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Near Earth Objects Research in Pulkovo Observatory

Published online by Cambridge University Press:  05 March 2015

A. V. Devyatkin
Affiliation:
Pulkovo Astronomical Observatory of Russian Academy of Science email: [email protected]
E. A. Bashakova
Affiliation:
Pulkovo Astronomical Observatory of Russian Academy of Science email: [email protected]
D. L. Gorshanov
Affiliation:
Pulkovo Astronomical Observatory of Russian Academy of Science email: [email protected]
A. V. Ivanov
Affiliation:
Pulkovo Astronomical Observatory of Russian Academy of Science email: [email protected]
S. V. Karashevich
Affiliation:
Pulkovo Astronomical Observatory of Russian Academy of Science email: [email protected]
V. V. Kouprianov
Affiliation:
Pulkovo Astronomical Observatory of Russian Academy of Science email: [email protected]
V. N. L'vov
Affiliation:
Pulkovo Astronomical Observatory of Russian Academy of Science email: [email protected]
K. N. Naumov
Affiliation:
Pulkovo Astronomical Observatory of Russian Academy of Science email: [email protected]
E. S. Romas
Affiliation:
Pulkovo Astronomical Observatory of Russian Academy of Science email: [email protected]
V. Yu. Slesarenko
Affiliation:
Pulkovo Astronomical Observatory of Russian Academy of Science email: [email protected]
N. A. Shakht
Affiliation:
Pulkovo Astronomical Observatory of Russian Academy of Science email: [email protected]
E. N. Sokov
Affiliation:
Pulkovo Astronomical Observatory of Russian Academy of Science email: [email protected]
S. D. Tsekmeister
Affiliation:
Pulkovo Astronomical Observatory of Russian Academy of Science email: [email protected]
O. O. Vasilkova
Affiliation:
Pulkovo Astronomical Observatory of Russian Academy of Science email: [email protected]
I. A. Vereschagina
Affiliation:
Pulkovo Astronomical Observatory of Russian Academy of Science email: [email protected]
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More than 20000 observations of Near Earth asteroids and comets are collected and reduced in Pulkovo Observatory during last 10 years. For observations of these objects two robotic telescopes are used – ZA-320M (Cassegrain system, D = 320 mm, F = 3200 mm) at Pulkovo and MTM-500M (Maksutov – Cassegrain system, D = 500 mm, F = 4100 mm) at Kislovodsk mountain station. These telescopes perform CCD observations of objects up to 18.0 and 20.5 magnitude, correspondingly. The results of observations are regularly submitted to Minor Planet Center.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2015 

References

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