GLAST Large Area Telescope Multiwavelength Planning
| dc.creator | Reimer, O. | |
| dc.creator | Michelson, P. F. | |
| dc.creator | Cameron, R. A. | |
| dc.creator | Digel, S. W. | |
| dc.creator | Thompson, D. J. | |
| dc.creator | Wood, K. S. | |
| dc.date | 2006-11-21 | |
| dc.date.accessioned | 2026-07-07T10:36:37Z | |
| dc.date.available | 2026-07-07T10:36:37Z | |
| dc.description | 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. | |
| dc.description | Comments: 4 pages, Accepted for publication in Astrophysics and Space Science, Proc. of "The Multi-Messenger Approach to High-Energy Gamma-ray Sources (Third Workshop on the Nature of Unidentified High-Energy Sources)", Barcelona, July 4-7, 2006 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0611652 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0611652 | |
| dc.identifier | Astrophys.SpaceSci.309:523-526,2007 | |
| dc.identifier | doi:10.1007/s10509-007-9474-z | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/180114 | |
| dc.subject | Astrophysics | |
| dc.title | GLAST Large Area Telescope Multiwavelength Planning | |
| dc.type | text |