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Statements

Subject Item
n2:RIV%2F00070327%3A_____%2F00%3A00006425%21RIV%2F2004%2FGA0%2FHVEZD4%2FN
rdf:type
skos:Concept n15:Vysledek
dcterms:description
The increasing rate of NEO discoveries in recent years requires more precise follow-up observations over a sufficient arc. Here we discuss methods and results of the targeted NEO follow-up astrometry programme at the Klet' Observatory. The 0.57-meter reflector, equipped with a CCD camera, has been used for confirmations of newly discovered NEO candidates and early follow-up astrometry of NEOs at the discovery opposition since 1994. Klet' Observatory is one of the most productive sites in the world in this field. The Klet' Observatory obtained astrometric observations of 85 per cent of the Potentially Hazardous Asteroids discovered in 1998, the majority of them as confirmations of the discovery and early follow-up used for preliminary orbit computations. The recoveries of NEOs at a second opposition and follow-up astrometry of poorly observed NEOs at further oppositions are also provided. In the near future we are going to finish an extension of this programme to fainter objects and very fast-moving ob The increasing rate of NEO discoveries in recent years requires more precise follow-up observations over a sufficient arc. Here we discuss methods and results of the targeted NEO follow-up astrometry programme at the Klet' Observatory. The 0.57-meter reflector, equipped with a CCD camera, has been used for confirmations of newly discovered NEO candidates and early follow-up astrometry of NEOs at the discovery opposition since 1994. Klet' Observatory is one of the most productive sites in the world in this field. The Klet' Observatory obtained astrometric observations of 85 per cent of the Potentially Hazardous Asteroids discovered in 1998, the majority of them as confirmations of the discovery and early follow-up used for preliminary orbit computations. The recoveries of NEOs at a second opposition and follow-up astrometry of poorly observed NEOs at further oppositions are also provided. In the near future we are going to finish an extension of this programme to fainter objects and very fast-moving ob
dcterms:title
The importance of follow-up observations for newly discovered NEOs The importance of follow-up observations for newly discovered NEOs
skos:prefLabel
The importance of follow-up observations for newly discovered NEOs The importance of follow-up observations for newly discovered NEOs
skos:notation
RIV/00070327:_____/00:00006425!RIV/2004/GA0/HVEZD4/N
n3:strany
955-959
n3:aktivita
n4:P
n3:aktivity
P(GA205/98/0266)
n3:cisloPeriodika
10
n3:dodaniDat
n11:2004
n3:domaciTvurceVysledku
n9:7127243
n3:druhVysledku
n8:J
n3:duvernostUdaju
n14:S
n3:entitaPredkladatele
n6:predkladatel
n3:idSjednocenehoVysledku
713253
n3:idVysledku
RIV/00070327:_____/00:00006425
n3:jazykVysledku
n10:eng
n3:klicovaSlova
Near Earth Object;astrometry;follow-up;
n3:klicoveSlovo
n13:Near%20Earth%20Object n13:astrometry n13:follow-up
n3:kodStatuVydavatele
GB - Spojené království Velké Británie a Severního Irska
n3:kontrolniKodProRIV
[B6CE5286F4A1]
n3:nazevZdroje
Planetary and Space Science
n3:obor
n12:BN
n3:pocetDomacichTvurcuVysledku
3
n3:pocetTvurcuVysledku
3
n3:projekt
n17:GA205%2F98%2F0266
n3:rokUplatneniVysledku
n11:2000
n3:svazekPeriodika
48
n3:tvurceVysledku
Tichá, Jana
s:numberOfPages
5