Published April 10, 2009 | Version v1
Journal article

MULTIWAVELENGTH OBSERVATIONS OF MARKARIAN 421 IN 2005-2006

  • 1. High Energy Physics Division, Argonne National Laboratory, 9700 South Cass Avenue, Argonne, IL 60439 (United States)
  • 2. Department of Physical and Life Sciences, Galway-Mayo Institute of Technology, Dublin Road, Galway, Republic of Ireland (Ireland)
  • 3. School of Physics and Astronomy, University of Leeds, Leeds, LS2 9JT (United Kingdom)
  • 4. Department of Physics, Washington University, St. Louis, MO 63130 (United States)
  • 5. School of Physics, University College Dublin, Belfield, Dublin 4, Republic of Ireland (Ireland)
  • 6. Department of Physics and Astronomy, University of California, Los Angeles, CA 90095 (United States)
  • 7. School of Physics, National University of Ireland, Galway, Republic of Ireland (Ireland)
  • 8. Astronomy Department, Adler Planetarium and Astronomy Museum, Chicago, IL 60605 (United States)
  • 9. Physics Department, McGill University, Montreal, QC H3A 2T8 (Canada)
  • 10. Department of Astronomy and Astrophysics, 525 Davey Lab., Penn. State University, University Park, PA 16802 (United States)
  • 11. Department of Physics, Purdue University, West Lafayette, IN 47907 (United States)
  • 12. Department of Physics and Astronomy, Barnard College, Columbia University, NY 10027 (United States)

Description

Since 2005 September, the Whipple 10 m Gamma-ray Telescope has been operated primarily as a blazar monitor. The five northern hemisphere blazars that have already been detected at the Whipple Observatory, Markarian 421 (Mrk 421), H1426+428, Mrk 501, 1ES 1959+650, and 1ES 2344+514, are monitored routinely each night that they are visible. We report on the Mrk 421 observations taken from 2005 November to 2006 June in the gamma-ray, X-ray, optical, and radio bands. During this time, Mrk 421 was found to be variable at all wavelengths probed. Both the variability and the correlations among different energy regimes are studied in detail here. A tentative correlation, with large spread, was measured between the X-ray and gamma-ray bands, while no clear correlation was evident among the other energy bands. In addition to this, the well-sampled spectral energy distribution of Mrk 421 (1101+384) is presented for three different activity levels. The observations of the other blazar targets will be reported separately.

Availability note (English)

Available from http://dx.doi.org/10.1088/0004-637X/695/1/596

Additional details

Identifiers

Publishing Information

Journal Title
Astrophysical Journal
Journal Volume
695
Journal Issue
1
Journal Page Range
p. 596-618
ISSN
0004-637X
CODEN
ASJOAB

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
41039648
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
ACTIVITY LEVELS; BL LACERTAE OBJECTS; ENERGY SPECTRA; GAMMA RADIATION; NORTHERN HEMISPHERE; TELESCOPES; WAVELENGTHS
Descriptors DEC
COSMIC RADIO SOURCES; EARTH PLANET; ELECTROMAGNETIC RADIATION; IONIZING RADIATIONS; PLANETS; RADIATIONS; SPECTRA