Data

Parkes observations for project P574 semester 2018APRS_05

Commonwealth Scientific and Industrial Research Organisation
Dai, Shi ; Possenti, Andrea ; Manchester, Dick ; Johnston, Simon ; Hobbs, George ; 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:doi10.25919/5ba7fac940961&rft.title=Parkes observations for project P574 semester 2018APRS_05&rft.identifier=https://doi.org/10.25919/5ba7fac940961&rft.publisher=Commonwealth Scientific and Industrial Research Organisation&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\r\nare (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, Dick &rft.creator=Johnston, Simon &rft.creator=Hobbs, George &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=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 2018.&rft_subject=pulsars&rft_subject=neutron stars&rft_subject=P574_2018APRS&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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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 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.

Available: 2018-09-24

Data time period: 2018-08-24 to 2018-08-27

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Astronomical Sciences | Astronomical Sciences Not Elsewhere Classified | P574_2018APRS | Physical Sciences | neutron stars | pulsars |

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