Bloom, Steven D. and Dale, Daniel A. (2001) Optical identification and monitoring of high energy gamma-ray sources. In: Gamma 2001. AIP Conference Proceedings. No.587. American Institute of Physics , Melville, NY, pp. 329-332. ISBN 0-7354-0027-X http://resolver.caltech.edu/CaltechAUTHORS:20111111-090857288
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We will be presenting updated results to our optical survey of the "error boxes" of EGRET unidentified sources at high Galactic latitude. It is our intention to search for potential blazars that may have been missed in the original identification process. We have first searched the error boxes of unidentified sources at |b|>20° for flat spectrum radio sources using NASA Extragalactic Database (NED). For each such radio source found we conducted optical searches for counterparts using the Palomar 60-inch telescope. Many of the radio sources have plausible optical counterparts, and spectroscopy will be conducted at a later date to determine which sources are quasars or active galaxies (AGN's). Though it is plausible that several of these sources are extragalactic, no blazar-like activity has yet been observed.
|Item Type:||Book Section|
|Additional Information:||© 2001 American Institute of Physics. Issue Date: 7 October 2001. This work has made use of the NASA Extragalactic Database and the Astrophysical Data System web abstract server.|
|Subject Keywords:||gamma-ray sources (astronomical), radiosources (astronomical), BL Lac-type objects, quasars, astronomical telescopes, astronomical catalogues, astronomical atlases|
|Classification Code:||PACS: 98.70.Rz; 95.80.+p; 98.54.Cm|
|Official Citation:||Optical identification and monitoring of high energy gamma-ray sources Steven D. Bloom and Daniel A. Dale, AIP Conf. Proc. 587, 329 (2001), DOI:10.1063/1.1419424|
|Usage Policy:||No commercial reproduction, distribution, display or performance rights in this work are provided.|
|Deposited By:||Tony Diaz|
|Deposited On:||18 Jan 2012 22:26|
|Last Modified:||26 Dec 2012 14:24|
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