Published February 1, 2013
| Version v1
Journal article
SHALON observations of High-Frequency- and Low-Frequency-Peaked BL Lac objects
Creators
- 1. P. N. Lebedev Physical Institute, Russian Academy of Science (Russian Federation)
Description
The BL Lac objects come in two subclasses: the 'low-frequency-peaked BL Lac objects' in which the synchrotron peak falls in the IR-optical range and the 'high-frequency-peaked BL Lac objects' where it falls in the UV-X-ray bands. The observation results of high-frequency peaked BL Lac object: Mkn421 (z = 0.031), Mkn501 (z = 0.034), Mkn 180 (z = 0.045) and low-frequency peaked BL Lac object OJ 287 (z=0.306) are presented with integral spectra, images and spectral energy distributions combined with those in all broad energy range. Mkn 180 and OJ 287 blazars were recently detected by SHALON Cherenkov telescopic system.
Availability note (English)
Available from http://dx.doi.org/10.1088/1742-6596/409/1/012112Additional details
Identifiers
Publishing Information
- Journal Title
- Journal of Physics. Conference Series (Online)
- Journal Volume
- 409
- Journal Issue
- 1
- Journal Page Range
- [5 p.]
- ISSN
- 1742-6596
Conference
- Title
- 23. European cosmic ray symposium; 32. Russian cosmic ray conference
- Dates
- 3-7 Jul 2012
- Place
- Moscow (Russian Federation)
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 44061723
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ASTROPHYSICS; BL LACERTAE OBJECTS; CHERENKOV COUNTERS; COSMIC RAY DETECTION; ENERGY SPECTRA; FREQUENCY DEPENDENCE; INFRARED RADIATION; MOUNTAINS; RADIOWAVE RADIATION; SYNCHROTRON RADIATION; TELESCOPE COUNTERS; VISIBLE RADIATION; X RADIATION
- Descriptors DEC
- BREMSSTRAHLUNG; COSMIC RADIO SOURCES; DETECTION; ELECTROMAGNETIC RADIATION; IONIZING RADIATIONS; MEASURING INSTRUMENTS; PHYSICS; RADIATION DETECTION; RADIATION DETECTORS; RADIATIONS; SPECTRA