The 80-cm azimuthal telescope is newly mounted at Yaoan Station, Purple Mountain Observatory in 2018. The astrometric performance of the telescope is tested in the following three aspects. (a) The geometric distortion of its CCD attached. It is stable in both a single epoch and multi epochs. Eight distortion solutions are derived over about one year. The maximum values range from 0.75 to 0.79 pixel and the median values range from 0.14 to 0.16 pixel. (b) The limit magnitude of stars. About 20.5 magnitude (Gaia-G) stars can be detected with Johnson-V filter exposured in 300 seconds. The astrometric error of about 20.5 magnitude stars is estimated at 0.14 arcsec using the fitted sigmoidal function. (c) The astrometric accuracy and the precisi...
The Extremely Large Telescope and the Thirty Meter Telescope will use state of the art multiconjugat...
Context. Gaia Data Release 1 (DR1) contains astrometric results for more than 1 billion stars bright...
Context. Current instrument developments at the largest telescopes worldwide involve the installatio...
Aims. Astrometric observations performed by the Gaia Follow-Up Network for Solar System Objects (Gai...
Telescope (hereafter, TNT) is an 80-cm Cassegrain reflecting telescope located at the Xinglong Obser...
Proceedings of the 3rd Gaia-FUN-SSO International Worshop held 24-26 November 2014 in Paris, FranceI...
© 2015 ESO. Aims. Astrometric observations performed by the Gaia Follow-Up Network for Solar System ...
The Astrometric Telescope Facility (ATF) is designed to be a space-based facility searching for plan...
Astrometry satellites have common technological issues. (A) Astrometry satellites are requ...
Multi-conjugated adaptive optics (MCAO) is essential for performing astrometry with the Extremely La...
The space astrometry mission Gaia, planned for launch in 2013 by the European Space Agency (ESA), wi...
© ESO, 2016.Context. Gaia Data Release 1 (DR1) contains astrometric results for more than 1 billion ...
Becallse reasonably priced CCD detectors are.available, amateurs can IlOw make astrometric observati...
Large ground-based telescopes equipped with adaptive optics (AO) systems have ushered in a new era o...
International audienceAfter a CCD image of the four Galilean satellites of Jupiter is obtained by a ...
The Extremely Large Telescope and the Thirty Meter Telescope will use state of the art multiconjugat...
Context. Gaia Data Release 1 (DR1) contains astrometric results for more than 1 billion stars bright...
Context. Current instrument developments at the largest telescopes worldwide involve the installatio...
Aims. Astrometric observations performed by the Gaia Follow-Up Network for Solar System Objects (Gai...
Telescope (hereafter, TNT) is an 80-cm Cassegrain reflecting telescope located at the Xinglong Obser...
Proceedings of the 3rd Gaia-FUN-SSO International Worshop held 24-26 November 2014 in Paris, FranceI...
© 2015 ESO. Aims. Astrometric observations performed by the Gaia Follow-Up Network for Solar System ...
The Astrometric Telescope Facility (ATF) is designed to be a space-based facility searching for plan...
Astrometry satellites have common technological issues. (A) Astrometry satellites are requ...
Multi-conjugated adaptive optics (MCAO) is essential for performing astrometry with the Extremely La...
The space astrometry mission Gaia, planned for launch in 2013 by the European Space Agency (ESA), wi...
© ESO, 2016.Context. Gaia Data Release 1 (DR1) contains astrometric results for more than 1 billion ...
Becallse reasonably priced CCD detectors are.available, amateurs can IlOw make astrometric observati...
Large ground-based telescopes equipped with adaptive optics (AO) systems have ushered in a new era o...
International audienceAfter a CCD image of the four Galilean satellites of Jupiter is obtained by a ...
The Extremely Large Telescope and the Thirty Meter Telescope will use state of the art multiconjugat...
Context. Gaia Data Release 1 (DR1) contains astrometric results for more than 1 billion stars bright...
Context. Current instrument developments at the largest telescopes worldwide involve the installatio...