Waszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015). "Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry". The Astronomical Journal. 150 (3): 35. arXiv:1504.04041. Bibcode:2015AJ....150...75W. doi:10.1088/0004-6256/150/3/75.
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Pravec (2012) web: rotation period 4.65 hours with a brightness amplitude of 0.02 mag. Quality Code is 1. Summary figures at the LCDB and Ondrejov Asteroid Photometry Project (data sheet). Comment Pravec, Kusnirak: Period set at a half of the estimate by Warner (2011); H_R = 9.40±0.03, assuming G = 0.12±0.08.
Waszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015). "Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry". The Astronomical Journal. 150 (3): 35. arXiv:1504.04041. Bibcode:2015AJ....150...75W. doi:10.1088/0004-6256/150/3/75.
Pravec, Petr; Harris, Alan W.; Kusnirák, Peter; Galád, Adrián; Hornoch, Kamil (September 2012). "Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations". Icarus. 221 (1): 365–387. Bibcode:2012Icar..221..365P. doi:10.1016/j.icarus.2012.07.026.
Waszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015). "Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry". The Astronomical Journal. 150 (3): 35. arXiv:1504.04041. Bibcode:2015AJ....150...75W. doi:10.1088/0004-6256/150/3/75.
Pravec, Petr; Harris, Alan W.; Kusnirák, Peter; Galád, Adrián; Hornoch, Kamil (September 2012). "Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations". Icarus. 221 (1): 365–387. Bibcode:2012Icar..221..365P. doi:10.1016/j.icarus.2012.07.026.
Lightcurve plot of (795) Fini, at the Palmer Divide Observatory, B. D. Warner (2010). Rotation period 7.586±0.001 h hours with a brightness amplitude of 0.02±0.01 mag. Quality code of 1+. Summary figures at the LCDB.
Pravec (2012) web: rotation period 4.65 hours with a brightness amplitude of 0.02 mag. Quality Code is 1. Summary figures at the LCDB and Ondrejov Asteroid Photometry Project (data sheet). Comment Pravec, Kusnirak: Period set at a half of the estimate by Warner (2011); H_R = 9.40±0.03, assuming G = 0.12±0.08.
Lightcurve plot of (795) Fini, at the Palmer Divide Observatory, B. D. Warner (2010). Rotation period 7.586±0.001 h hours with a brightness amplitude of 0.02±0.01 mag. Quality code of 1+. Summary figures at the LCDB.