Astronomical Data Center

ADCADC/CDS Standard Document for Catalog:
/catalogs/1/1044/

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

1. Use the ADC Data Viewer Suite to visualize the data. [preview
2. Get the data files via anonymous FTP. (See Note.) [ftp


I/44        Second Cat of Fundamental Stars (SPF2)     (Baturina+ 1986)
================================================================================
Catalogue of Coordinates of Reference Faint, Bright and Double Stars
South of -47 Degree and Corrections to FK4 Positions as Observed by
Pulkovo Astronomers with the Meridian Circle at the Cerro-Kalan
Observatory (Chile) in 1963-1968
    Baturina G.D., Bedin V.S., Gnevysheva K.G., Zverev M.S., Naumova A.A.,
    Plugina A.I., Polozhentsev D.D., Polozhentseva T.A., Stepanova E.A.
   <Tr. Glav. Astron. Obs. Pulkovo, Ser.2, 86, 4-158 (1986)>
   =1986TrPul..86....4B
================================================================================
ADC_Keywords: Meridian observations ; Positional data

Description:
   The Catalogue  SPF2  was obtained from  observations of the
   fundamental FK4 stars as a reference stars for SRS,  BS and DS star.
   Observations were made by Pulkovo observers  in  the declination zone
   -42 to -90 and +16 to -16 degrees using Repsold Meridian Circle of
   the Cerro Calan  Observatory (Santiago, Chile) from 1963 to 1968.

Introduction:
   They worked in closed cooperations with their Chilean colleagues
   who  observed  other declination zones. In total 15160 observations
   were made of FK4 stars. The reductions of observations were
   made by the quasi-absolute method proposed  by M.S.Zverev (1969).
   Investigations were carried out of the systematic differences of
   type "E-W" as well as of the personal  equations. Also differences of
   type "Upper - Lower culmination" were investigated. All these
   corrections were applied to the  observations. The  mean  error of
   the single observations reduced to the equator is +/- 14.0 millisecond
   of time.  The mean error  of the position of a single star reduced
   to the equator is +/- 2.8 millisec of time (each position in the
   middle are consists from 25 observations). The main results of the
   systematic errors were published by Zverev and Naumova.

File Summary:
--------------------------------------------------------------------------------
  FileName      Lrecl  Records   Explanations
--------------------------------------------------------------------------------
ReadMe             80        .   This file
spf2.dat           47      326   +16 to -16 deg - RA corrections
spf2a.dat          47      280   -40 to -90 deg - RA and Dec. for 280 stars
spf2b.dat          51       62   -40 to -90 deg - RA with upper and lower
                                 culmination separate
--------------------------------------------------------------------------------

See also:
    I/82 : SPF1 Catalogue  (Anguita+ 1975)
    I/78 : SPF3 Catalogue (Loyola+ 1974)

Byte-by-byte Description of file: spf2.dat
--------------------------------------------------------------------------------
   Bytes Format  Units   Label    Explanations
--------------------------------------------------------------------------------
   1-2   I2      ---     03       "03"
   3-6   I4      ---     ID       FK4 number
   7-10  F4.1    mag     mag      Magnitude
   11-12 I2      h       RAh      Right Ascension (B1950.0) hours
   13-14 I2      min     RAm      Right Ascension (B1950.0) minutes
   15-20 F6.3    s       RAs      Right Ascension (B1950.0) seconds
   21    A1      ---     DE-      [-0]Declination (B1950.0) sign
   22-23 I2      deg     DEd      Declination (B1950.0) degrees
   24-25 I2      arcmin  DEm      Declination (B1950.0) arcminutes
   26-30 F5.2    arcsec  DEs      Declination (B1950.0) arcsec
   31-36 F6.3    s       del_RA   RA-RA(FK4)
   37-41 F5.2    a       Ep-1900  Epoch of mean observation - 1900 years
   42-45 F4.3    s       e       *Error
   46-47 I2      ---     N        Number of observations
--------------------------------------------------------------------------------
Note on e:
   E*cos(DE)    where E = error of observations
--------------------------------------------------------------------------------

Byte-by-byte Description of file: spf2a.dat
--------------------------------------------------------------------------------
   Bytes Format  Units   Label    Explanations
--------------------------------------------------------------------------------
   1-2   I2      ---     rem     *Remark
   3-6   I4      ---     ID       FK4 number
   7-10  F4.1    mag     mag      Magnitude
   11-12 I2      h       RAh      Right Ascension (B1950.0) hours
   13-14 I2      min     RAm      Right Ascension (B1950.0) minutes
   15-20 F6.3    s       RAs      Right Ascension (B1950.0) seconds
   21    A1      ---     DE-      [-0]Declination (B1950.0) sign
   22-23 I2      deg     DEd      Declination (B1950.0) degrees
   24-25 I2      arcmin  DEm      Declination (B1950.0) arcminutes
   26-30 F5.2    arcsec  DEs      Declination (B1950.0) arcsec
   31-36 F6.3    s       del_RA   RA-RA(FK4)
   37-41 F5.2    a       Ep-1900  Epoch of mean observation - 1900 years
   42-45 F4.3    s       e       *Error
   46-47 I2      ---     N        Number of observations
--------------------------------------------------------------------------------
Note on rem:
        "-3"    data of spf2b.dat exist
        "03"    data of spf2b.dat do not exist
Note on e:
   E*cos(DE)    where E = error of observations
--------------------------------------------------------------------------------

Byte-by-byte Description of file: spf2b.dat
--------------------------------------------------------------------------------
   Bytes Format  Units   Label    Explanations
--------------------------------------------------------------------------------
   1     I1      ---     3        "3"
   2-5   I4      ---     ID       FK4 number
   6-8   F3.1    mag     mag      Magnitude
   9-10  I2      h       RAh      Right Ascension (B1950.0) hours
   11-12 I2      min     RAm      Right Ascension (B1950.0) minutes
   13    A1      ---     DE-      [-0]Declination (B1950.0) sign
   14-15 I2      deg     DEd      Declination (B1950.0) degrees
   16-17 I2      arcmin  DEm      Declination (B1950.0) arcminutes
   18-23 F6.3    s       uRA      RA-RA(FK4) (upper culmination)
   24-28 F5.2    a       uEp-1900 Epoch of mean obs (upper culmination) - 1900
   29-32 F4.3    s       ue       Error (upper culmination)
   33-34 I2      ---     uN       Number of observations (upper culmination)
   35-40 F6.3    s       lRA      RA-RA(FK4) (lower culmination)
   41-45 F5.2    a       lEp-1900 Epoch of mean obs (lower culmination) - 1900
   46-49 F4.3    s       le       Error (lower culmination)
   50-51 I2      ---     lN       Number of observations
--------------------------------------------------------------------------------

Acknowledgements:
    We appreciate the extensive information provided by D. Polojentsev.

References:
   M.S.Zverev. Astronomicheskii Zhurnal (Soviet Astronomy), v.46,
     p.1290, 1969.
   M.S.Zverev, A.A.Naumova, D.D.Polojentsev, E.A.Ctepanova.
     Astronomicheskii Zhurnal (Soviet Astronomy), v. 50, pp.433-435
   G.D.Baturina et al.  Trudy Glavnoy Astronomicheskoi Observatorii
     (Tran. of the Pulkovo Observatory) v.86, pp. 4-158, 1986
================================================================================
(End)        Nancy Grace Roman and Julie Anne Watko [SSDOO/ADC]      29-Feb-1996

Go to ADC Home Page