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  ERRATUM: Timing of five millisecond pulsars discovered in the PALFA survey (2015, ApJ, 800, 123)

Scholz, P., Kaspi, V. M., Lyne, A. G., Stappers, B. W., Bogdanov, S., Cordes, J. M., et al. (2015). ERRATUM: Timing of five millisecond pulsars discovered in the PALFA survey (2015, ApJ, 800, 123). Astrophysical Journal, 805(1): 85. doi:10.1088/0004-637X/805/1/85.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0027-BCA3-8 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0027-BCA4-6
Genre: Journal Article

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 Creators:
Scholz, P., Author
Kaspi, V. M., Author
Lyne, A. G., Author
Stappers, B. W., Author
Bogdanov, S., Author
Cordes, J. M., Author
Crawford, F., Author
Ferdman, R. D., Author
Freire, P. C. C., Author
Hessels, J. W. T., Author
Lorimer, D. R., Author
Stairs, I. H., Author
Allen, B.1, Author              
Brazier, A., Author
Camilo, F., Author
Cardoso, R. F., Author
Chatterjee, S., Author
Deneva, J. S., Author
Jenet, F. A., Author
Karako-Argaman, C., Author
Knispel, B.1, Author              Lazarus, P., AuthorLee, K. J., Authorvan Leeuwen, J., AuthorLynch, R., AuthorMadsen, E. C., AuthorMcLaughlin, M. A., AuthorRansom, S. M., AuthorSiemens, X., AuthorSpitler, L. G., AuthorStovall, K., AuthorSwiggum, J. K., AuthorVenkataraman, A., AuthorZhu, W. 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, High Energy Astrophysical Phenomena, astro-ph.HE
 Abstract: We present the discovery of five millisecond pulsars (MSPs) from the PALFA Galactic plane survey using Arecibo. Four of these (PSRs J0557+1551, J1850+0244, J1902+0300, and J1943+2210) are binary pulsars whose companions are likely white dwarfs, and one (PSR J1905+0453) is isolated. Phase-coherent timing solutions, ranging from $\sim$1 to $\sim$3 years in length, and based on observations from the Jodrell Bank and Arecibo telescopes, provide precise determinations of spin, orbital, and astrometric parameters. All five pulsars have large dispersion measures ($>100$ pc cm$^{-3}$, within the top 20% of all known Galactic field MSPs) and are faint (1.4 GHz flux density < 0.1 mJy, within the faintest 5% of all known Galactic field MSPs), illustrating PALFA's ability to find increasingly faint, distant MSPs in the Galactic plane. In particular, PSR J1850+0244 has a dispersion measure of 540 pc cm$^{-3}$, the highest of all known MSPs. Such distant, faint MSPs are important input for accurately modeling the total Galactic MSP population.

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 Dates: 2015-01-152015
 Publication Status: Published in print
 Pages: 12 pages, 7 figures, ApJ in press
 Publishing info: -
 Table of Contents: -
 Rev. Method: -
 Identifiers: DOI: 10.1088/0004-637X/805/1/85
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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: 805 (1) Sequence Number: 85 Start / End Page: - Identifier: ISSN: 0004-637X
CoNE: https://pure.mpg.de/cone/journals/resource/954922828215_2