ODIN: a new model and ephemeris for the Pluto system

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Table 1

Properties of the observations to which ODIN was fitted.

Origin	Number	Reference frame	Observations	Reference	Years

Lowell, Yerkes and McDonald Observatory	552	B1950	Photographic	Cohen et al. (1967)	1914–1965
Asiago Observatory	175	B1950	Photographic	Barbieri et al. (1972, 1975, 1979,	1971–1997
				1988)
A.J. Dyer Observatory	15	B1950	Photographic	Hardie et al. (1985)	1965–1981
La Silla	45	B1950	Photographic	Debehogne et al. (1981);	1980 and 1985
				Debehogne & de Freitas Mourao (1988)
Torino Observatory	39	B1950	Photographic	Zappala et al. (1980, 1983)	1973–1982
Brorfelde Observatory	15	B1950	Photographic	Jensen (1979)	1975–1978
Lick Observatory	11	B1950	Photographic	Klemola & Harlan (1982, 1984, 1986)	1980–1985
Flagstaff Observatory	5	B1950	Photographic	Harrington & Walker (1984)	1980 and 1983
La Silla	29	J2000	Photographic	Gemmo & Barbieri (1994)	1989–1990
Pulkovo astrograph	207	J2000	Photographic	Rylkov et al. (1995)	1930–1993
FASTT	914	J2000	CCD	IAU Comm. 4^a	from 1995
				FASTT website^b
Table Mountain	259	J2000	CCD	IAU Comm. 4^a	1997–2010
Bordeaux-Floirac Observatory	87	J2000	CCD	Rapaport et al. (2002)	1995–1997 and 2002–2005
Observatoire de Haute-Provence	242	J2000	CCD		1997–2010
Observatoire du Pic du Midi	73	J2000	CCD		2011
Stellar occultations	14	J2000	Occultations	Assafin et al. (2010), Bruno	2005–2008
				Sicardy (priv. comm.)

Notes.

^(a)

http://iau-comm4.jpl.nasa.gov/plan-eph-data/.

^(b)

http://www.nofs.navy.mil/data/plansat.html

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