3-11 July 2007
Merida, Mexico
Mexico/General timezone
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Contribution Poster

Merida, Mexico - Regency (Hyatt)

STACEE Observations of 1ES 1218+304

Speakers

  • Reshmi MUKHERJEE

Primary authors

Co-authors

  • Naureen AKHTER (Dept. of Physics & Astronomy, Barnard College, Columbia University, New York, NY 10027)
  • J. BALL (Department of Physics and Astronomy, University of California, Los Angeles, CA 90095)
  • J. E. CARSON (Department of Physics and Astronomy, University of California, Los Angeles, CA 90095 (Current address: Stanford Linear Accelerator Center, MS 29, Menlo Park, CA 94025))
  • C. E. COVAULT (Department of Physics, Case Western Reserve University, Cleveland, OH 44106)
  • D. D. DRISCOLL (Department of Physics, Case Western Reserve University, Cleveland, OH 44106)
  • P. FORTIN (Department of Physics, McGill University, Montreal, QC H3A 2T8, Canada (Current Address: Department of Physics and Astronomy, Barnard College, Columbia University, New York, NY 10027))
  • D. M. GINGRICH (Department of Physics, University of Alberta, Edmonton, AB T6G 2G7 Canada & TRIUMF, Vancouver, BC V6T 2A3 Canada)
  • D. S. HANNA (Department of Physics, McGill University, Montreal, QC H3A 2T8, Canada)
  • A. JARVIS (Department of Physics and Astronomy, University of California, Los Angeles, Los Angeles, CA 90095)
  • J. KILDEA (Department of Physics, McGill University, Montreal, QC H3A 2T8, Canada (Current address: Fred Lawrence Whipple Observatory, Harvard-Smithsonian Center for Astrophysics, Amado, AZ 85645))
  • T. LINDNER (Department of Physics, McGill University, Montreal, QC H3A 2T8, Canada (Current Address: Department of Physics and Astronomy, University of British Columbia, Vancouver, BC V6T 1Z1, Canada))
  • C. E. MUELLER (Department of Physics, McGill University, Montreal, QC H3A 2T8, Canada)
  • R. A. ONG (Department of Physics and Astronomy, University of California, Los Angeles, Los Angeles, CA 90095)
  • K. RAGAN (Department of Physics, McGill University, Montreal, QC H3A 2T8, Canada)
  • D. A. WILLIAMS (Santa Cruz Institute for Particle Physics, University of California, Santa Cruz, Santa Cruz, CA 95064)
  • J. ZWEERINK (Department of Physics and Astronomy, University of California, Los Angeles, Los Angeles, CA 90095)

Abstract content

We present the analysis and results of recent high-energy gamma-ray observations of the high energy-peaked BL Lac (HBL) object 1ES 1218+304 with the Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE). 1ES 1218+304 is an X-ray bright HBL at a redshift z=0.182, and has been predicted to emit high energy gamma rays above 100 GeV, detectable by ground-based Cherenkov telescopes. Recently, this source has been detected by MAGIC and VERITAS, confirming these predictions. STACEE's sensitivity to astrophysical sources at energies above 100 GeV allows it to explore high energy sources such as X-ray bright active galaxies and gamma-ray bursts. We will present results from STACEE observations of 1ES 1218+304 in the 2006-2007 observing season.

If this papers is presented for a collaboration, please specify the collaboration

STACEE collaboration

Reference

Proceedings of the 30th International Cosmic Ray Conference; Rogelio Caballero, Juan Carlos D'Olivo, Gustavo Medina-Tanco, Lukas Nellen, Federico A. Sánchez, José F. Valdés-Galicia (eds.); Universidad Nacional Autónoma de México, Mexico City, Mexico, 2008; Vol. 3 (OG part 2), pages 925-928