Precise calibration of CCD images with a small field of view
| Autor: | QY Peng, Alain Vienne, YB Han, Li ZL(李自力) |
|---|---|
| Přispěvatelé: | Joint Laboratory for Optical Astronomy, Chinese Academy of Sciences, Institut de Mécanique Céleste et de Calcul des Ephémérides (IMCCE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Lille-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Astronomie de Lille (LAL), Université de Lille, Sciences et Technologies-Centre National de la Recherche Scientifique (CNRS), National Astronomical Observatoires-CAS, Yunnan Astronomical Observatory, Chinese Academy of Sciences |
| Rok vydání: | 2004 |
| Předmět: |
Physics
Astrophysics::Instrumentation and Methods for Astrophysics Astronomy Astronomy and Astrophysics Astrometry Space and Planetary Science Planet Asteroid Saturn Physics::Space Physics Calibration Astrophysics::Solar and Stellar Astrophysics Satellite Natural satellite Astrophysics::Earth and Planetary Astrophysics [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] Astrophysics::Galaxy Astrophysics Small field of view Remote sensing |
| Zdroj: | Astronomy and Astrophysics-A&A Astronomy and Astrophysics-A&A, 2004, 424, pp.339-344. ⟨10.1051/0004-6361:20034083⟩ |
| ISSN: | 1432-0746 0004-6361 |
| DOI: | 10.1051/0004-6361:20034083 |
| Popis: | International audience; A precise astrometric calibration method is presented for a CCD image with a small field of view. Its detailed computational formulae are given, and its feasibility and accuracy are tested by the observations of both the star and Phoebe, the 9th satellite of Saturn. This new method can also be applicable to other planetary satellites, asteroids and optical counterparts of extragalactic radio sources. |
| Databáze: | OpenAIRE |
| Externí odkaz: |
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