Data

Parkes observations for project P1082 semester 2020OCTS_03

Commonwealth Scientific and Industrial Research Organisation
Keane, Evan ; Johnston, Simon ; Dai, Shi ; Morello, Vincent
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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/dpk9-wc19&rft.title=Parkes observations for project P1082 semester 2020OCTS_03&rft.identifier=10.25919/dpk9-wc19&rft.publisher=Commonwealth Scientific and Industrial Research Organisation (CSIRO)&rft.description=Globular clusters can harbour many compact objects including intermediate mass black holes and a zoo of neutron star systems. Mercer 5 is a newly identified globular cluster whose gamma-ray emission properties suggest it may host 200 or more millisecond pulsars. If this is the case it could be the most abundant system known by some distance, opening up several avenues of study on fundamental astrophysical questions. Using the UWL receiver we propose to perform deep searches of the cluster with Parkes to identify the pulsar population.&rft.creator=Keane, Evan &rft.creator=Johnston, Simon &rft.creator=Dai, Shi &rft.creator=Morello, Vincent &rft.date=2021&rft.edition=v1&rft_rights=All Rights (including copyright) CSIRO 2020.&rft_rights=Creative Commons Attribution https://creativecommons.org/licenses/by/4.0/&rft_subject=pulsars, neutron stars, compact binaries and/or black-holes, transients, P1082_2020OCTS&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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All Rights (including copyright) CSIRO 2020.

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Brief description

Globular clusters can harbour many compact objects including intermediate mass black holes and a zoo of neutron star systems. Mercer 5 is a newly identified globular cluster whose gamma-ray emission properties suggest it may host 200 or more millisecond pulsars. If this is the case it could be the most abundant system known by some distance, opening up several avenues of study on fundamental astrophysical questions. Using the UWL receiver we propose to perform deep searches of the cluster with Parkes to identify the pulsar population.

Data time period: 2020-10-01 to 2021-03-31

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