Variations of the TeV energy spectrum at different flux levels of Mkn 421 observed with the HEGRA system of Cherenkov telescopes

Free access article

Issue		A&A Volume 393, Number 1, October I 2002


Page(s)		89 - 99
Section		Extragalactic astronomy
DOI		http://dx.doi.org/10.1051/0004-6361:20021005

A&A 393, 89-99 (2002)
DOI: 10.1051/0004-6361:20021005

Variations of the TeV energy spectrum at different flux levels of Mkn 421 observed with the HEGRA system of Cherenkov telescopes

F. Aharonian¹, A. Akhperjanian², M. Beilicke³, K. Bernlöhr¹, H. Börst⁴, H. Bojahr⁵, O. Bolz¹, T. Coarasa⁶, J. Contreras⁶, J. Cortina⁶, L. Costamante¹, S. Denninghoff⁶, V. Fonseca⁷, M. Girma¹, N. Götting³, G. Heinzelmann³, G. Hermann¹, A. Heusler¹, W. Hofmann¹, D. Horns¹, I. Jung¹, R. Kankanyan¹, M. Kestel⁶, J. Kettler¹, A. Kohnle¹, A. Konopelko¹, H. Kornmeyer⁶, D. Kranich⁶, H. Krawczynski^{1, 8}, H. Lampeitl¹, M. Lopez⁷, E. Lorenz⁶, F. Lucarelli⁷, O. Mang⁴, H. Meyer⁵, R. Mirzoyan⁶, M. Milite³, A. Moralejo⁷, E. Ona⁷, M. Panter¹, A. Plyasheshnikov^{1, 9}, G. Pühlhofer¹, G. Rauterberg⁴, R. Reyes⁶, W. Rhode⁵, J. Ripken³, G. Rowell¹, V. Sahakian², M. Samorski⁴, M. Schilling⁴, M. Siems⁴, D. Sobzynska^{6, 10}, W. Stamm⁴, M. Tluczykont³, H.J. Völk¹, C. A. Wiedner¹, W. Wittek⁶ and R. A. Remillard¹¹

¹ Max-Planck-Institut für Kernphysik, Postfach 103980, 69029 Heidelberg, Germany
² Yerevan Physics Institute, Alikhanian Br. 2, 375036 Yerevan, Armenia
³ Universität Hamburg, Institut für Experimentalphysik, Luruper Chaussee 149, 22761 Hamburg, Germany
⁴ Universität Kiel, Institut für Experimentelle und Angewandte Physik, Leibnizstraße 15-19, 24118 Kiel, Germany
⁵ Universität Wuppertal, Fachbereich Physik, Gaußstr. 20, 42097 Wuppertal, Germany
⁶ Max-Planck-Institut für Physik, Föhringer Ring 6, 80805 München, Germany
⁷ Universidad Complutense, Facultad de Ciencias Físicas, Ciudad Universitaria, 28040 Madrid, Spain
⁸ Now at Yale University, PO Box 208101, New Haven, CT 06520-8101, USA
⁹ On leave from Altai State University, Dimitrov Street 66, 656099 Barnaul, Russia
¹⁰ Home institute: University Lodz, Poland
¹¹ Center for Space Research, MIT, Cambridge, MA02139

(Received 31 May 2002 / Accepted 5 July 2002)

Abstract
The nearby BL Lacertae (BL Lac) object Markarian 421 ( Mkn 421 ) at a red shift z=0.031 was observed to undergo strong TeV $\gamma$ -ray outbursts in the observational periods from December 1999 until May 2001. The time averaged flux level $F(E>1{\rm\,TeV})$ in the 1999/2000 season was $(1.43\pm0.04)$ $\times$ 10^-11 ph cm ^-2 s ^-1, whereas in the 2000/2001 season the average integral flux increased to $(4.19\pm0.04)$ $\times$ 10^-11 ph cm ^-2 s ^-1. Both energy spectra are curved and well fit by a power law with an exponential cut-off energy at $3.6(+0.4-0.3)_{\rm stat}(+0.9-0.8)_{\rm sys}$ TeV. The respective energy spectra averaged over each of the two time periods indicate a spectral hardening for the 2000/2001 spectrum. The photon index changes from $2.39\pm0.09_{\rm stat}$ for 1999/2000 to $2.19\pm0.02_{\rm stat}$ in 2000/2001. The energy spectra derived for different average flux levels ranging from 0.5 to 10 $\times$ 10^-11 ph cm ^-2 s ^-1 follow a clear correlation of photon index and flux level. Generally, the energy spectra are harder for high flux levels. From January to April 2001 Mkn 421 showed rapid variability (doubling time as short as 20 min), accompanied with a spectral hardening with increasing flux level within individual nights. For two successive nights (MJD 51989-51991, March 21-23, 2001), this correlation of spectral hardness and change in flux has been observed within a few hours. The cut-off energy for the Mkn 421 TeV spectrum remains within the errors constant for the different flux levels and differs by $\Delta E=2.6\pm0.6_{\rm stat}\pm0.6_{\rm sys}$ TeV from the value determined for Mkn 501. This indicates that the observed exponential cut-off in the energy spectrum of Mkn 421 is not solely caused by absorption of multi-TeV photons by pair-production processes with photons of the extragalactic near/mid infrared background radiation.

Key words: gamma rays: observations -- BL Lacertae objects: individual: Mkn 421

Offprint request: D. Horns, Dieter.Horns@mpi-hd.mpg.de

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