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David L. Rabinowitz
David Lincoln Rabinowitz (born 1960) is a researcher at Yale University. He has built CCD cameras and software for the detection of near-Earth asteroids and Kuiper Belt Objects,〔(David Rabinowitz overview )〕 and his research has helped reduce the assumed number of near-Earth asteroids larger than 1 km by half, from 1,000–2,000 to 500–1,000〔(NASA report on the reduction of the number of near earth asteroids. )〕 He has also assisted in the detection of distant solar system objects, supernovae, and quasars, thereby helping to understand the origin and evolution of the solar system and the dark energy driving the accelerated expansion of the universe.
Collaborating with Michael Brown and Chad Trujillo of the Quasar Equatorial Survey Team, he has participated in the discovery of several plutoids such as 90377 Sedna (possibly the first known inner Oort cloud object〔(''The Astrophysical Journal''. )〕), 90482 Orcus,〔(BBC report. )〕 Eris (more massive than Pluto), ,〔M. E. Brown, A. H. Bouchez, D. L. Rabinowitz, R. Sari, C. A. Trujillo, M. A. van Dam, R. Campbell, J. Chin, S. Hartman, E. Johansson, R. Lafon, D. LeMignant, P. Stomski, D. Summers, P. L. Wizinowich ''Keck Observatory laser guide star adaptive optics discovery and characterization of a satellite to large Kuiper belt object 2003 EL61'', The Astrophysical Journal Letters, 632, L45 (October 2005) (Full text from Caltech )〕 and ,〔(Memphis Archeological and Geological Society. )〕 although he would not get credit for Haumea.
Together with Tom Gehrels of the University of Arizona and his Spacewatch Team, Rabinowitz discovered or co-discovered other astronomical objects including 5145 Pholus〔(The Encyclopedia of Astrobiology, Astronomy and Spaceflight. )〕 and 1991 BA.
== References ==
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