KLENOT - Near Earth and Other unusual objects observations

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00070327%3A_____%2F04%3A00014367" target="_blank" >RIV/00070327:_____/04:00014367 - isvavai.cz</a>

Result on the web

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DOI - Digital Object Identifier

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Result language

angličtina

Original language name

KLENOT - Near Earth and Other unusual objects observations

Original language description

The KLENOT project is a project of the Klet Observatory, Czech Republic, devoted to astrometric observations of Near Earth objects, distant objects and comets. The improved effort of the large NEO surveys resulting in an increasing number of newly discovered NEOs calls for continuous follow-up astrometry to secure an accurate orbit determination of discovered bodies first in discovery opposition and then during next apparitions. Considering this urgent need of astrometric follow-up, the fact that many of these targets are fainter then magnitude 20.0~V and our results and experience in minor planet and comet CCD astrometry done at Klet since 1993, we decided to bring into operation a new 1-m class facility working on a permanent basis - the KLENOT telescope. The regular observing of the telescope started in March 2002 (the MPC code 246). Beside methods and techniques we use for follow-up astrometry we present most important results of the project.

Czech name

KLENOT - Near Earth and Other unusual objects observations

Czech description

The KLENOT project is a project of the Klet Observatory, Czech Republic, devoted to astrometric observations of Near Earth objects, distant objects and comets. The improved effort of the large NEO surveys resulting in an increasing number of newly discovered NEOs calls for continuous follow-up astrometry to secure an accurate orbit determination of discovered bodies first in discovery opposition and then during next apparitions. Considering this urgent need of astrometric follow-up, the fact that many of these targets are fainter then magnitude 20.0~V and our results and experience in minor planet and comet CCD astrometry done at Klet since 1993, we decided to bring into operation a new 1-m class facility working on a permanent basis - the KLENOT telescope. The regular observing of the telescope started in March 2002 (the MPC code 246). Beside methods and techniques we use for follow-up astrometry we present most important results of the project.

Type

D - Article in proceedings

CEP classification

BN - Astronomy and celestial mechanics, astrophysics

OECD FORD branch

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Project

<a href="/en/project/GP205%2F02%2FP114" target="_blank" >GP205/02/P114: Orbital elements and ephemerides determination of small bodies of the solar system</a><br>

Continuities

P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Publication year

2004

Confidentiality

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection

Proceedings IAU Colloquium No. 197:DYNAMICS OF POPULATIONS OF PLANETARY SYSTEMS

ISBN

0-521-85203-X

ISSN

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e-ISSN

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Number of pages

5

Pages from-to

271-274

Publisher name

The International Astronomical Union

Place of publication

Cambridge Univ Press

Event location

Belgrade, Serbia & Montenegro

Event date

Aug 31, 2004

Type of event by nationality

WRD - Celosvětová akce

UT code for WoS article

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