21 Lutetia UBVRI light curves (Lamy+, 2010)

Details 21 Lutetia UBVRI light curves (Lamy+, 2010) 21 Lutetia UBVRI light curves (Lamy+, 2010)

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ycat..35219019l&link_type=abstract

VizieR On-line Data Catalog: J/A+A/521/A19. Originally published in: 2010A&A...521A..19L

Physics

Planets, Photometry: Ubvri

Scientific paper

The asteroid was imaged on 2 and 3 January 2007 with the Narrow Angle Camera (NAC) of the Optical, Spectroscopic, and Infrared Remote Imaging System (OSIRIS) during the cruise phase of the Rosetta spacecraft. The geometric conditions were such that the aspect angle was 44° (i.e., mid-northern latitudes) and the phase angle 22.4°. Lutetia was continuously monitored over 14.3h, thus exceeding one rotational period and a half, with twelve filters whose spectral coverage extended from 271 to 986nm. An accurate photometric calibration was obtained from the observations of a solar analog star, 16 Cyg B.
(5 data files).

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