KLENOT - PRACTICAL USE OF SOLAR SYSTEM DYNAMICS IN FOLLOW-UP ASTROMETRY OBSERVATIONS OF SMALL SOLAR SYSTEM BODIES

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00070327%3A_____%2F03%3A00014366" target="_blank" >RIV/00070327:_____/03:00014366 - isvavai.cz</a>

Výsledek na webu

—

DOI - Digital Object Identifier

—

Jazyk výsledku

angličtina

Název v původním jazyce

KLENOT - PRACTICAL USE OF SOLAR SYSTEM DYNAMICS IN FOLLOW-UP ASTROMETRY OBSERVATIONS OF SMALL SOLAR SYSTEM BODIES

Popis výsledku v původním jazyce

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 m_V=20.0m 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). We discuss here methods and techniques we use for follow-up astrometry. Some of the practical results are also mentioned.

Název v anglickém jazyce

KLENOT - PRACTICAL USE OF SOLAR SYSTEM DYNAMICS IN FOLLOW-UP ASTROMETRY OBSERVATIONS OF SMALL SOLAR SYSTEM BODIES

Popis výsledku anglicky

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 m_V=20.0m 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). We discuss here methods and techniques we use for follow-up astrometry. Some of the practical results are also mentioned.

Druh

D - Stať ve sborníku

CEP obor

BN - Astronomie a nebeská mechanika, astrofyzika

OECD FORD obor

—

Projekt

<a href="/cs/project/GP205%2F02%2FP114" target="_blank" >GP205/02/P114: Výpočet elementů dráhy a efemerid malých těles sluneční soustavy</a><br>

Návaznosti

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

Rok uplatnění

2003

Kód důvěrnosti údajů

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

Název statě ve sborníku

The Proceedings of the JOURNEES 2003

ISBN

—

ISSN

—

e-ISSN

—

Počet stran výsledku

2

Strana od-do

290-291

Název nakladatele

Institute of Applied Astronomy of the Russian Academy of Sciences and Observatoire de Paris

Místo vydání

France

Místo konání akce

St. Petersburg, Russia

Datum konání akce

22. 9. 2003

Typ akce podle státní příslušnosti

WRD - Celosvětová akce

Kód UT WoS článku

—