Data

Parkes observations for project P262 semester 2006APRS

Commonwealth Scientific and Industrial Research Organisation
Manchester, Dick ; Lewis, Dion ; Sarkissian, John ; Hobbs, George
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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:doi10.4225/08/520048D7143BF&rft.title=Parkes observations for project P262 semester 2006APRS&rft.identifier=https://doi.org/10.4225/08/520048D7143BF&rft.publisher=Commonwealth Scientific and Industrial Research Organisation&rft.description=Young pulsars are of interest in several different ways: they are sometimesassociated with supernova remnants, they sometimes have high-energy(optical, X-ray, gamma-ray) pulsed emission, and they usually havesignificant period variations and often suffer glitches. We propose frequentmonitoring of the period of about 35 mostly young pulsars to providea database for high-energy, ATCA and LBA observations of pulsars and toinvestigate variations in their period.&rft.creator=Manchester, Dick &rft.creator=Lewis, Dion &rft.creator=Sarkissian, John &rft.creator=Hobbs, George &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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Creative Commons Attribution 3.0 Unported Licence
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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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Young pulsars are of interest in several different ways: they are sometimes
associated with supernova remnants, they sometimes have high-energy
(optical, X-ray, gamma-ray) pulsed emission, and they usually have
significant period variations and often suffer glitches. We propose frequent
monitoring of the period of about 35 mostly young pulsars to provide
a database for high-energy, ATCA and LBA observations of pulsars and to
investigate variations in their period.

Available: 2013-08-06

Data time period: 2006-04-01 to 2006-09-30

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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