Bulletin of the Lebedev Physics Institute

, Volume 46, Issue 7, pp 225–227 | Cite as

Search for Periodic Radio Emission of the Gamma Pulsar J0357+3205 in Individual Records at the Frequency of 111 MHz

  • S. A. Tyul’bashevEmail author
  • M. A. Kitaeva


Radio emission of the gamma pulsar J0357+3205 is searched in the meter wavelength range. Periodic radiation is found in one of the 1700 observation sessions performed. The average pulsar profile is single-component with a half-width of 20–25 ms. The pulsar flux density estimate is 14 mJy.


radio-quite pulsars observations at low frequencies data analysis 


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  1. 1.
    A. A. Abdo, M. Ackermann, M. Ajello, et al., Science 325, 840 (2009).ADSCrossRefGoogle Scholar
  2. 2.
    F. Camilo, P. S. Ray, S. M. Ransom, et al., Astrophys. J. 705, 1 (2009).ADSCrossRefGoogle Scholar
  3. 3.
    Pei Wang et al., Presentation at the Conference FPS7, China, Guangzhou, 2018, Google Scholar
  4. 4.
    S. A. Tyul’bashev, V. S. Tyul’bashev, M. A. Kitaeva et al., Astron. Rep. 61, 848 (2017).ADSCrossRefGoogle Scholar
  5. 5.
    V. I. Shishov, I. V. Chashei, V. V. Oreshko, et al., Astron. Rep. 60, 1067 (2016).ADSCrossRefGoogle Scholar
  6. 6.
    S. A. Tyul’bashev, V. S. Tyul’bashev, V. V. Oreshko, and S. V. Logvinenko, Astron. Rep. 60, 220 (2016).ADSCrossRefGoogle Scholar
  7. 7.
    M. Marelli, A. De Luca, D. Salvetti, et al., Aasrophys. J. 765, 36 (2013).ADSCrossRefGoogle Scholar

Copyright information

© Allerton Press, Inc. 2019

Authors and Affiliations

  1. 1.Pushchino Radio Astronomy ObservatoryLebedev Physical InstitutePushchino, Moscow regionRussia

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