Data

Parkes observations for project P863 semester 2016OCTS

Commonwealth Scientific and Industrial Research Organisation
Hobbs, G ; Johnston, Simon ; Hollow, Robert ; Ravi, Vikram ; Kerr, Matthew ; Shannon, Ryan ; Dai, Shi ; Ward, 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:doi10.25919/5bb102286be27&rft.title=Parkes observations for project P863 semester 2016OCTS&rft.identifier=10.25919/5bb102286be27&rft.publisher=Commonwealth Scientific and Industrial Research Organisation (CSIRO)&rft.description=In this proposal we request observations from the Parkes radio telescope to survey time variability in the radio emission from a sample of pulsars. The aim is to elucidate different phenomena occurring in the pulsars' magnetospheres. We have chosen a sample of ten pulsars that exhibit various characteristics of the state-changing phenomenon (some are moding pulsars and some are intermittent pulsars). We plan to use the dual-band, multibeam and the H-OH receivers that will provide us with information at widely separated frequency bands.&rft.creator=Hobbs, G &rft.creator=Johnston, Simon &rft.creator=Hollow, Robert &rft.creator=Ravi, Vikram &rft.creator=Kerr, Matthew &rft.creator=Shannon, Ryan &rft.creator=Dai, Shi &rft.creator=Ward, Charlotte &rft.date=2017&rft.edition=v1&rft_rights=All Rights (including copyright) CSIRO 2017.&rft_rights=Creative Commons Attribution https://creativecommons.org/licenses/by/4.0/&rft_subject=pulsars, neutron stars&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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Brief description

In this proposal we request observations from the Parkes radio telescope to survey time variability in the radio emission from a sample of pulsars. The aim is to elucidate different phenomena occurring in the pulsars' magnetospheres. We have chosen a sample of ten pulsars that exhibit various characteristics of the state-changing phenomenon (some are moding pulsars and some are intermittent pulsars). We plan to use the dual-band, multibeam and the H-OH receivers that will provide us with information at widely separated frequency bands.

Data time period: 2016-10-01 to 2017-03-31

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Subjects
Astronomical and Space Sciences | Astronomical and Space Sciences Not Elsewhere Classified | Physical Sciences | pulsars, neutron stars |

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