
+ F4.2,1X,F5.2,1X,F5.2,1X,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'hyades.dat')
write(6,*) '....Loading file: hyades.dat'
do i__=1,25
read(1,'(A68)')ar__7
read(ar__7,8)
+ CNS3_7(i__),Halp_1(i__),TiO2_2(i__),TiO4_2(i__),TiO5_2(i__),
+ Sp_3(i__),Mv_1(i__),Vmag_7(i__),V_I_1(i__),
+ log_L_Ha__Lbol_1(i__),log_LX_Lbol(i__),Mbol_1(i__)
if(ar__7(6:10) .EQ. '') Halp_1(i__) = rNULL__
if(ar__7(12:16) .EQ. '') TiO2_2(i__) = rNULL__
if(ar__7(18:22) .EQ. '') TiO4_2(i__) = rNULL__
if(ar__7(24:28) .EQ. '') TiO5_2(i__) = rNULL__
if(ar__7(47:50) .EQ. '') V_I_1(i__) = rNULL__
if(ar__7(52:56) .EQ. '') log_L_Ha__Lbol_1(i__) = rNULL__
if(ar__7(58:62) .EQ. '') log_LX_Lbol(i__) = rNULL__
if(ar__7(64:68) .EQ. '') Mbol_1(i__) = rNULL__
c ..............Just test output...........
write(6,8)
+ CNS3_7(i__),Halp_1(i__),TiO2_2(i__),TiO4_2(i__),TiO5_2(i__),
+ Sp_3(i__),Mv_1(i__),Vmag_7(i__),V_I_1(i__),
+ log_L_Ha__Lbol_1(i__),log_LX_Lbol(i__),Mbol_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'ic2602.dat' ! Photometric and spectroscopic data for
* IC 2602 stars (table 4c of paper II)
C Format for file interpretation
9 format(
+ I4,1X,F5.2,1X,F5.3,1X,F5.3,1X,F5.3,1X,F4.1,1X,F5.2,1X,F5.2,1X,
+ F4.2,1X,F5.2,1X,F5.2,1X,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'ic2602.dat')
write(6,*) '....Loading file: ic2602.dat'
do i__=1,26
read(1,'(A68)')ar__8
read(ar__8,9)
+ CNS3_8(i__),Halp_2(i__),TiO2_3(i__),TiO4_3(i__),TiO5_3(i__),
+ Sp_4(i__),Mv_2(i__),Vmag_8(i__),V_I_2(i__),
+ log_L_Ha__Lbol_1(i__),log_LX_Lbol_1(i__),Mbol_2(i__)
if(ar__8(6:10) .EQ. '') Halp_2(i__) = rNULL__
if(ar__8(12:16) .EQ. '') TiO2_3(i__) = rNULL__
if(ar__8(18:22) .EQ. '') TiO4_3(i__) = rNULL__
if(ar__8(24:28) .EQ. '') TiO5_3(i__) = rNULL__
if(ar__8(47:50) .EQ. '') V_I_2(i__) = rNULL__
if(ar__8(52:56) .EQ. '') log_L_Ha__Lbol_1(i__) = rNULL__
if(ar__8(58:62) .EQ. '') log_LX_Lbol_1(i__) = rNULL__
if(ar__8(64:68) .EQ. '') Mbol_2(i__) = rNULL__
c ..............Just test output...........
write(6,9)
+ CNS3_8(i__),Halp_2(i__),TiO2_3(i__),TiO4_3(i__),TiO5_3(i__),
+ Sp_4(i__),Mv_2(i__),Vmag_8(i__),V_I_2(i__),
+ log_L_Ha__Lbol_1(i__),log_LX_Lbol_1(i__),Mbol_2(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end