A. Zic, D. Reardon, Agastya Kapur, G. Hobbs, R. Mandow, M. Curyło, R. Shannon, Jacob Askew, M. Bailes, N. D. R. Bhat, A. Cameron, Zu-Cheng Chen, Shi Dai, Valentina Di Marco, Yi Feng, M. Kerr, Atharva Kulkarni, M. Lower, Rui Luo, R. Manchester, M. T. Miles, R. Nathan, S. Osłowski, Axl F. Rogers, C. Russell, J. Sarkissian, Mohsen Shamohammadi, R. Spiewak, N. Thyagarajan, L. Toomey, Shuangqiang Wang, Lei Zhang, Songbo Zhang, Xingjiang Zhu
{"title":"帕克斯脉冲星定时阵列第三次数据发布","authors":"A. Zic, D. Reardon, Agastya Kapur, G. Hobbs, R. Mandow, M. Curyło, R. Shannon, Jacob Askew, M. Bailes, N. D. R. Bhat, A. Cameron, Zu-Cheng Chen, Shi Dai, Valentina Di Marco, Yi Feng, M. Kerr, Atharva Kulkarni, M. Lower, Rui Luo, R. Manchester, M. T. Miles, R. Nathan, S. Osłowski, Axl F. Rogers, C. Russell, J. Sarkissian, Mohsen Shamohammadi, R. Spiewak, N. Thyagarajan, L. Toomey, Shuangqiang Wang, Lei Zhang, Songbo Zhang, Xingjiang Zhu","doi":"10.1017/pasa.2023.36","DOIUrl":null,"url":null,"abstract":"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 yr with a typical cadence of 3 weeks. This data release is formed by combining an updated version of our second data release with \n$\\sim$\n 3 yr 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.","PeriodicalId":4,"journal":{"name":"ACS Applied Energy Materials","volume":null,"pages":null},"PeriodicalIF":5.4000,"publicationDate":"2023-06-28","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"35","resultStr":"{\"title\":\"The Parkes Pulsar Timing Array third data release\",\"authors\":\"A. Zic, D. Reardon, Agastya Kapur, G. Hobbs, R. Mandow, M. Curyło, R. Shannon, Jacob Askew, M. Bailes, N. D. R. Bhat, A. Cameron, Zu-Cheng Chen, Shi Dai, Valentina Di Marco, Yi Feng, M. Kerr, Atharva Kulkarni, M. Lower, Rui Luo, R. Manchester, M. T. Miles, R. Nathan, S. Osłowski, Axl F. Rogers, C. Russell, J. Sarkissian, Mohsen Shamohammadi, R. Spiewak, N. Thyagarajan, L. Toomey, Shuangqiang Wang, Lei Zhang, Songbo Zhang, Xingjiang Zhu\",\"doi\":\"10.1017/pasa.2023.36\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"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 yr with a typical cadence of 3 weeks. This data release is formed by combining an updated version of our second data release with \\n$\\\\sim$\\n 3 yr 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.\",\"PeriodicalId\":4,\"journal\":{\"name\":\"ACS Applied Energy Materials\",\"volume\":null,\"pages\":null},\"PeriodicalIF\":5.4000,\"publicationDate\":\"2023-06-28\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"35\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"ACS Applied Energy Materials\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://doi.org/10.1017/pasa.2023.36\",\"RegionNum\":3,\"RegionCategory\":\"材料科学\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q2\",\"JCRName\":\"CHEMISTRY, PHYSICAL\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"ACS Applied Energy Materials","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1017/pasa.2023.36","RegionNum":3,"RegionCategory":"材料科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"CHEMISTRY, PHYSICAL","Score":null,"Total":0}
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 yr 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 yr 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.
期刊介绍:
ACS Applied Energy Materials is an interdisciplinary journal publishing original research covering all aspects of materials, engineering, chemistry, physics and biology relevant to energy conversion and storage. The journal is devoted to reports of new and original experimental and theoretical research of an applied nature that integrate knowledge in the areas of materials, engineering, physics, bioscience, and chemistry into important energy applications.