Abstract:
We report on TeV γ-ray observations of the blazar Mrk421 (redshift of 0.031) with the VERITAS observatory and the Whipple 10 m Cherenkov telescope. The excellent sensitivity of VERITAS allowed us to sample the TeV γ-ray fluxes and energy spectra with unprecedented accuracy where Mrk421 was detected in each of the pointings. A total of 47.3 hr of VERITAS and 96 hr of Whipple 10 m data were acquired between 2006 January and 2008 June. We present the results of a study of the TeV γ-ray energy spectra as a function of time and for different flux levels. On 2008 May 2 and 3, bright TeV γ-ray flares were detected with fluxes reaching the level of 10 Crab. The TeV γ-ray data were complemented with radio, optical, and X-ray observations, with flux variability found in all bands except for the radio wave band. The combination of the Rossi X-ray Timing Explorer and Swift X-ray data reveal spectral hardening with increasing flux levels, often correlated with an increase of the source activity in TeV γ-rays. Contemporaneous spectral energy distributions were generated for 18 nights, each of which are reasonably described by a one-zone synchrotron self-Compton model. © 2011. The American Astronomical Society. All rights reserved.
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Citas:
---------- APA ----------
(2011)
. TeV and multi-wavelength observations of Mrk421 in 2006-2008. Astrophysical Journal, 738(1).
http://dx.doi.org/10.1088/0004-637X/738/1/25---------- CHICAGO ----------
Acciari, V.A.
"TeV and multi-wavelength observations of Mrk421 in 2006-2008"
. Astrophysical Journal 738, no. 1
(2011).
http://dx.doi.org/10.1088/0004-637X/738/1/25---------- MLA ----------
Acciari, V.A.
"TeV and multi-wavelength observations of Mrk421 in 2006-2008"
. Astrophysical Journal, vol. 738, no. 1, 2011.
http://dx.doi.org/10.1088/0004-637X/738/1/25---------- VANCOUVER ----------
Acciari, V.A. TeV and multi-wavelength observations of Mrk421 in 2006-2008. Astrophys. J. 2011;738(1).
http://dx.doi.org/10.1088/0004-637X/738/1/25