Published October 22, 1999 | Version Published
Book Section - Chapter Open

Novel design for an all-sky low-energy gamma-ray observatory (ALLEGRO)

  • 1. ROR icon Northwestern University
  • 2. ROR icon University of California, Riverside
  • 3. ROR icon University of Alabama in Huntsville
  • 4. ROR icon California Institute of Technology
  • 5. ROR icon Purdue University West Lafayette

Abstract

We present a novel concept for a MIDEX satellite mission that allows all sky coverage for gamma-ray bursts and hard x-ray transients. The multiscale alternating shadow collimator (MASC) alone allows for arc minute positioning of 1 second bursts 3 times weaker than the BATSE sensitivity. Our scientific objectives include the ability: (a) to detect and monitor thousands of gamma-ray bursts (GRBs) and hard x- ray sources with sensitivity 3-10 times better than BATSE; (b) to solve the gamma-ray burst mystery; (c) to use gamma- ray bursts as probes of cosmological star formation and to measure cosmological parameters; (d) to understand the physics of the high energy radiation from AGNs and BLAZARs; (e) to study the physics of matter in the extreme around black holes and neutron stars; (f) to determine the pulsar birth rate and physical characteristics. The mission concept, MASC concept, and simulations are presented.

Additional Information

© 1999 Society of Photo-Optical Instrumentation Engineers (SPIE). We thank Alan Wolfe for help in designing the ground support system.

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Eprint ID
91442
Resolver ID
CaltechAUTHORS:20181204-132721661

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2018-12-06
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2021-11-16
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Infrared Processing and Analysis Center (IPAC)
Series Name
Proceedings of SPIE
Series Volume or Issue Number
3765