Astronomical Data Center

ADCADC/CDS Standard Document for Catalog:
/catalogs/1/1082/

The following is the "ReadMe" document that describes this ADC catalog. You can access the files described here in three ways:

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2. Get the data files via anonymous FTP. (See Note.) [ftp


I/82                SPF1 Catalogue    (Anguita+ 1975)
================================================================================
First Santiago-Pulkovo Fundamental Stars Catalogue (SPF1)
     Anguita C., Carrasco G., Loyola P.R., Bedin V.N., Naumova A.A.,
     Polojentsev D.D., Polojentseva T.A., Tavastherna K.N., Zverev M.S.
    <Publ. Dept. Astron., Univ. of Chile, 2, 181 (1975)>
    =1975PDAUC...2..181A
================================================================================
ADC_Keywords: Meridian observations ; Positional data ; Stars, fundamental

Description:
    The "First Santiago-Pulkovo Fundamental Stars Catalogue (SPF1)"
    contains right ascension observations of 1043 FK4 stars made during
    the period 1963 to 1968 with the Repsold Meridian Circle located at
    Cerro Calan Observatory in Chile. The FK4 stars were observed during
    series of observations of Southern Reference Stars (SRS) and Bright
    Stars (BS) international programs. Approximately 30 to 45 FK4 stars
    were measured during each 2- to 2-1/2-hour series, and included stars
    observed along the meridian between +41deg and -90deg in upper
    culmination and from -90deg to -68deg in lower culmination. The lower
    culmination observations are given in a separate table in the source
    reference; they are included in the file "lower".

    This work was made during the observations of the SRS and BS
    international programmes. These series of fundamental stars were
    periodically observed on the whole arc of meridian from +40 deg. to
    -68 sp deg. 211 series of observations were made with 6793 RA of stars
    observed.

    The reduction of observations was made by Zverev's quasi-absolute
    method (M.S.Zverev, Astr.J. USSR, 1965, v.42, p.823 and 1969, v.46,
    p.129.). The mean error of the positions of stars in the Catalogue is

    M.E. (Delta Alfa x cos Dec.) = +/- 0.008 timesec.


File Summary:
--------------------------------------------------------------------------------
 FileName    Lrecl    Records    Explanations
--------------------------------------------------------------------------------
ReadMe          80          .    This file
catalog.dat     43       1043    The SPF1 Catalogue
lower.dat       43         82    Lower culminations
--------------------------------------------------------------------------------

Byte-by-byte Description of file: catalog.dat, lower.dat
--------------------------------------------------------------------------------
   Bytes Format  Units   Label    Explanations
--------------------------------------------------------------------------------
   1-  4  I4     ---     FK4        [1/1987]   Number in the FK4 catalogue
                                    (Fricke and Kopff 1963).
   6-  7  I2     h       RAh        Approximate Right Ascension 1950 (hours)
   9- 10  I2     min     RAm        Approximate Right Ascension 1950 (minutes)
      12  A1     ---     DE-        Approximate Declination 1950 (sign)
  13- 14  I2     deg     DEd        Approximate Declination 1950 (degrees)
  16- 17  I2     arcmin  DEm        Approximate Declination 1950 (minutes)
  19- 23  I5     ms      dRAms(i)   Correction to the FK4 right ascension in the
                                    instrumental system (RA-RA(i)) for the
                                    mean epoch of the observations.
  25- 29  I5     ms      dRAms(FK4) Correction to the FK4 right ascension in the
                                    FR4 system for the mean
                                    epoch of the observations.
  31- 32  I2     ---     o_dRAms(i) Number of observations for dRAms(i)
  34- 36  I3     ms      e_dRAms(i) ? Mean square error of the
                                    catalogue position multiplied by
                                    cos(delta), computed with the
                                    deviations of the observations from the
                                    mean.
  38- 43  I6     yr      Epoch      Mean epoch of the observations
--------------------------------------------------------------------------------

Related Data:
  I/44 : SPF2 Catalogue (unpublished)
  I/78 : SPF3 Catalogue (Loyola and Shishkina, =1974PDAUC...2..159L)

Acknowledgments:
    Appreciation is expressed to Dr. A. Fresneau of the CDS, Strasbourg,
    for preparing a handwritten format description of the CDS tape at my
    request, and to Dr. A. Gutirrez-Moreno for sending the University of
    Chile publication required for comparison purposes.

References:
  Fricke, W. and Ropff, A. 1963, Fourth Fundamental Katalog (FK4J,
    Veroeff. Astron. Rechen-Inst. Heidelberg, No. 10.

Historical Notes:
  * March 1982: The SPF1 catalogue was received on magnetic tape from
    the Centre de Donnees Stellaires (CDS), Strasbourg. The data had been
    received on punched cards from the Astronomisches Rechen-Institut,
    Heidelberg and had been punched from a handwritten version (A.
    Fresneau, private communication). A check against the published
    catalogue (Anguita et al. 1975) revealed an extra record in the
    machine-readable version (FR4 #1121 with only one observation; the
    observation must have been removed before publication and has been
    deleted from the file) and one record having an incorrect FK4 number
    and displaced (this has been corrected), plus several stars whose
    right ascensions and declinations disagree by 1m or 1' between the
    computer file and the published catalogue (these have not been changed
    since the right ascensions and declinations are only approximate and
    are not the principal data of the catalogue). The logical record
    length (LRECL) of the file received (the upper and lower culmination
    observations were on a single file) was 88 bytes (a card image plus
    8-byte allowance for CDS identification number); since bytes 50-88
    were always blank, LRECL was changed to 49 bytes to save storage
    space. The upper and lower culmination tables were separated into two
    files due to the fact that lower culmination observations are made at
    lower altitude and are often of lower accuracy than upper culmination
    observations.
  * 18-Sep-1995: Documentation standardized at CDS.
================================================================================
(End)      Dimitri Polojentsev [Pulkovo], Francois Ochsenbein [CDS]  18-Sep-1995

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