Data

Parkes observations for project P1165 semester 2023APRS_01

Commonwealth Scientific and Industrial Research Organisation
Xu, xin ; Dai, Shi ; Bai, Juntao ; Zhi, QiJun
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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/pq6y-zm04&rft.title=Parkes observations for project P1165 semester 2023APRS_01&rft.identifier=https://doi.org/10.25919/pq6y-zm04&rft.publisher=Commonwealth Scientific and Industrial Research Organisation&rft.description=We carried out a pilot FAST survey at intermediate Galactic latitudes and discovered five new pulsars (including two millisecond pulsars, MSPs). We confirmed all five pulsars and timed two pulsars (J1826-0049 and J1849+1000) during the 2022OCTS semester. A coherent timing solution was obtained for J1826-0049 (4.59 ms) and it is in a 6.7-day orbit with a white dwarf companion. The other pulsar, J1849+1000, turned out to be potentially exotic. While its large spin period variation can be fitted by a 26-day circular orbit with a massive companion, the residuals show strong quasi-periodic variations, which suggest the existence of a third object in an inner orbit. If confirmed, J1849+1000 will be in a stellar triple system with an outer orbit of 26 days and an inner orbit of a few days. This makes it potentially a unique system for tests of gravitational theories and understanding the formation and evolution of triple systems. Here we propose to continue our timing of J1826-0049 and J1849+1000. The goal is to refine our measurement of the parameters of J1826-0049 and understand the nature of J1849+1000&rft.creator=Xu, xin &rft.creator=Dai, Shi &rft.creator=Bai, Juntao &rft.creator=Zhi, QiJun &rft.date=2023&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 2023.&rft_subject=pulsars&rft_subject=neutron stars&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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We carried out a pilot FAST survey at intermediate Galactic latitudes and discovered five new pulsars (including two millisecond pulsars, MSPs). We confirmed all five pulsars and timed two pulsars (J1826-0049 and J1849+1000) during the 2022OCTS semester. A coherent timing solution was obtained for J1826-0049 (4.59 ms) and it is in a 6.7-day orbit with a white dwarf companion. The other pulsar, J1849+1000, turned out to be potentially exotic. While its large spin period variation can be fitted by a 26-day circular orbit with a massive companion, the residuals show strong quasi-periodic variations, which suggest the existence of a third object in an inner orbit. If confirmed, J1849+1000 will be in a stellar triple system with an outer orbit of 26 days and an inner orbit of a few days. This makes it potentially a unique system for tests of gravitational theories and understanding the formation and evolution of triple systems. Here we propose to continue our timing of J1826-0049 and J1849+1000. The goal is to refine our measurement of the parameters of J1826-0049 and understand the nature of J1849+1000

Available: 2023-05-16

Data time period: 2023-04-01 to 2023-09-30

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ACN 633 798 857