GLAST large area telescope multiwavelength planning
Gamma-ray astrophysics depends in many ways on multiwavelength studies. The Gamma-ray Large Area Space Telescope (GLAST) Large Area Telescope (LAT) Collaboration has started multiwavelength planning well before the scheduled 2007 launch of the observatory. Some of the high-priority multiwavelength needs include: (1) availability of contemporaneous radio and X-ray timing of pulsars; (2) expansion of blazar catalogs, including redshift measurements; (3) improved observations of molecular clouds, especially at high galactic latitudes; (4) simultaneous broad-band blazar monitoring; (5) characterization of gamma-ray transients, including gamma ray bursts; (6) radio, optical, X-ray and TeV counterpart searches for reliable and effective sources identification and characterization. Several of these activities are needed to be in place before launch.
KeywordsGamma rays Multiwavelength Observatories
PACS95.40.+s 95.55.Ka 95.85.Pw
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- Michelson, P.: Instrument for the gamma-ray large area space telescope (GLAST) mission. In: J.E. Trümper, H.D. Tananbaum (eds.) X-Ray and Gamma-Ray Telescopes and Instruments for Astronomy. Proc. SPIE, vol. 4851, pp. 1144–1150 (2003) Google Scholar
- Thompson, D.J.: Gamma ray pulsars. In: Cheng, K.S., Romero, G.E. (eds.) Cosmic Gamma-Ray Sources, pp. 149–168. Kluwer Academic, Dordrecht (2004) Google Scholar