GLAST: Physics Goals And Instrument Status

@inproceedings{Carson2006GLASTPG,
  title={GLAST: Physics Goals And Instrument Status},
  author={Jennifer E. Carson},
  year={2006}
}
The Gamma-ray Large Area Space Telescope (GLAST) is a space-based observatory scheduled to launch in October 2007 with two instruments: (1) the GLAST Burst Monitor (GBM), sensitive to photon energies between 8 keV and 25 MeV and optimized to detect gamma-ray bursts, and (2) the Large Area Telescope (LAT), sensitive to gamma rays between 20 MeV and 300 GeV and designed to survey the gamma-ray sky with unprecedented sensitivity. We describe the LAT and the GBM. We then focus on the LAT's… 

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References

SHOWING 1-10 OF 12 REFERENCES

The GLAST burst monitor

The next large NASA mission in the field of gamma-ray astronomy, GLAST, is scheduled for launch in 2007. Aside from the main instrument LAT (Large-Area Telescope), a gamma-ray telescope for the

The Luminosity Function of the EGRET Gamma-Ray Blazars

We examine the properties of the gamma-ray active galactic nuclei (AGNs) detected by EGRET. We calculate the evolution and luminosity function of the gamma-ray-loud AGNs, and we estimate the

The gamma-ray background from blazars : a new look

We present the results of a new model calculation of the γ-ray background produced by unresolved blazars, using the second EGRET catalogue and taking account of flaring. These results are compared to

Multiwavelength Observations of Markarian 501 during the 1997 High State

During the observation period 1997, the nearby blazar Mrk 501 showed extremely strong emission and high variability. We examine multiwavelength aspects of this event using radio, optical, soft and

X-Ray Spectral Variability Signatures of Flares in BL Lacertae Objects

We present a detailed parameter study of the time-dependent electron injection and kinematics and the self-consistent radiation transport in jets of intermediate- and low-frequency peaked BL Lac

X-ray spectral variability signatures of flares in BL Lac objects

We are presenting a detailed parameter study of the time-dependent electron injection and kinematics and the self-consistent radiation transport in jets of intermediate and low-frequency peaked BL

Proc of SPIE

The contribution of unresolved radio-loud AGN to the extragalactic diffuse gamma-ray background

We present a calculation of the blazar contribution to the extragalactic diffuse γ-ray background (EGRB) in the EGRET energy range. Our model is based on inverse-Compton scattering as the dominant

subm i tted to A pJ

  • 2006

MNRAS

  • MNRAS
  • 2000