Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations
By P. Pravec, Alan W. Harris, P. Kušnirák, A. Galád, K. Hornoch. 2012
178 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Atmospheric Science
View Paper: https://www.semanticscholar.org/paper/9636a9ad9d98c4f758c3e007d4a8c301c3f52152
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In Astronomy and Astrophysics
In Atmospheric Science
Citations in the corpus
- Asteroid family ages (2015, unknown): “2.2] and in (Pravec et al., 2012).”
- The taxonomic distribution of asteroids from multi-filter all-sky photometric surveys (2013, background): “Evaluation for a particular target should be considered with caution, the absolute magnitude and albedo being possibly subject to large uncertainties and biases (e.g., Romanishin and Tegler 2005, Mueller et al. 2011, Pravec et al. 2012).”
- INITIAL PERFORMANCE OF THE NEOWISE REACTIVATION MISSION (2014, unknown): “The IAU phase slope parameter G is assumed to be 0.15±0.10 unless independent measurements were available for a given object from Warner et al. (2009) or Pravec et al. (2012); otherwise, H values were taken from the Minor Planet Center.”