Data

Parkes observations for project P574 semester 2014OCTS

Commonwealth Scientific and Industrial Research Organisation
Kerr, Matthew ; Possenti, Andrea ; Manchester, Dick ; Johnston, Simon ; Hobbs, George ; Romani, R ; Thompson, David J. ; Weltevrede, Patrick ; Shannon, Ryan ; Petroff, Emily ; Brook, Paul
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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:doi10.4225/08/57EE8426EDED3&rft.title=Parkes observations for project P574 semester 2014OCTS&rft.identifier=https://doi.org/10.4225/08/57EE8426EDED3&rft.publisher=Commonwealth Scientific and Industrial Research Organisation&rft.description=We request time to observe 230 pulsars on a regular basis in order to provide the accurate ephemerides necessary for the detection and characterisation of gamma-ray pulsars with the Fermi satellite. The main science goals are to increase the number of known gamma-ray pulsars (both radio loud and radio quiet), to determine accurate pulse profiles, and to characterise their high energy (phase-resolved) spectra. In the radio, the observations will also allow us to find glitches, characterise timing noise, investigate dispersion and rotation measure variability, and enhance our knowledge of single pulse phenomenology. To date, we\rare (co-)authors on 45 papers arising from the collaboration and P574 data. The data have contributed to the PhD theses of Lucas Guillemot and Damien Parent from the Bordeaux Fermi group and Kyle Watters from Stanford. Currently four students have active projects using the radio datasets.&rft.creator=Kerr, Matthew &rft.creator=Possenti, Andrea &rft.creator=Manchester, Dick &rft.creator=Johnston, Simon &rft.creator=Hobbs, George &rft.creator=Romani, R &rft.creator=Thompson, David J. &rft.creator=Weltevrede, Patrick &rft.creator=Shannon, Ryan &rft.creator=Petroff, Emily &rft.creator=Brook, Paul &rft.date=2015&rft.edition=v1&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 2015.&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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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 2015.

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We request time to observe 230 pulsars on a regular basis in order to provide the accurate ephemerides necessary for the detection and characterisation of gamma-ray pulsars with the Fermi satellite. The main science goals are to increase the number of known gamma-ray pulsars (both radio loud and radio quiet), to determine accurate pulse profiles, and to characterise their high energy (phase-resolved) spectra. In the radio, the observations will also allow us to find glitches, characterise timing noise, investigate dispersion and rotation measure variability, and enhance our knowledge of single pulse phenomenology. To date, we\r
are (co-)authors on 45 papers arising from the collaboration and P574 data. The data have contributed to the PhD theses of Lucas Guillemot and Damien Parent from the Bordeaux Fermi group and Kyle Watters from Stanford. Currently four students have active projects using the radio datasets.

Available: 2015-05-05

Data time period: 2014-10-01 to 2015-03-31

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ACN 633 798 857