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Ultra-wide Bandwidth Observations of 19 Pulsars with Parkes Telescope
Zhou, Zu-Rong1,2; Wang, Jing-Bo1,3,4; Wang, Na1,3,4; Hobbs, George5; Wang, Shuang-Qiang1,2,6
2022-08-01
Source PublicationResearch in Astronomy and Astrophysics
ISSN1674-4527
Volume22Issue:8Pages:85001
Contribution Rank1
AbstractFlux densities are basic observation parameters to describe pulsars. In the most updated pulsar catalog, 24% of the listed radio pulsars have no flux density measurement at any frequency. Here, we report the first flux density measurements, spectral indices, pulse profiles, and correlations of the spectral index with pulsar parameters for 19 pulsars employing the Ultra-Wideband Low receiver system installed on the Parkes radio telescope. The results for spectral indices of 17 pulsars are in the range between -0.6 and -3.10. The polarization profiles of thirteen pulsars are shown. There is a moderate correlation between the spectral index and spin frequency. For most pulsars detected, the signal-to-noise ratio of pulse profile is not high, so DM, Faraday rotation measure, and polarization cannot be determined precisely. Twenty-nine pulsars were not detected in our observations. We discuss the possible explanations for why these pulsars were not detected.
Keyword(stars:) pulsars: general stars: neutron methods: data analysis flux-density measurements polarization discovery spectra polarimetry profiles emission Astronomy & Astrophysics
SubtypeArticle
DOI10.1088/1674-4527/ac712b
URL查看原文
Indexed BySCI
Language英语
WOS IDWOS:000825854600001
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Cited Times:1[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/5152
Collection射电天文研究室_脉冲星研究团组
Affiliation1.Xinjiang Astronomical Observatory, Chinese Academy of Sciences, Urumqi, Xinjiang 830011, China; wangjingbo@xao.ac.cn, na.wang@xao.ac.cn;
2.University of Chinese Academy of Sciences, 19A Yuquan Road, Beijing 100049, China;
3.Xinjiang Key Laboratory of Radio Astrophysics, 150 Science1-Street, Urumqi, Xinjiang 830011, China;
4.Key Lab of Radio Astronomy, Chinese Academy of Sciences, Beijing 100101, China;
5.CSIRO Astronomy and Space Science, PO Box 76, Epping, NSW 1710, Australia;
6.CAS Key Laboratory of FAST, NAOC, Chinese Academy of Sciences, Beijing 100101, China
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Zhou, Zu-Rong,Wang, Jing-Bo,Wang, Na,et al. Ultra-wide Bandwidth Observations of 19 Pulsars with Parkes Telescope[J]. Research in Astronomy and Astrophysics,2022,22(8):85001.
APA Zhou, Zu-Rong,Wang, Jing-Bo,Wang, Na,Hobbs, George,&Wang, Shuang-Qiang.(2022).Ultra-wide Bandwidth Observations of 19 Pulsars with Parkes Telescope.Research in Astronomy and Astrophysics,22(8),85001.
MLA Zhou, Zu-Rong,et al."Ultra-wide Bandwidth Observations of 19 Pulsars with Parkes Telescope".Research in Astronomy and Astrophysics 22.8(2022):85001.
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