4.6 Article

THE LA SILLA-QUEST KUIPER BELT SURVEY

Journal

ASTRONOMICAL JOURNAL
Volume 144, Issue 5, Pages -

Publisher

IOP PUBLISHING LTD
DOI: 10.1088/0004-6256/144/5/140

Keywords

instrumentation: detectors; Kuiper belt: general; planets and satellites: detection

Funding

  1. NASA [NNX10AB31G]
  2. DOE [DE-FG02-ER92-40704]
  3. NSF Astronomy and Astrophysics Postdoctoral Fellowship [AST-1003258]
  4. NASA [NNX10AB31G, 136599] Funding Source: Federal RePORTER

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We describe the instrumentation and detection software and characterize the detection efficiency of an automated, all-sky, southern-hemisphere search for Kuiper Belt Objects (KBOs) brighter than R mag 21.4. The search relies on Yale University's 160 Megapixel QUEST camera, previously used for the successful surveys at Palomar that detected most of the distant dwarf planets, and now installed on the ESO 1.0 m Schmidt telescope at La Silla, Chile. Extensive upgrades were made to the telescope control system to support automation, and significant improvements were made to the camera. To date, 63 new KBOs have been discovered, including a new member of the Haumea collision family (2009 YE7) and a new distant object with an inclination exceeding 70 degrees (2010 WG9). In a survey covering similar to 7500 deg(2), we have thus far detected 77 KBOs and Centaurs, more than any other full-hemisphere search to date. Using a pattern of dithered pointings, we demonstrate a search efficiency exceeding 80%. We are currently on track to complete the southern-sky survey and detect any bright KBOs that have eluded detection from the north.

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