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A survey for TNOs using the APS POSS...

Rhoads, Edward.

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A survey for TNOs using the APS POSS I database.

Record Type:	Electronic resources : Monograph/item
Title/Author:	A survey for TNOs using the APS POSS I database./
Author:	Rhoads, Edward.
Description:	95 p.
Notes:	Source: Dissertation Abstracts International, Volume: 66-03, Section: B, page: 1511.
Contained By:	Dissertation Abstracts International66-03B.
Subject:	Physics, Astronomy and Astrophysics. -
Online resource:	http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=3167711
ISBN:	0542036177

A survey for TNOs using the APS POSS I database.
Rhoads, Edward.

A survey for TNOs using the APS POSS I database. - 95 p.

Source: Dissertation Abstracts International, Volume: 66-03, Section: B, page: 1511.

Thesis (Ph.D.)--University of Minnesota, 2005.

The first epoch Palomar Observatory Sky Survey (POSS I) is an ideal and unused archive for the purpose of data mining Trans-Neptunian Objects (TNOs). The POSS I survey has positions accurate to 0.3&inches;, and covers over three quarters of the sky within 15 degrees of the ecliptic. There were 148 plates scanned by the Automated Plate Scanner project (Pennington et al 1993) that were useful for discovering TNOs with diameters of 500 km or larger. The effective sky coverage area for this search was 4931 square degrees; making this survey one of the most extensive to date. To refine the search we first determined the expected TNO parameters on these plates such as motion between the red and blue plates, the O-E color, and ellipticity using known TNOs. During the time between exposures on the POSS I O and E fields (30--40 minutes), the motion in Right Ascension (RA) for a TNO or Centaur is expected to be between 1&inches; to 5&inches;. Also, the direction of movement, within the errors, was expected to be within 20 degrees of parallel to the ecliptic. Using Varuna, Quaoar, and Pluto the expected O-E color is between 1.0 (0.2 magnitudes bluer than the color of Pluto) and 4.0 (a very red limit). The ellipticity on the O plate and the E plate are found to lie within 0.2 of each other. Finally, real objects are expected to have diameters consistent with the seeing of the plate, and solar system objects are expected to have diameters consistent with their movement during the plate exposure. Every candidate that remained after the various criteria had been applied was visually inspected in order to determine if it was a potential solar system object. The results of this massive survey yielded 17 reliable TNOs and TNO candidates, including Pluto, Quaoar, and Varuna. In addition to the TNOs, 28 Centaur and 31 Asteroid candidates were found. Also, Quaoar was pre-covered, and the Main Belt Asteroid Delia was also recovered.

ISBN: 0542036177Subjects--Topical Terms:

1019521
Physics, Astronomy and Astrophysics.

A survey for TNOs using the APS POSS I database.
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100 1 $a Rhoads, Edward. $3 1905383
245 1 2 $a A survey for TNOs using the APS POSS I database.
300 $a 95 p.
500 $a Source: Dissertation Abstracts International, Volume: 66-03, Section: B, page: 1511.
500 $a Advisers: Charles E. Woodward; Roberta M. Humphreys.
502 $a Thesis (Ph.D.)--University of Minnesota, 2005.
520 $a The first epoch Palomar Observatory Sky Survey (POSS I) is an ideal and unused archive for the purpose of data mining Trans-Neptunian Objects (TNOs). The POSS I survey has positions accurate to 0.3&inches;, and covers over three quarters of the sky within 15 degrees of the ecliptic. There were 148 plates scanned by the Automated Plate Scanner project (Pennington et al 1993) that were useful for discovering TNOs with diameters of 500 km or larger. The effective sky coverage area for this search was 4931 square degrees; making this survey one of the most extensive to date. To refine the search we first determined the expected TNO parameters on these plates such as motion between the red and blue plates, the O-E color, and ellipticity using known TNOs. During the time between exposures on the POSS I O and E fields (30--40 minutes), the motion in Right Ascension (RA) for a TNO or Centaur is expected to be between 1&inches; to 5&inches;. Also, the direction of movement, within the errors, was expected to be within 20 degrees of parallel to the ecliptic. Using Varuna, Quaoar, and Pluto the expected O-E color is between 1.0 (0.2 magnitudes bluer than the color of Pluto) and 4.0 (a very red limit). The ellipticity on the O plate and the E plate are found to lie within 0.2 of each other. Finally, real objects are expected to have diameters consistent with the seeing of the plate, and solar system objects are expected to have diameters consistent with their movement during the plate exposure. Every candidate that remained after the various criteria had been applied was visually inspected in order to determine if it was a potential solar system object. The results of this massive survey yielded 17 reliable TNOs and TNO candidates, including Pluto, Quaoar, and Varuna. In addition to the TNOs, 28 Centaur and 31 Asteroid candidates were found. Also, Quaoar was pre-covered, and the Main Belt Asteroid Delia was also recovered.
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790 $a 0130
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