Data

Parkes observations for project P860 semester 2019APRS_03

Commonwealth Scientific and Industrial Research Organisation
Balakrishnan, Vishnu ; Possenti, Andrea ; Johnston, Simon ; Kramer, Michael ; Burgay, Marta ; Bailes, Matthew ; Bhat, Ramesh ; van Straten, Willem ; Stappers, Benjamin ; Champion, David ; Jameson, Andrew ; Cameron, Andrew ; Ng, Cherry ; Petroff, Emily ; Barr, Ewan ; Flynn, Chris ; Bhandari, Shivani ; Wongphechauxsorn, Jompoj
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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:doi10.25919/5d480f039ce51&rft.title=Parkes observations for project P860 semester 2019APRS_03&rft.identifier=https://doi.org/10.25919/5d480f039ce51&rft.publisher=Commonwealth Scientific and Industrial Research Organisation&rft.description=This is a request for observing time for the initial follow-up of pulsar discoveries from the low-latitude Galactic plane section of the HTRU survey (P630). We have now completed a first pass processing of the entire survey with our periodicity search algorithm as well as the partially-coherent segmented acceleration search pipeline, and have discovered 106 previously unknown pulsars. \rInteresting science can usually only be derived from a new pulsar after confirmation and a follow-up timing campaign is carried out. One year of initial timing is the minimum timespan required to fully characterise any newly-discovered pulsars, essential for deriving pulsar parameters such as the characteristic age, magnetic ?eld strength, spin-down rate, as well as to detect any unexpected behaviour of the pulsar which might result from emission instabilities. \rThis follow-up timing project is necessary for following up on any interesting pulsar systems discovered from the HTRU Galactic plane survey. Since all of the pulsars on the observing list here are being followed-up for the first time, they will produce completely new and exciting results. In addition, this timing project will enable a large-scale examination of the Galactic plane pulsar population, exploring the true boundaries of pulsar parameter space.&rft.creator=Balakrishnan, Vishnu &rft.creator=Possenti, Andrea &rft.creator=Johnston, Simon &rft.creator=Kramer, Michael &rft.creator=Burgay, Marta &rft.creator=Bailes, Matthew &rft.creator=Bhat, Ramesh &rft.creator=van Straten, Willem &rft.creator=Stappers, Benjamin &rft.creator=Champion, David &rft.creator=Jameson, Andrew &rft.creator=Cameron, Andrew &rft.creator=Ng, Cherry &rft.creator=Petroff, Emily &rft.creator=Barr, Ewan &rft.creator=Flynn, Chris &rft.creator=Bhandari, Shivani &rft.creator=Wongphechauxsorn, Jompoj &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=compact binaries and/or black-holes&rft_subject=transients&rft_subject=P860_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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This is a request for observing time for the initial follow-up of pulsar discoveries from the low-latitude Galactic plane section of the HTRU survey (P630). We have now completed a first pass processing of the entire survey with our periodicity search algorithm as well as the partially-coherent segmented acceleration search pipeline, and have discovered 106 previously unknown pulsars. \r
Interesting science can usually only be derived from a new pulsar after confirmation and a follow-up timing campaign is carried out. One year of initial timing is the minimum timespan required to fully characterise any newly-discovered pulsars, essential for deriving pulsar parameters such as the characteristic age, magnetic ?eld strength, spin-down rate, as well as to detect any unexpected behaviour of the pulsar which might result from emission instabilities. \r
This follow-up timing project is necessary for following up on any interesting pulsar systems discovered from the HTRU Galactic plane survey. Since all of the pulsars on the observing list here are being followed-up for the first time, they will produce completely new and exciting results. In addition, this timing project will enable a large-scale examination of the Galactic plane pulsar population, exploring the true boundaries of pulsar parameter space.

Available: 2019-08-06

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

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ACN 633 798 857