Data

Parkes observations for project P794 semester 2011APRS

Commonwealth Scientific and Industrial Research Organisation
Verbiest, Joris P.W. ; Kramer, Michael ; Antoniadis, John ; Tauris, Thomas
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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:doi10.4225/08/52352D662A610&rft.title=Parkes observations for project P794 semester 2011APRS&rft.identifier=https://doi.org/10.4225/08/52352D662A610&rft.publisher=Commonwealth Scientific and Industrial Research Organisation&rft.description=We propose timing observations of the millisecond pulsar J1933-6211, which is likely to be the least heavy neutron star known. Measurement of its mass will have significant impact on stellar evolution scenarios, accretion efficiencies and neutron star formation scenarios. In addition to this, the pulsar may well be a good candidate for inclusion in pulsar timing array efforts. \r\rThis proposal is an initial, limited time request to attempt to a) place a strong limit on the pulsar mass, b) attempt to phase-connect the archival data, c) enable detailed analysis of which observations will be needed for precise measurement of the pulsar mass and d) determined if the pulsar can be timed precisely enough to be included in timing array efforts.&rft.creator=Verbiest, Joris P.W. &rft.creator=Kramer, Michael &rft.creator=Antoniadis, John &rft.creator=Tauris, Thomas &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=pulsars&rft_subject=neutron stars&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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All Rights (including copyright) CSIRO Australia 2011.

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We propose timing observations of the millisecond pulsar J1933-6211, which is likely to be the least heavy neutron star known. Measurement of its mass will have significant impact on stellar evolution scenarios, accretion efficiencies and neutron star formation scenarios. In addition to this, the pulsar may well be a good candidate for inclusion in pulsar timing array efforts. \r
\r
This proposal is an initial, limited time request to attempt to a) place a strong limit on the pulsar mass, b) attempt to phase-connect the archival data, c) enable detailed analysis of which observations will be needed for precise measurement of the pulsar mass and d) determined if the pulsar can be timed precisely enough to be included in timing array efforts.

Available: 2013-09-15

Data time period: 2011-04-01 to 2011-09-30

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Subjects
Astronomical Sciences | Astronomical Sciences Not Elsewhere Classified | Physical Sciences | neutron stars | pulsars |

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Identifiers
ACN 633 798 857