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The Detection Limits for Trans-Neptunian Dwarf Planets of the Siding Spring Survey

Bannister, M. T. and Brown, M. E. and Schmidt, B. P. and McNaught, R. and Garradd, G. and Larson, S. and Beshore, E. (2012) The Detection Limits for Trans-Neptunian Dwarf Planets of the Siding Spring Survey. Meteoritics and Planetary Science, 47 (S1). A53-A53. ISSN 1086-9379. doi:10.1111/j.1945-5100.2012.01401_2.x.

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The population of icy objects beyond Neptune provide dynamical and compositional insight into the early history and subsequent evolution of the Solar System. The past several years have seen the completion of major surveys of this population across the Northern Hemisphere sky and the introduction of surveys in the South. We present the results of our archival search of more than ten thousand square degrees of sky south of the ecliptic observed over five years, with an approximate limiting flux of m(clear)~19.5. We detail our innovative survey technique, its null detection, and our modelling of the survey's sensitivity via a synthetic population of trans-Neptunian objects (TNOs).

Item Type:Article
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URLURL TypeDescription
Brown, M. E.0000-0002-8255-0545
Schmidt, B. P.0000-0001-6589-1287
Larson, S.0000-0002-0057-8211
Additional Information:© 2012 Meteoritical Society. Issue published online: 6 Aug 2012. Article first published online: 8 Aug 2012.
Issue or Number:S1
Record Number:CaltechAUTHORS:20121002-144803978
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Official Citation:The 75th Annual Meeting of the Meteoritical Society Cairns, Australia, 12-17 August, 2012. Meteoritics & Planetary Science, 47: A35–A436. doi: 10.1111/j.1945-5100.2012.01401_2.x
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:34639
Deposited By: Ruth Sustaita
Deposited On:02 Oct 2012 22:03
Last Modified:09 Nov 2021 23:09

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