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Buie, M. W.; Millis, R. L.; Wasserman, L. H.; Elliot, J. L.; Kern, S. D.; Clancy, K. B.; et al. (June 2003). "Procedures, Resources and
Selected Results of the Deep Ecliptic Survey".
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395:"The Deep Ecliptic Survey: A Search for Kuiper Belt Objects and Centaurs. II. Dynamical Classification, the Kuiper Belt Plane, and the Core Population"
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Elliot, J. L.; Kern, S. D.; Clancy, K. B.; Gulbis, A. A. S.; Millis, R. L.; Buie, M. W.; et al. (February 2005).
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of 22.5, which means an estimated 50% of objects of this magnitude have been found.
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The survey has also established the mean Kuiper Belt plane and introduced new
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The remarkable first observations and/or discoveries include:
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Since 1998 through the end of 2003, the survey covered 550
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312:(0.96) taking the object from the inside of the Neptune's
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198:objects (KBOs), using the facilities of the
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586:Discoveries by the Deep Ecliptic Survey
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364:"Minor Planet Discoverers (by number)"
284:too far to be affected (scattered) by
202:(NOAO). The principal investigator is
200:National Optical Astronomy Observatory
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466:10.1023/B:MOON.0000031930.13823.be
370:. 4 September 2016. Archived from
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265:trans-Neptunian object
20:discovered: 9
576:Astronomical surveys
316:to more than 1000 AU
188:Deep Ecliptic Survey
135:88611 Teharonhiawako
411:2005AJ....129.1117E
368:Minor Planet Center
169:(361701) 2007 VZ171
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60:38083 Rhadamanthus
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376:. Retrieved
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310:eccentricity
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288:and a large
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548:Outer space
536:Spaceflight
241:19521 Chaos
232:28978 Ixion
215:sensitivity
196:Kuiper belt
47:22 May 2001
43:28978 Ixion
26:19521 Chaos
570:Categories
350:References
282:perihelion
512:Astronomy
474:14820512
343:inclined
245:cubewano
234:, large
498:Portals
454:Bibcode
407:Bibcode
336:2002 XU
321:2001 QR
286:Neptune
252:1998 WW
236:plutino
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262:binary
524:Stars
470:S2CID
444:arXiv
314:orbit
267:(TNO)
213:with
380:2016
186:The
178:list
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