First NuSTAR observations of the BL Lac - type blazar PKS 2155-304: constraints on the jet content and distribution of radiating particles
- SLAC National Accelerator Lab., Menlo Park, CA (United States); Stanford Univ., CA (United States)
- SLAC National Accelerator Lab., Menlo Park, CA (United States); Stanford Univ., CA (United States); Polish Academy of Sciences (PAS), Warsaw (Poland)
- California Institute of Technology (CalTech), Pasadena, CA (United States)
- Max Planck Inst. fuer Physik, Munich (Germany)
- SLAC National Accelerator Lab., Menlo Park, CA (United States); Stanford Univ., CA (United States); California State Univ., East Bay, Hayward, CA (United States)
- Univ. of Tokyo (Japan)
- Yale Univ., New Haven, CT (United States)
- Polish Academy of Sciences (PAS), Warsaw (Poland)
- Clemson Univ., SC (United States)
- Univ. de Savoie, Annecy-le-Vieux (France)
- Ecole Polytechnique, Palaiseau (France)
- California Institute of Technology (CalTech), Pasadena, CA (United States). Jet Propulsion Lab. (JPL)
- Durham Univ. (United Kingdom)
- Univ. of Toulouse (France); Centre National de la Recherche Scientifique (CNRS), Toulouse (France)
- Univ. of California, Berkeley, CA (United States)
- Technical Univ. of Denmark, Lyngby (Denmark)
- Univ. of California, Berkeley, CA (United States); Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
- ASI Science Data Center, Rome (Italy)
- Inst. of Physical and Chemical Research (RIKEN), Wako (Japan)
- Columbia Univ., New York, NY (United States)
- ASI Science Data Center, Rome (Italy); Istituto Nazionale di Astrofisica (INAF), Monteporzio (Italy)
- Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
- NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States)
Here we report the first hard X-ray observations with NuSTAR of the BL Lac-type blazar PKS 2155-304, augmented with soft X-ray data from XMM-Newton and γ-ray data from the Fermi Large Area Telescope, obtained in 2013 April when the source was in a very low flux state. A joint NuSTAR and XMM spectrum, covering the energy range 0.5–60 keV, is best described by a model consisting of a log-parabola component with curvature $$\beta ={0.3}_{-0.1}^{+0.2}$$ and a (local) photon index 3.04 ± 0.15 at photon energy of 2 keV, and a hard power-law tail with photon index 2.2 ± 0.4. The hard X-ray tail can be smoothly joined to the quasi-simultaneous γ-ray spectrum by a synchrotron self-Compton component produced by an electron distribution with index p = 2.2. Assuming that the power-law electron distribution extends down to γmin = 1 and that there is one proton per electron, an unrealistically high total jet power of Lp ~ 1047 erg s–1 is inferred. This can be reduced by two orders of magnitude either by considering a significant presence of electron–positron pairs with lepton-to-proton ratio $${n}_{{\rm{e}}+{\rm{e}}-}/{n}_{{\rm{p}}}\sim 30$$, or by introducing an additional, low-energy break in the electron energy distribution at the electron Lorentz factor γbr1 ~ 100. In either case, the jet composition is expected to be strongly matter-dominated.
- Research Organization:
- Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
- Sponsoring Organization:
- USDOE National Nuclear Security Administration (NNSA); National Aeronautics and Space Administration (NASA); Polish National Science Centre (NCN)
- Contributing Organization:
- Fermi-LAT Collaboration
- Grant/Contract Number:
- AC52-07NA27344; NNG08FD60C; 2015/18/E/ST9/00580; NNX14AQ07H
- OSTI ID:
- 1876966
- Report Number(s):
- LLNL-JRNL-837152; 1056887; TRN: US2307352
- Journal Information:
- The Astrophysical Journal (Online), Vol. 831, Issue 2; ISSN 1538-4357
- Publisher:
- IOP PublishingCopyright Statement
- Country of Publication:
- United States
- Language:
- English
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