I/210  Mean Positions and proper motions of 995 FK4Sup stars    (Schwan+ 1993)
Improved mean positions and proper motions for the 995 FK4Sup stars
not included in the FK5 Extension
     Schwan H., Bastian U., Bien R., Jaehrling R., Jahreiss H., Roeser S
    <Veroeff. Astron. Rechen-Inst. Heidelberg, 34 (1993)>
    =1993VeARI..34....1S 1993VeARI..34....1S
ADC_Keywords: Positional data ; Proper motions ; Stars, fundamental
Description:
    This catalogue lists improved mean positions and proper motions for
    the 995 stars in the FK4 Supplement (Veroeff. Astron. Rechen-Inst.
    Heidelberg No 11, 1963) which were not included in the Fifth
    Fundamental Catalogue (Part I: "The Basic FK5", Fricke et al., 1988,
    Veroeff. Astron. Rechen-Inst. Heidelberg No 32, Catalogue I/149/; Part
    II: "The FK5 Extension", Fricke et al., 1991, Veroeff. Astron.
    Rechen-Inst. Heidelberg No 33, Catalogue I/175/). The main purpose of
    the FK4 Supplement was to stimulate further observations within
    absolute and differential programs of the stars listed in that
    catalogue with the aim of their inclusion as new fundamental stars
    into a future fundamental catalogue. The new fundamental stars should
    increase the star density without extending the magnitude limit to
    fainter magnitudes. Since the publication of the "Supplement-Katalog
    des FK3" (published in Astron-Geodaet. Jahrbuch 1954 and
    Astron-Geodaet. Jahrbuch 1956) these stars were included in many
    observing programs.
    Within work on deriving the FK5 Extension all stars in the FK4
    Supplement had been treated in exactly the same way and improved mean
    positions and proper motions had thus been obtained for all FK4 Sup
    stars. For more details reference is made to the introduction of the
    FK5 Extension. FK4 Sup stars with the best astrometric data were
    included in the FK5 Extension for achieving a homogeneous distribution
    in magnitude and taking simultaneously into account an even
    distribution on the sky. This selection process included 992 of the
    1987 FK4 Sup stars into the FK5 Extension.
    Although the astrometric precision of the stars given in the present
    catalogue is inferior to that of the FK4 Supplement stars included in
    the FK5 Extension, they deserve being published because a considerable
    number of observations has been obtained for these stars since about
    1955, stimulated by the publication of the FK3 Supplement. The average
    mean epoch of observation of the stars given is therefore shifted to
    comparatively modern epochs (see the table in Section 2 of the
    publication). The astrometric precision of the stars presented here is
    better than for most other published star positions and proper
    motions, and the positions and proper motions are the best which could
    be derived from the available observations. These observations are
    published in the same catalogues as listed in the FK5, Part II on
    pages 139 ff. The apparent visual magnitudes are between 3.6 and 7.7
    with a concentration around the mean value of 5.94. They are thus
    within the magnitude limit of the Basic FK5.
File Summary:
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 FileName    Lrecl    Records    Explanations
--------------------------------------------------------------------------------
ReadMe          80          .    This file
catalog.dat    203        995    The catalogue
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See also:
  I/143 : Fourth Fundamental Catalogue and Supplement (FK4) (Fricke+ 1963)
  I/149 : Fifth Fundamental Catalogue, part I   FK5(I)    (Fricke+, 1988)
  I/175 : Fifth Fundamental Catalogue, part III FK5(III)  (Fricke+, 1988)
  I/161 : AGK3R (Smith, 1990)
Byte-by-byte Description of file: catalog.dat
--------------------------------------------------------------------------------
   Bytes Format  Units    Label     Explanations
--------------------------------------------------------------------------------
   1-  4  I4     ---      FK4       Designation
   7-  8  I2     h        RAh       Right Ascension Epoch=J2000 Equinox=J2000
                                      (hours)
  10- 11  I2     min      RAm       Right Ascension J2000 (minutes)
  13- 18  F6.3   s        RAs       Right Ascension J2000 (seconds)
  21- 27  F7.3   10ms/yr  pmRA      Proper motion in RA (s/Julian century) J2000
      30  A1     ---      DE-       Declination J2000 (sign)
  31- 32  I2     deg      DEd       Declination Epoch + Equinox J2000 (degrees)
  34- 35  I2     arcmin   DEm       Declination J2000 (minutes)
  37- 41  F5.2   arcsec   DEs       Declination J2000 (seconds)
  44- 50  F7.2  10mas/yr  pmDE      Proper motion in DE (arcsec/Julian century),
                                       J2000 system
  53- 54  I2     h        RA1950h   Right Ascension Equinox=B1950 Equinox=B1950
                                      (hours)
  56- 57  I2     min      RA1950m   Right Ascension B1950 (minutes)
  59- 64  F6.3   s        RA1950s   Right Ascension B1950 (seconds)
  67- 73  F7.3   10ms/yr  pmRA1950  Proper motion in RA (s/Julian century),
                                      B1950 system
      76  A1     ---      DE1950-   Declination B1950 (sign)
  77- 78  I2     deg      DE1950d   Declination Epoch + Equinox B1950 (degrees)
  80- 81  I2     arcmin   DE1950m   Declination B1950 (minutes)
  83- 87  F5.2   arcsec   DE1950s   Declination B1950 (seconds)
  90- 96  F7.2  10mas/yr  pmDE1950  Proper motion in DE (arcsec/Julian century),
                                      B1950 system
  99-103  F5.2   yr       EpRA-1900 Mean epoch in RA (1900+)
 104-108  F5.1   ms       e_RAs     Mean error of RA at the mean epoch (1)
 109-113  F5.0 0.01ms/yr  e_pmRA    Mean error of pmRA in 0.001s/century
 117-121  F5.2   yr       EpDE-1900 Mean epoch in DE (1900+)
 123-126  F4.1   10mas    e_DEs     Mean error of DE at the mean epoch (1)
 129-131  F3.0 0.1mas/yr  e_pmDE    Mean error of pmDE in 0.01arcsec/century
 136-140  F5.2   mag      Vmag      Photoelectric apparent visual magnitude
                                      from various sources
     141  A1     ---    n_Vmag      [V] 'V' if the star is variable
 143-148  A6     ---      Sp        Spectrum mainly from HD; byte 146 is '+'
                                      if two spectra
 151-156  F6.4   arcsec   plx       [0/.075]? Parallax from preliminary
                                      version of van Altena's catalogue of
                                      trigonometric parallaxes (I/174/)
 159-165  F7.2   km/s     RV        ? Radial velocity from various sources
 168-172  I5     ---      AGK3R     [1/21499]? Designation in AGK3R catalogue
                                      (Smith 1990, catalogue I/161/)
 175-179  I5     ---      SRS       ]50000/70000[? Designation in
                                      Southern Reference System + 50000
 181-186  I6     ---      HD        [1/225300] HD Designation (2)
     188  I1     ---    n_DM        [1/3] DM designator: 1=BD, 2=CoD, 3=CPD
 189-196  A8     ---      DM        Durchmusterung identification
 199-203  I5     ---      GC        Designation in General Catalogue (I/113/)
--------------------------------------------------------------------------------
Note (1): the last digit of the mean errors of mean positions for the
    less precise stars in the IRS list (numbers larger than 4000) is
    always a zero; it is not a computed digit but has merely been added
    to pad the field.
Note (2): stars with composite spectrum have two successive HD numbers;
    the smaller one is only given.
Courtesy: Heiner Schwan, ARI
History:
  * 17-Apr-2002: standardized
(End)                                    Francois Ochsenbein [CDS]   04-Jul-1994