On the Precision of Star Positions Observation Made with the Pulkovo HMC.

Author:

Kirian T.,Pinigin G.

Abstract

After the automation of the Pulkovo HMC two catalogs of Positions of 1081 Stars from FK5B, FK4S, FKFS and RRS were observed. Every star was observed more than three times during the period from March 1988 to May 1990. The internal error of a single observation of FK5 stars was estimated as 0.S015(Sec-Z)0.6, 0″.16 (Sec-Z)0.9 in α and δ. A comparison of the declination of FK5B Stars observed with HMC with those of Bordeaux 86, CAMC 86 and PMC 86÷88 shows the Δδδ differences of the order of 0″.1 in the declination zone 40°÷60°.

Publisher

Cambridge University Press (CUP)

Reference8 articles.

1. Kirian T.R. , Naumov K.N. , Smirnov B.N. , Nikiforova O.Y. , Gorshanov D.L , Pinigin G.I. , Protsyuk Y.I. , Kapkov V.B. , Gumerov R.I. and Aupov F.G. (1992) ‘The Results of the differential determination of the right ascention and declination of the stars made by Pulkovo Sukharev's HMC at 1988-90’, VINITI 6.05.92, N.1488-B92 (in Russian).

2. ‘Comparison of FK5 with Bordeaux and Carlsberg meridian circle observations’;Morrison;Astronomy and Astrophysics,1990

3. ‘The Tokyo PMC Catalog 88: Catalog of Positions of 3800 Stars observed in 1988 and planetary positions observed in 1986 to 1988 with Tokyo photoelectric meridian circle’;Yoshizawa;Publ. Nat. Astron. Obs. Japan,1992

4. Automatic Horizontal Meridian Circle at Pulkovo

5. A new generation of Pulkovo observatory meridian instruments and the first results of observations

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