Published April 12, 2000 | Version v1
Journal article

The Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE): New results at 100 GeV

  • 1. Enrico Fermi Institute, University of Chicago, Chicago, Illinois 60637 (United States)
  • 2. Institute of Geophysics and Planetary Physics, Univ. of California, Riverside, California 92521 (United States)
  • 3. Santa Cruz Institute for Particle Physics, Univ. of California, Santa Cruz, California 95064 (United States)
  • 4. Department of Physics, University of Alberta, Edmonton, Alberta (Canada)
  • 5. Department of Physics and Astronomy, California State Univ., Los Angeles, California 90032 (United States)
  • 6. Department of Physics, McGill University, Montreal, Quebec H3A 2T8 (Canada)
  • 7. Department of Physics and Astronomy, Barnard College and Columbia Univ., New York, 10027 (United States)

Description

The Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE) is a new ground-based instrument for observing astrophysical sources of gamma-rays in the energy range from 50 to 250 GeV. The first phase of STACEE, using 32 large heliostat mirrors, was completed in the fall of 1998. We describe the STACEE operations and observations during the 1998-1999 winter observing season. We have detected the Crab Nebula with high significance (∼7σ). This result demonstrates that the STACEE concept is sound and that we can expect to make sensitive measurements of gamma-ray sources at energies below 100 GeV. The full STACEE instrument, with 64 heliostats, will be completed during the year 2000. The first three years of observations with the complete instrument will include a range of sources with an emphasis on Active Galactic Nuclei (AGN) and supernova remnants

Additional details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
510
Journal Issue
1
Journal Page Range
p. 632-636
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
5. Compton symposium on gamma-ray astronomy
Dates
15-17 Sep 1999
Place
Portsmouth, NH (United States)

Optional Information

Notes
(c) 2000 American Institute of Physics.