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 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 dRA RA-RA(FK4) 37-41 F5.2 a Ep-1900 Epoch of mean observation - 1900 years 42-45 F4.3 s e_RA *Error on Right Ascension 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 on Right Ascension 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] 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
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line