Search Results - "Lommen, A. N."

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    Arecibo timing and single-pulse observations of 17 pulsars by Champion, D. J., Lorimer, D. R., McLaughlin, M. A., Xilouris, K. M., Arzoumanian, Z., Freire, P. C. C., Lommen, A. N., Cordes, J. M., Camilo, F.

    “…We report on timing and single-pulse observations of 17 pulsars discovered at the Arecibo Observatory. The highlights of our sample are the recycled pulsars…”
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    Journal Article
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    LIMITS ON THE STOCHASTIC GRAVITATIONAL WAVE BACKGROUND FROM THE NORTH AMERICAN NANOHERTZ OBSERVATORY FOR GRAVITATIONAL WAVES by Demorest, P B, Ferdman, R D, Gonzalez, M E, Nice, D, Ransom, S, Stairs, I H, Arzoumanian, Z, Brazier, A, BURKE-SPOLAOR, S, Chamberlin, S J

    Published in The Astrophysical journal (10-01-2013)
    “…We present an analysis of high-precision pulsar timing data taken as part of the North American Nanohertz Observatory for Gravitational Waves (NANOGrav)…”
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    PSR J0609+2130: a disrupted binary pulsar? by Lorimer, D. R., McLaughlin, M. A., Arzoumanian, Z., Xilouris, K. M., Cordes, J. M., Lommen, A. N., Fruchter, A. S., Chandler, A. M., Backer, D. C.

    “…We report the discovery and initial timing observations of a 55.7-ms pulsar, J0609+2130, found during a 430-MHz drift-scan survey with the Arecibo radio…”
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    Masses, Parallax, and Relativistic Timing of the PSR J1713+0747 Binary System by Splaver, Eric M, Nice, David J, Stairs, Ingrid H, Lommen, Andrea N, Backer, Donald C

    Published in The Astrophysical journal (10-02-2005)
    “…We report on 12 years of observations of PSR J1713+0747, a pulsar in a 68 day orbit with a white dwarf. Pulse times of arrival were measured with uncertainties…”
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    The Parallax and Proper Motion of PSR J0030+0451 by Lommen, Andrea N, Kipphorn, Richard A, Nice, David J, Splaver, Eric M, Stairs, Ingrid H, Backer, Donald C

    Published in The Astrophysical journal (10-05-2006)
    “…We report the parallax and proper motion of millisecond pulsar J0030+0451, one of 13 known isolated millisecond pulsars in the disk of the Galaxy. We obtained…”
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    Measuring the mass of solar system planets using pulsar timing by Champion, D. J, Hobbs, G. B, Manchester, R. N, Edwards, R. T, Backer, D. C, Bailes, M, Bhat, N. D. R, Burke-Spolaor, S, Coles, W, Demorest, P. B, Ferdman, R. D, Folkner, W. M, Hotan, A. W, Kramer, M, Lommen, A. N, Nice, D. J, Purver, M. B, Sarkissian, J. M, Stairs, I. H, van Straten, W, Verbiest, J. P. W, Yardley, D. R. B

    Published 21-08-2010
    “…High-precision pulsar timing relies on a solar-system ephemeris in order to convert times of arrival (TOAs) of pulses measured at an observatory to the solar…”
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    Journal Article