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Gamma-ray emission from PSR J0007+7303 using seven year

Journal Article · · The Astrophysical Journal (Online)
 [1];  [2];  [1];  [3];  [1]
  1. Institute of Space Sciences (CSIC–IEEC), Barcelona (Spain)
  2. Institute of Space Sciences (CSIC–IEEC) and Catalan Institution for Research and Advanced Studies (ICREA), Barcelona (Spain)
  3. Institute of Space Sciences (CSIC–IEEC), Barcelona (Spain); Univ. of Amsterdam (Netherlands). Astronomical Inst. Anton Pannekoek
We report on a detailed analysis of the bright gamma-ray pulsar (PSR) J0007+7303, based on more than seven years of Fermi Large Area Telescope Pass 8 data. We also confirm that PSR J0007+7303 is significantly detected as a point source also during the off-peak phases with a test statistic value of 262 (~16σ). In the description of the off-peak spectrum of PSR J0007+7303, a power law with an exponential cutoff at 2.7 ± 1.2 ± 1.3 GeV (the first/second uncertainties correspond to statistical/systematic errors) is preferred over a single power law at a level of 3.5σ. The possible existence of a cutoff hints at a magnetospheric origin of the emission. In addition, no extended gamma-ray emission is detected that is compatible with either the supernova remnant (CTA 1) or the very high-energy (>100 GeV) pulsar wind nebula. A flux upper limit of 6.5 × 10-12 erg cm-2 s-1 in the energy range 10–300 GeV is reported, for an extended source assuming the morphology of the VERITAS detection. During on-peak phases, a sub-exponential cutoff is significantly preferred (~11σ) for representing the spectral energy distribution, in both the phase-averaged and phase-resolved spectra. Furthermore, three glitches are detected during the observation period and we found no flux variability at the time of the glitches or in the long-term behavior. We also report the discovery of a previously unknown gamma-ray source in the vicinity of PSR J0007+7303, Fermi J0020+7328, which we associate with the z = 1.781 quasar S5 0016+73. A concurrent analysis of this source is needed to correctly characterize the behavior of CTA 1 and it is also presented in the paper.
Research Organization:
SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
Sponsoring Organization:
USDOE
Grant/Contract Number:
AC02-76SF00515
OSTI ID:
1355711
Alternate ID(s):
OSTI ID: 22667279
Journal Information:
The Astrophysical Journal (Online), Journal Name: The Astrophysical Journal (Online) Journal Issue: 1 Vol. 831; ISSN 1538-4357
Publisher:
Institute of Physics (IOP)Copyright Statement
Country of Publication:
United States
Language:
English

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Cited By (6)

Order parameters for the high-energy spectra of pulsars journal February 2018
Prospects for the detection of high-energy (E > 25 GeV) Fermi pulsars with the Cherenkov Telescope Array journal June 2017
Spectral characterization of the non-thermal X-ray emission of gamma-ray pulsars journal December 2019
Observing and Modeling the Gamma-Ray Emission from Pulsar/Pulsar Wind Nebula Complex PSR J0205+6449/3C 58 journal May 2018
Order parameters for the high-energy spectra of pulsars text January 2018
Observing and modeling the gamma-ray emission from pulsar/pulsar wind nebula complex PSR J0205+6449/3C 58 text January 2018

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