The Parkes Pulsar Timing Array Third Data Release
We present the third data release from the Parkes Pulsar Timing Array (PPTA) project. The release contains observations of 32 pulsars obtained using the 64-m Parkes "Murriyang" radio telescope. The data span is up to 18 years with a typical cadence of 3 weeks. This data release is formed b...
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| creator | Zic, Andrew Reardon, Daniel J Kapur, Agastya Hobbs, George Mandow, Rami Curyło, Małgorzata Shannon, Ryan M Askew, Jacob Bailes, Matthew Bhat, N. D. Ramesh Cameron, Andrew Chen, Zu-Cheng Dai, Shi Di Marco, Valentina Feng, Yi Kerr, Matthew Kulkarni, Atharva Lower, Marcus E Luo, Rui Manchester, Richard N Miles, Matthew T Nathan, Rowina S Osłowski, Stefan Rogers, Axl F Russell, Christopher J Sarkissian, John M Shamohammadi, Mohsen Spiewak, Renée Thyagarajan, Nithyanandan Toomey, Lawrence Wang, Shuangqiang Zhang, Lei Zhang, Songbo Zhu, Xing-Jiang |
| description | We present the third data release from the Parkes Pulsar Timing Array (PPTA)
project. The release contains observations of 32 pulsars obtained using the
64-m Parkes "Murriyang" radio telescope. The data span is up to 18 years with a
typical cadence of 3 weeks. This data release is formed by combining an updated
version of our second data release with $\sim 3$ years of more recent data
primarily obtained using an ultra-wide-bandwidth receiver system that operates
between 704 and 4032 MHz. We provide calibrated pulse profiles, flux-density
dynamic spectra, pulse times of arrival, and initial pulsar timing models. We
describe methods for processing such wide-bandwidth observations, and compare
this data release with our previous release. |
| doi_str_mv | 10.48550/arxiv.2306.16230 |
| format | Article |
| fullrecord | <record><control><sourceid>arxiv_GOX</sourceid><recordid>TN_cdi_arxiv_primary_2306_16230</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2306_16230</sourcerecordid><originalsourceid>FETCH-LOGICAL-a670-d6f6978de9e4d58ad805528af7fe4578bffa3437b561b609959925dd176415433</originalsourceid><addsrcrecordid>eNotzs1qAjEUQOFsXBTtA3RlXmDGZJKbn6VYWwtCpWQ_3CE3GhylZFT07dtqV2d3-Bh7kaLWDkDMsFzzpW6UMLU0v3liMuyIb7DsaeCbcz9g4SEf8nHL56XgjYddLpG_4gn5F_WEA03YKGE_0PN_xyy8LcNiVa0_3z8W83WFxooqmmS8dZE86QgOoxMAjcNkE2mwrksJlVa2AyM7I7wH7xuIUVqjJWilxmz62N7N7XfJByy39s_e3u3qB8ffPJQ</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>The Parkes Pulsar Timing Array Third Data Release</title><source>arXiv.org</source><creator>Zic, Andrew ; Reardon, Daniel J ; Kapur, Agastya ; Hobbs, George ; Mandow, Rami ; Curyło, Małgorzata ; Shannon, Ryan M ; Askew, Jacob ; Bailes, Matthew ; Bhat, N. D. Ramesh ; Cameron, Andrew ; Chen, Zu-Cheng ; Dai, Shi ; Di Marco, Valentina ; Feng, Yi ; Kerr, Matthew ; Kulkarni, Atharva ; Lower, Marcus E ; Luo, Rui ; Manchester, Richard N ; Miles, Matthew T ; Nathan, Rowina S ; Osłowski, Stefan ; Rogers, Axl F ; Russell, Christopher J ; Sarkissian, John M ; Shamohammadi, Mohsen ; Spiewak, Renée ; Thyagarajan, Nithyanandan ; Toomey, Lawrence ; Wang, Shuangqiang ; Zhang, Lei ; Zhang, Songbo ; Zhu, Xing-Jiang</creator><creatorcontrib>Zic, Andrew ; Reardon, Daniel J ; Kapur, Agastya ; Hobbs, George ; Mandow, Rami ; Curyło, Małgorzata ; Shannon, Ryan M ; Askew, Jacob ; Bailes, Matthew ; Bhat, N. D. Ramesh ; Cameron, Andrew ; Chen, Zu-Cheng ; Dai, Shi ; Di Marco, Valentina ; Feng, Yi ; Kerr, Matthew ; Kulkarni, Atharva ; Lower, Marcus E ; Luo, Rui ; Manchester, Richard N ; Miles, Matthew T ; Nathan, Rowina S ; Osłowski, Stefan ; Rogers, Axl F ; Russell, Christopher J ; Sarkissian, John M ; Shamohammadi, Mohsen ; Spiewak, Renée ; Thyagarajan, Nithyanandan ; Toomey, Lawrence ; Wang, Shuangqiang ; Zhang, Lei ; Zhang, Songbo ; Zhu, Xing-Jiang</creatorcontrib><description>We present the third data release from the Parkes Pulsar Timing Array (PPTA)
project. The release contains observations of 32 pulsars obtained using the
64-m Parkes "Murriyang" radio telescope. The data span is up to 18 years with a
typical cadence of 3 weeks. This data release is formed by combining an updated
version of our second data release with $\sim 3$ years of more recent data
primarily obtained using an ultra-wide-bandwidth receiver system that operates
between 704 and 4032 MHz. We provide calibrated pulse profiles, flux-density
dynamic spectra, pulse times of arrival, and initial pulsar timing models. We
describe methods for processing such wide-bandwidth observations, and compare
this data release with our previous release.</description><identifier>DOI: 10.48550/arxiv.2306.16230</identifier><language>eng</language><subject>Physics - Cosmology and Nongalactic Astrophysics ; Physics - General Relativity and Quantum Cosmology ; Physics - High Energy Astrophysical Phenomena ; Physics - Solar and Stellar Astrophysics</subject><creationdate>2023-06</creationdate><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,782,887</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/2306.16230$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.2306.16230$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Zic, Andrew</creatorcontrib><creatorcontrib>Reardon, Daniel J</creatorcontrib><creatorcontrib>Kapur, Agastya</creatorcontrib><creatorcontrib>Hobbs, George</creatorcontrib><creatorcontrib>Mandow, Rami</creatorcontrib><creatorcontrib>Curyło, Małgorzata</creatorcontrib><creatorcontrib>Shannon, Ryan M</creatorcontrib><creatorcontrib>Askew, Jacob</creatorcontrib><creatorcontrib>Bailes, Matthew</creatorcontrib><creatorcontrib>Bhat, N. D. Ramesh</creatorcontrib><creatorcontrib>Cameron, Andrew</creatorcontrib><creatorcontrib>Chen, Zu-Cheng</creatorcontrib><creatorcontrib>Dai, Shi</creatorcontrib><creatorcontrib>Di Marco, Valentina</creatorcontrib><creatorcontrib>Feng, Yi</creatorcontrib><creatorcontrib>Kerr, Matthew</creatorcontrib><creatorcontrib>Kulkarni, Atharva</creatorcontrib><creatorcontrib>Lower, Marcus E</creatorcontrib><creatorcontrib>Luo, Rui</creatorcontrib><creatorcontrib>Manchester, Richard N</creatorcontrib><creatorcontrib>Miles, Matthew T</creatorcontrib><creatorcontrib>Nathan, Rowina S</creatorcontrib><creatorcontrib>Osłowski, Stefan</creatorcontrib><creatorcontrib>Rogers, Axl F</creatorcontrib><creatorcontrib>Russell, Christopher J</creatorcontrib><creatorcontrib>Sarkissian, John M</creatorcontrib><creatorcontrib>Shamohammadi, Mohsen</creatorcontrib><creatorcontrib>Spiewak, Renée</creatorcontrib><creatorcontrib>Thyagarajan, Nithyanandan</creatorcontrib><creatorcontrib>Toomey, Lawrence</creatorcontrib><creatorcontrib>Wang, Shuangqiang</creatorcontrib><creatorcontrib>Zhang, Lei</creatorcontrib><creatorcontrib>Zhang, Songbo</creatorcontrib><creatorcontrib>Zhu, Xing-Jiang</creatorcontrib><title>The Parkes Pulsar Timing Array Third Data Release</title><description>We present the third data release from the Parkes Pulsar Timing Array (PPTA)
project. The release contains observations of 32 pulsars obtained using the
64-m Parkes "Murriyang" radio telescope. The data span is up to 18 years with a
typical cadence of 3 weeks. This data release is formed by combining an updated
version of our second data release with $\sim 3$ years of more recent data
primarily obtained using an ultra-wide-bandwidth receiver system that operates
between 704 and 4032 MHz. We provide calibrated pulse profiles, flux-density
dynamic spectra, pulse times of arrival, and initial pulsar timing models. We
describe methods for processing such wide-bandwidth observations, and compare
this data release with our previous release.</description><subject>Physics - Cosmology and Nongalactic Astrophysics</subject><subject>Physics - General Relativity and Quantum Cosmology</subject><subject>Physics - High Energy Astrophysical Phenomena</subject><subject>Physics - Solar and Stellar Astrophysics</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2023</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNotzs1qAjEUQOFsXBTtA3RlXmDGZJKbn6VYWwtCpWQ_3CE3GhylZFT07dtqV2d3-Bh7kaLWDkDMsFzzpW6UMLU0v3liMuyIb7DsaeCbcz9g4SEf8nHL56XgjYddLpG_4gn5F_WEA03YKGE_0PN_xyy8LcNiVa0_3z8W83WFxooqmmS8dZE86QgOoxMAjcNkE2mwrksJlVa2AyM7I7wH7xuIUVqjJWilxmz62N7N7XfJByy39s_e3u3qB8ffPJQ</recordid><startdate>20230628</startdate><enddate>20230628</enddate><creator>Zic, Andrew</creator><creator>Reardon, Daniel J</creator><creator>Kapur, Agastya</creator><creator>Hobbs, George</creator><creator>Mandow, Rami</creator><creator>Curyło, Małgorzata</creator><creator>Shannon, Ryan M</creator><creator>Askew, Jacob</creator><creator>Bailes, Matthew</creator><creator>Bhat, N. 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D. 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D. Ramesh</au><au>Cameron, Andrew</au><au>Chen, Zu-Cheng</au><au>Dai, Shi</au><au>Di Marco, Valentina</au><au>Feng, Yi</au><au>Kerr, Matthew</au><au>Kulkarni, Atharva</au><au>Lower, Marcus E</au><au>Luo, Rui</au><au>Manchester, Richard N</au><au>Miles, Matthew T</au><au>Nathan, Rowina S</au><au>Osłowski, Stefan</au><au>Rogers, Axl F</au><au>Russell, Christopher J</au><au>Sarkissian, John M</au><au>Shamohammadi, Mohsen</au><au>Spiewak, Renée</au><au>Thyagarajan, Nithyanandan</au><au>Toomey, Lawrence</au><au>Wang, Shuangqiang</au><au>Zhang, Lei</au><au>Zhang, Songbo</au><au>Zhu, Xing-Jiang</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The Parkes Pulsar Timing Array Third Data Release</atitle><date>2023-06-28</date><risdate>2023</risdate><abstract>We present the third data release from the Parkes Pulsar Timing Array (PPTA)
project. The release contains observations of 32 pulsars obtained using the
64-m Parkes "Murriyang" radio telescope. The data span is up to 18 years with a
typical cadence of 3 weeks. This data release is formed by combining an updated
version of our second data release with $\sim 3$ years of more recent data
primarily obtained using an ultra-wide-bandwidth receiver system that operates
between 704 and 4032 MHz. We provide calibrated pulse profiles, flux-density
dynamic spectra, pulse times of arrival, and initial pulsar timing models. We
describe methods for processing such wide-bandwidth observations, and compare
this data release with our previous release.</abstract><doi>10.48550/arxiv.2306.16230</doi><oa>free_for_read</oa></addata></record> |
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| identifier | DOI: 10.48550/arxiv.2306.16230 |
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| language | eng |
| recordid | cdi_arxiv_primary_2306_16230 |
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| subjects | Physics - Cosmology and Nongalactic Astrophysics Physics - General Relativity and Quantum Cosmology Physics - High Energy Astrophysical Phenomena Physics - Solar and Stellar Astrophysics |
| title | The Parkes Pulsar Timing Array Third Data Release |
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