Abstract
Exceptionally strong and long-lasting flaring activity of the blazar Mrk 421 occurred between 2001 January and March. Based on the excellent signal-to-noise ratio of the data, we derive the energy spectrum between 260 GeV and 17 TeV with unprecedented statistical precision. The spectrum is not well described by a simple power law even with a curvature term. Instead, the data can be described by a power law with exponential cutoff: DN/dE ∝ E-2.14±0.03statℓ-E/E0m-2S-2 TeV-1 with E0=4.3±0.3statTeV.Mrk 421 is the second -ray blazar that 0 stat unambiguously exhibits an absorption-like feature in its spectral energy distribution at 3-6 TeV.
Original language | English |
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Pages (from-to) | L45-L48 |
Journal | Astrophysical Journal Letters |
Volume | 560 |
Issue number | 1 |
DOIs | |
State | Published - Oct 10 2001 |
Keywords
- BL Lacertae Objects: Individual (Markarian 421)-Gamma Rays: Observations