Data

Parkes observations for project P602 semester 2007OCTS

Commonwealth Scientific and Industrial Research Organisation
Camilo, Fernando ; Reynolds, John
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ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Adc&rfr_id=info%3Asid%2FANDS&rft_id=info:doi10.4225/08/52292AE9B2D80&rft.title=Parkes observations for project P602 semester 2007OCTS&rft.identifier=https://doi.org/10.4225/08/52292AE9B2D80&rft.publisher=Commonwealth Scientific and Industrial Research Organisation&rft.description=We have detected dispersed radio pulsations positionally coincident witha magnetar candidate. If they arise from the magnetar, this would beonly the second such instance. On the other hand, maybe the candidateis not a magnetar - but the unusual radio pulsations are certainly real.We therefore wish to get to the bottom of this potentially very excitingdiscovery. The immediate need is to characterize the behavior of theradio emission, and over a period of approximately one year attempt toobtain a timing position to compare to the precisely-known position ofthe X-ray source.&rft.creator=Camilo, Fernando &rft.creator=Reynolds, John &rft.date=2013&rft.edition=v2&rft_rights=Creative Commons Attribution 3.0 Unported Licence https://creativecommons.org/licenses/by/3.0/&rft_rights=Data is accessible online and may be reused in accordance with licence conditions&rft_rights=All Rights (including copyright) CSIRO Australia 2011.&rft_subject=Stellar&rft_subject=Galactic&rft_subject=Astronomical sciences not elsewhere classified&rft_subject=Astronomical sciences&rft_subject=PHYSICAL SCIENCES&rft.type=dataset&rft.language=English Access the data
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Data is accessible online and may be reused in accordance with licence conditions

All Rights (including copyright) CSIRO Australia 2011.

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We have detected dispersed radio pulsations positionally coincident with
a magnetar candidate. If they arise from the magnetar, this would be
only the second such instance. On the other hand, maybe the candidate
is not a magnetar - but the unusual radio pulsations are certainly real.
We therefore wish to get to the bottom of this potentially very exciting
discovery. The immediate need is to characterize the behavior of the
radio emission, and over a period of approximately one year attempt to
obtain a timing position to compare to the precisely-known position of
the X-ray source.

Available: 2013-09-06

Data time period: 2007-04-01 to 2008-03-31

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Subjects
Astronomical Sciences | Astronomical Sciences Not Elsewhere Classified | Galactic | Physical Sciences | Stellar |

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Identifiers
ACN 633 798 857