Data

Parkes observations for project P1016 semester 2019APRS_06

Commonwealth Scientific and Industrial Research Organisation
Kaczmarek, Jane ; Johnston, Simon ; Hobbs, George ; Oslowski, Stefan ; Dai, Shi
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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:doi10.25919/5d63c20d8ed2a&rft.title=Parkes observations for project P1016 semester 2019APRS_06&rft.identifier=https://doi.org/10.25919/5d63c20d8ed2a&rft.publisher=Commonwealth Scientific and Industrial Research Organisation&rft.description=Understanding rotating radio transients (RRATs) has the potential to uproot our understanding of core-collapse supernovae and the overall evolution of neutron stars. Despite this, RRATs remain an enigma and has numerous potential and conflicting explanations in the literature. These observations will observe a sample of RRATs with the UWL receiver, in tandem with the Five-hundred-meter Aperture Spherical Telescope (FAST), in order to directly test many of the competing theories that exist around RRATs and answer the question of where they fit amongst the overall population of neutron stars.&rft.creator=Kaczmarek, Jane &rft.creator=Johnston, Simon &rft.creator=Hobbs, George &rft.creator=Oslowski, Stefan &rft.creator=Dai, Shi &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=transients&rft_subject=P1016_2019APRS&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

Understanding rotating radio transients (RRATs) has the potential to uproot our understanding of core-collapse supernovae and the overall evolution of neutron stars. Despite this, RRATs remain an enigma and has numerous potential and conflicting explanations in the literature. These observations will observe a sample of RRATs with the UWL receiver, in tandem with the Five-hundred-meter Aperture Spherical Telescope (FAST), in order to directly test many of the competing theories that exist around RRATs and answer the question of where they fit amongst the overall population of neutron stars.

Available: 2019-08-27

Data time period: 2019-04-01 to 2019-09-30

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Astronomical Sciences | Astronomical Sciences Not Elsewhere Classified | P1016_2019APRS | Physical Sciences | neutron stars | pulsars | transients |

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