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Parkes observations for project P574 semester 2019OCTS_03

Commonwealth Scientific and Industrial Research Organisation
Sobey, Charlotte ; Possenti, Andrea ; Manchester, Dick ; Johnston, Simon ; Hobbs, George ; Weltevrede, Patrick ; Kerr, Matthew ; Shannon, Ryan ; Dai, Shi ; Kumamoto, Hiroki
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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:doi10.25919/5de58250e7e99&rft.title=Parkes observations for project P574 semester 2019OCTS_03&rft.identifier=https://doi.org/10.25919/5de58250e7e99&rft.publisher=Commonwealth Scientific and Industrial Research Organisation&rft.description=We request time to observe 260 pulsars on a regular basis to provide the accurate ephemerides necessary for the detection and characterisation of gamma-ray pulsars with the Fermi satellite. The primary 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 investigate: neutron stars and pulsar emission via detecting glitches and determining pulse timing parameters; and the ISM via measuring and monitoring dispersion measures, Faraday rotation measures, and scintillation. To date, we are (co-)authors on 75 papers arising from the collaboration and P574 data. The data have contributed to the PhD theses of students from Bordeaux, Manchester, Oxford, Stanford, and Swinburne.&rft.creator=Sobey, Charlotte &rft.creator=Possenti, Andrea &rft.creator=Manchester, Dick &rft.creator=Johnston, Simon &rft.creator=Hobbs, George &rft.creator=Weltevrede, Patrick &rft.creator=Kerr, Matthew &rft.creator=Shannon, Ryan &rft.creator=Dai, Shi &rft.creator=Kumamoto, Hiroki &rft.date=2019&rft.edition=v1&rft_rights=Creative Commons Attribution 4.0 International Licence https://creativecommons.org/licenses/by/4.0/&rft_rights=Data is accessible online and may be reused in accordance with licence conditions&rft_rights=All Rights (including copyright) CSIRO 2019.&rft_subject=pulsars&rft_subject=neutron stars&rft_subject=interstellar medium in and around the Milky Way&rft_subject=P574_2019OCTS&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 4.0 International Licence
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Data is accessible online and may be reused in accordance with licence conditions

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Brief description

We request time to observe 260 pulsars on a regular basis to provide the accurate ephemerides necessary for the detection and characterisation of gamma-ray pulsars with the Fermi satellite. The primary 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 investigate: neutron stars and pulsar emission via detecting glitches and determining pulse timing parameters; and the ISM via measuring and monitoring dispersion measures, Faraday rotation measures, and scintillation. To date, we are (co-)authors on 75 papers arising from the collaboration and P574 data. The data have contributed to the PhD theses of students from Bordeaux, Manchester, Oxford, Stanford, and Swinburne.

Available: 2019-12-03

Data time period: 2019-10-01 to 2020-03-31

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Astronomical Sciences | Astronomical Sciences Not Elsewhere Classified | P574_2019OCTS | Physical Sciences | interstellar medium in and around the Milky Way | neutron stars | pulsars |

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