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A very high energy gamma-ray survey ...

Fegan, Stephen.

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A very high energy gamma-ray survey of unidentified EGRET sources.

紀錄類型:	書目-電子資源 : Monograph/item
正題名/作者:	A very high energy gamma-ray survey of unidentified EGRET sources./
作者:	Fegan, Stephen.
面頁冊數:	205 p.
附註:	Source: Dissertation Abstracts International, Volume: 65-09, Section: B, page: 4620.
Contained By:	Dissertation Abstracts International65-09B.
標題:	Physics, Astronomy and Astrophysics. -
電子資源:	http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=3145066
ISBN:	0496036254

A very high energy gamma-ray survey of unidentified EGRET sources.
Fegan, Stephen.

A very high energy gamma-ray survey of unidentified EGRET sources. - 205 p.

Source: Dissertation Abstracts International, Volume: 65-09, Section: B, page: 4620.

Thesis (Ph.D.)--The University of Arizona, 2004.

A survey of unidentified 100 MeV gamma-ray sources is undertaken, with the Whipple 10m telescope, with the objective of detecting very high energy (>350 GeV) gamma-ray emission. The survey consists of nineteen sets of observations of sources detected by the EGRET instrument on the Compton Gamma-Ray Observatory between 1991 and 1995. Results for 21 EGRET sources are reported; in some cases two EGRET sources are close enough to be viewed in a single observation. For each EGRET source, candidate associations are listed and the implications of each candidate for VHE emission discussed. Finally, a study of the performance of a next-generation ground based instrument, VERITAS, using simulations is presented. The implications of the increased sensitivity of such an instrument for suture gamma-ray surveys is briefly discussed.

ISBN: 0496036254Subjects--Topical Terms:

1019521
Physics, Astronomy and Astrophysics.

A very high energy gamma-ray survey of unidentified EGRET sources.
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520 $a A survey of unidentified 100 MeV gamma-ray sources is undertaken, with the Whipple 10m telescope, with the objective of detecting very high energy (>350 GeV) gamma-ray emission. The survey consists of nineteen sets of observations of sources detected by the EGRET instrument on the Compton Gamma-Ray Observatory between 1991 and 1995. Results for 21 EGRET sources are reported; in some cases two EGRET sources are close enough to be viewed in a single observation. For each EGRET source, candidate associations are listed and the implications of each candidate for VHE emission discussed. Finally, a study of the performance of a next-generation ground based instrument, VERITAS, using simulations is presented. The implications of the increased sensitivity of such an instrument for suture gamma-ray surveys is briefly discussed.
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