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pro vyhledávání: '"Haydon S. Knight"'
Autor:
Haydon S. Knight
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 378:723-729
We report on 685-MHz observations of PSR J1823-3021A using the Parkes radio telescope. A total of 120 giant pulses (GPs) were found by searching for spiky emission at 16-(is time resolution. The energies of these pulses follow a power law that has a
Autor:
Haydon S. Knight
Publikováno v:
Chinese Journal of Astronomy and Astrophysics. 6:193-196
Several radio pulsars have now been shown to emit giant pulses that align in phase with high energy emission rather than with their integrated pulse components. We investigate whether timing of giant and γ-ray pulses can be used to improve limits on
Autor:
Haydon S. Knight
Publikováno v:
Chinese Journal of Astronomy and Astrophysics. 6:41-47
Evidence now exists that at least 14 pulsars emit distinctive pulses that are stronger and narrower than the average pulse. I review observations of these pulses in an effort to determine which sources share a common emission-mechanism. All of the gi
We report observations of Crab giant pulses made with the Australia Telescope Compact Array and a baseband recorder system, made simultaneously at two frequencies, 1300 and 1470 MHz. These observations were sensitive to pulses with amplitudes \ga 3 k
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::de316276b2d913abfe8417458803e973
http://arxiv.org/abs/0801.0334
http://arxiv.org/abs/0801.0334
Autor:
Glen Torr, Mervyn J. Lynch, Haydon S. Knight, Rachel L. Webster, Jamie Stevens, Frank H. Briggs, Colin J. Lonsdale, Randall B. Wayth, J. Stuart B. Wyithe, Divya Oberoi, Jonathon Kocz, Bruce Stansby, N. D. Ramesh Bhat, Roger J. Cappallo, David Herne, David G. Barnes, Judd D. Bowman
We report on the detection of giant pulses from the Crab Nebula pulsar at a frequency of 200 MHz using the field deployment system designed for the Mileura Widefield Array's Low Frequency Demonstrator (MWA-LFD). Our observations are among the first h
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b4fa5976f6d68b887bbe286fedddc254
We have conducted a search for giant pulses from four millisecond pulsars using the 100m Green Bank Telescope. Coherently dedispersed time-series from PSR J0218+4232 were found to contain giant pulses of very short intrinsic duration whose energies f
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::02e5df37c8fc090ecf67e1769816a54f
http://arxiv.org/abs/astro-ph/0512341
http://arxiv.org/abs/astro-ph/0512341
We have searched for microsecond-timescale broadband emission from a sample of eighteen millisecond pulsars. Our study places strong limits on such emission from several millisecond pulsars and shows that it is only present in a small subset of milli
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::304db56c3353d0e597de224943de8f76
Here we report timing measurements of the relativistic binary pulsar PSR J1141-6545 that constrain the component masses and demonstrate that the orbital period derivative \dot Pb = (-4+/-1)x10^-13 is consistent with gravitational wave emission as des
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d500aae7a968d221314936f3408401ad
http://arxiv.org/abs/astro-ph/0307468
http://arxiv.org/abs/astro-ph/0307468