Simultaneous X‐Ray and TeV Gamma‐Ray Observation of the TeV Blazar Markarian 421 during 2000 February and May
The Astrophysical Journal(2001)
Abstract
We present the results of simultaneous observations of the TeV blazar Markarian 421 at X-ray and TeV gamma-ray energies with the Rossi X-Ray T iming Explorer and the stereoscopic Cerenkov telescope system of the High Energy Gamma-Ray Astronomy (HEGRA) experiment, respectively. The source was monitored from 2000 February 2 to 16 and from 2000 May 3 to 8. In both energy bands several Ñares with very rapid Ñux variability were observed. In the X-ray band, the Ñux increased and decreased with e-folding times as short as about 5 hr. The 3È20 keV photon index varied between values of 2.2 and 2.9. For Ðve pointings the data show statistically signiÐcant evidence for spectral curvature. The photon index varied substantially on very short timescales : on 2000 February 11 it hardened within 1.6 hr by *!\ 0.18, and on February 14 it softened within 1.6 hr by *!\ 0.2. The TeV observations of February 7/8 showed statistically signiÐcant evidence for substantial TeV Ñux variability on a 30 minute timescale. The TeV energy spectrum averaged over all the observations of the campaign shows a similar steep slope as in earlier HEGRA observations : TeV)~! with dN/dE\N0(E/1 N0\ (25 ^ 1stat)] 10~12 photons cm~2 s~1 TeV~1 and Within statistical errors no evidence for a curvature of !\ 2.94^ stat the TeV energy spectrum is found. We show the results of modeling the data with a time-dependent homogeneous synchrotron self-Compton model. The X-ray and TeV gamma-ray emission strengths and energy spectra together with the rapid Ñux variability strongly suggest that the emission volume is approaching the observer with a Doppler factor of 50 or higher. The di†erent Ñux variability timescales observed at X-rays and TeV gamma rays indicate that a more detailed analysis will require inhomogeneous models with several emission zones. Subject headings : BL Lacertae objects : individual (Markarian 421) È galaxies : jets È gamma rays : observations
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Key words
BL Lacertae objects : individual (Markarian 421),galaxies : jets,gamma rays : observations
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