Astrophysics and Space Science

, Volume 309, Issue 1, pp 523–526

GLAST large area telescope multiwavelength planning

  • O. Reimer
  • P. F. Michelson
  • R. A. Cameron
  • S. W. Digel
  • D. J. Thompson
  • K. S. Wood
Original Article

DOI: 10.1007/s10509-007-9474-z

Cite this article as:
Reimer, O., Michelson, P.F., Cameron, R.A. et al. Astrophys Space Sci (2007) 309: 523. doi:10.1007/s10509-007-9474-z
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Abstract

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.

Keywords

Gamma rays Multiwavelength Observatories 

PACS

95.40.+s 95.55.Ka 95.85.Pw 

Copyright information

© Springer Science+Business Media B.V. 2007

Authors and Affiliations

  • O. Reimer
    • 1
  • P. F. Michelson
    • 1
  • R. A. Cameron
    • 2
  • S. W. Digel
    • 2
  • D. J. Thompson
    • 3
  • K. S. Wood
    • 4
  1. 1.HEPL & KIPACStanford UniversityStanfordUSA
  2. 2.SLAC & KIPACStanford UniversityMenlo ParkUSA
  3. 3.NASA Goddard Space Flight CenterGreenbeltUSA
  4. 4.Naval Research LaboratoryWashingtonUSA

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