Data

Parkes observations for project P871 semester 2017APRS

Commonwealth Scientific and Industrial Research Organisation
Petroff, Emily ; Possenti, Andrea ; Johnston, Simon ; Kramer, Michael ; Bailes, Matthew ; Burke-Spolaor, Sarah ; van Straten, Willem ; Stappers, Benjamin ; Keane, Evan ; Champion, David ; Jameson, Andrew ; Ng, Cherry ; Barr, Ewan ; Flynn, Chris ; Caleb, Manisha
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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:doi10.4225/08/59e45568e4ee1&rft.title=Parkes observations for project P871 semester 2017APRS&rft.identifier=https://doi.org/10.4225/08/59e45568e4ee1&rft.publisher=Commonwealth Scientific and Industrial Research Organisation&rft.description=Fast Radio Bursts (FRBs) are bright, millisecond-duration radio pulses hypothesized to originate at cosmological distances. To date, one FRB has been seen to repeat but their origins remain a puzzling mystery. Some have proposed FRBs come from Crab-like pulsar giant pulses or periods of high activity of distant magnetars. Both mechanisms would generate observable subsequent FRB-like events. In this proposal we directly test this hypothesis by monitoring the fields of two known FRBs to search for repeating pulses that may explain their progenitors. We target two sources with existing multi-wavelength archival images of the field and small DM-derived distances.&rft.creator=Petroff, Emily &rft.creator=Possenti, Andrea &rft.creator=Johnston, Simon &rft.creator=Kramer, Michael &rft.creator=Bailes, Matthew &rft.creator=Burke-Spolaor, Sarah &rft.creator=van Straten, Willem &rft.creator=Stappers, Benjamin &rft.creator=Keane, Evan &rft.creator=Champion, David &rft.creator=Jameson, Andrew &rft.creator=Ng, Cherry &rft.creator=Barr, Ewan &rft.creator=Flynn, Chris &rft.creator=Caleb, Manisha &rft.date=2017&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 2017.&rft_subject=pulsars&rft_subject=neutron stars&rft_subject=surveys and studies of distant galaxies&rft_subject=transients&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

All Rights (including copyright) CSIRO 2017.

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Fast Radio Bursts (FRBs) are bright, millisecond-duration radio pulses hypothesized to originate at cosmological distances. To date, one FRB has been seen to repeat but their origins remain a puzzling mystery. Some have proposed FRBs come from Crab-like pulsar giant pulses or periods of high activity of distant magnetars. Both mechanisms would generate observable subsequent FRB-like events. In this proposal we directly test this hypothesis by monitoring the fields of two known FRBs to search for repeating pulses that may explain their progenitors. We target two sources with existing multi-wavelength archival images of the field and small DM-derived distances.

Available: 2017-10-16

Data time period: 2017-04-01 to 2017-09-30

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Subjects
Astronomical Sciences | Astronomical Sciences Not Elsewhere Classified | Physical Sciences | neutron stars | pulsars | surveys and studies of distant galaxies | transients |

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Identifiers
ACN 633 798 857