Data

Parkes observations for project P574 semester 2018APRS_04

Commonwealth Scientific and Industrial Research Organisation
Dai, Shi ; Possenti, Andrea ; Manchester, R ; Johnston, Simon ; Hobbs, G ; Weltevrede, Patrick ; Kerr, Matthew ; Shannon, Ryan ; Ilie, Cristina-Diana ; Sobey, Charlotte
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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:doi10.25919/5b873ec46e5ac&rft.title=Parkes observations for project P574 semester 2018APRS_04&rft.identifier=10.25919/5b873ec46e5ac&rft.publisher=Commonwealth Scientific and Industrial Research Organisation (CSIRO)&rft.description=We request time to observe 260 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 are (co-)authors on 70 papers arising from the collaboration and P574 data. The data have contributed to the PhD theses of students from Bordeaux, Stanford, Swinburne and Oxford.&rft.creator=Dai, Shi &rft.creator=Possenti, Andrea &rft.creator=Manchester, R &rft.creator=Johnston, Simon &rft.creator=Hobbs, G &rft.creator=Weltevrede, Patrick &rft.creator=Kerr, Matthew &rft.creator=Shannon, Ryan &rft.creator=Ilie, Cristina-Diana &rft.creator=Sobey, Charlotte &rft.date=2018&rft.edition=v1&rft_rights=All Rights (including copyright) CSIRO 2018.&rft_rights=Creative Commons Attribution https://creativecommons.org/licenses/by/4.0/&rft_subject=pulsars, neutron stars, P574_2018APRS&rft_subject=Astronomical and Space Sciences not elsewhere classified&rft_subject=PHYSICAL SCIENCES&rft_subject=ASTRONOMICAL AND SPACE SCIENCES&rft.type=dataset&rft.language=English Access the data

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Creative Commons Attribution
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All Rights (including copyright) CSIRO 2018.

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Data is accessible online and may be reused in accordance with licence conditions

Brief description

We request time to observe 260 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
are (co-)authors on 70 papers arising from the collaboration and P574 data. The data have contributed to the PhD theses of students from Bordeaux, Stanford, Swinburne and Oxford.

Data time period: 2018-07-20 to 2018-07-25

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