Photometry of 3 main belt asteroids (Marciniak+, 2009)

Details Photometry of 3 main belt asteroids (Marciniak+, 2009) Photometry of 3 main belt asteroids (Marciniak+, 2009)

Feb 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ycat..34980313m&link_type=abstract

VizieR On-line Data Catalog: J/A+A/498/313. Originally published in: 2009A&A...498..313M

Physics

Minor Planets, Photometry

Scientific paper

Table aspdat.dat contains aspect data for all of the observing runs, that is: distances from the object to th Sun and to the Earth in AU, phase angles and ecliptic coordinates of a given asteroid at a given moment. The last column contains the observatory code. The files *lcs.dat contain asteroid brightness and geometry for corresponding epochs. These files were used for obtaining shape models and spin states of the asteroids. All lightcurves are relative.
(5 data files).

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