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  Timing and Interstellar Scattering of Thirty-five Distant Pulsars Discovered in the PALFA Survey

Nice, D. J., Altiere, E., Bogdanov, S., Cordes, J. M., Farrington, D., Hessels, J. W. T., et al. (2013). Timing and Interstellar Scattering of Thirty-five Distant Pulsars Discovered in the PALFA Survey. Astrophysical Journal, 772: 50. doi:10.1088/0004-637X/772/1/50.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0014-9A56-3 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0014-9A57-1
Genre: Journal Article

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 Creators:
Nice, D. J., Author
Altiere, E., Author
Bogdanov, S., Author
Cordes, J. M., Author
Farrington, D., Author
Hessels, J. W. T., Author
Kaspi, V. M., Author
Lyne, A. G., Author
Popa, L., Author
Ransom, S. M., Author
Sanpa-arsa, S., Author
Stappers, B. W., Author
Wang, Y., Author
Allen, B.1, Author              
Bhat, N. D. R., Author
Brazier, A., Author
Camilo, F., Author
Champion, D. J., Author
Chatterjee, S., Author
Crawford, F., Author
Deneva, J. S., AuthorDesvignes, G., AuthorFreire, P. C. C., AuthorJenet, F. A., AuthorKnispel, B.1, Author              Lazarus, P., AuthorLee, K. J., Authorvan Leeuwen, J., AuthorLorimer, D. R., AuthorLynch, R., AuthorMcLaughlin, M. A., AuthorScholz, P., AuthorSiemens, X., AuthorStairs, I. H., AuthorStovall, K., AuthorVenkataraman, A., AuthorZhu, W., Author more..
Affiliations:
1Observational Relativity and Cosmology, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, ou_24011              

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Free keywords: Astrophysics, Solar and Stellar Astrophysics, astro-ph.SR, Astrophysics, High Energy Astrophysical Phenomena, astro-ph.HE
 Abstract: We have made extensive observations of 35 distant slow (non-recycled) pulsars discovered in the ongoing Arecibo PALFA pulsar survey. Timing observations of these pulsars over several years at Arecibo Observatory and Jodrell Bank Observatory have yielded high-precision positions and measurements of rotation properties. Despite being a relatively distant population, these pulsars have properties that mirror those of the previously known pulsar population. Many of the sources exhibit timing noise, and one underwent a small glitch. We have used multifrequency data to measure the interstellar scattering properties of these pulsars. We find scattering to be higher than predicted along some lines of sight, particularly in the Cygnus region. Lastly, we present XMM-Newton and Chandra observations of the youngest and most energetic of the pulsars, J1856+0245, which has previously been associated with the GeV-TeV pulsar wind nebula HESS J1857+026.

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 Dates: 2013-04-272013-07-072013
 Publication Status: Published in print
 Pages: Published in the Astrophysical Journal
 Publishing info: -
 Table of Contents: -
 Rev. Method: -
 Identifiers: arXiv: 1304.7370
DOI: 10.1088/0004-637X/772/1/50
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Title: Astrophysical Journal
Source Genre: Journal
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Publ. Info: Chicago, IL : University of Chicago Press for the American Astronomical Society
Pages: - Volume / Issue: 772 Sequence Number: 50 Start / End Page: - Identifier: ISSN: 0004-637X
CoNE: /journals/resource/954922828215_2