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Observations of Nine Millisecond Pulsars at 8600 MHz Using the TMRT
Wang, Xiao-Wei1,2; Yan, Zhen1,2,3; Shen, Zhi-Qiang1,2,3,4; Tong, Hao5; Zhou, Xia3,6,7; Zhao, Rong-Bing1,2,3; Wu, Ya-Jun1,2,3; Huang, Zhi-Peng1,2,4; Wang, Rui1,2; Liu, Jie1
2024
Source PublicationASTROPHYSICAL JOURNAL
ISSN0004-637X
Volume961Issue:1Pages:48
Contribution Rank6
AbstractWe report detection results of nine millisecond pulsars (MSPs) at 8600 MHz using simultaneous 2250 and 8600 MHz observations conducted with the Shanghai Tian Ma Radio Telescope. Mainly benefiting from updated ephemerids with 2250 MHz observations, integrated profiles of all nine MSPs at 8600 MHz are successfully obtained by coherently adding multi-epoch (3-83 epochs) observation data spanning from 19-1210 days, which significantly increases the number of MSPs with published profiles (from 4 to 11) above 8000 MHz, as seven of our target MPSs had no related results previously. Combining our new flux density and pulse width measurements with previous low-frequency results, we study their integrated profile evolution and spectral behaviors in a wider frequency range. We find their component separations and pulse widths remain almost constant, which is consistent with previous findings. While dramatic evolution of integrated profiles exists at low frequencies, we observe a potential end of the related evolution around 5 GHz in eight MSPs. The spectra of four MSPs are found to deviate from a single power law, and we fit them with a broken power law. The change in the profile of PSR J1713+0747, which started around MJD 59320-59321, seems to be more prominent as the observation frequency increases. Compared with the effects of the interstellar medium, we prefer to explain this event as some changes in the magnetosphere. We also find its integrated profile possibly had not recovered to the pre-event state until MJD 59842-59857.
DOI10.3847/1538-4357/ad0724
Indexed BySCI
Language英语
WOS KeywordFLUX-DENSITY MEASUREMENTS ; SINGLE-PULSE ; BACK-END ; BINARY ; EMISSION ; SPECTRA ; DISCOVERY ; PROFILES ; CENSUS ; POLARIMETRY
Funding ProjectSTCSM divided by Natural Science Foundation of Shanghai Municipalityhttps://doi.org/10.13039/100007219[2022YFA1603104] ; National Key R&D Program of China[U2031119] ; National Key R&D Program of China[12041301] ; National Natural Science Foundation of China[20ZR1467600] ; Natural Science Foundation of Shanghai
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:001141968400001
PublisherIOP Publishing Ltd
Funding OrganizationSTCSM divided by Natural Science Foundation of Shanghai Municipalityhttps://doi.org/10.13039/100007219 ; National Key R&D Program of China ; National Natural Science Foundation of China ; Natural Science Foundation of Shanghai
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Cited Times:3[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/5750
Collection射电天文研究室_脉冲星研究团组
Corresponding AuthorYan, Zhen
Affiliation1.Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China
2.Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing 100049, Peoples R China
3.Chinese Acad Sci, Key Lab Radio Astron & Technol, A20 Datun Rd, Beijing 100101, Peoples R China
4.Shanghai Tech Univ, Sch Phys Sci & Technol, Shanghai 201210, Peoples R China
5.Guangzhou Univ, Sch Phys & Mat Sci, Dept Astron, Guangzhou 510006, Peoples R China
6.Chinese Acad Sci, Xinjiang Astron Observ, Xinjiang 830011, Peoples R China
7.Xinjiang Key Lab Radio Astrophys, 150 Sci 1 St, Urumqi 830011, Peoples R China
Recommended Citation
GB/T 7714
Wang, Xiao-Wei,Yan, Zhen,Shen, Zhi-Qiang,et al. Observations of Nine Millisecond Pulsars at 8600 MHz Using the TMRT[J]. ASTROPHYSICAL JOURNAL,2024,961(1):48.
APA Wang, Xiao-Wei.,Yan, Zhen.,Shen, Zhi-Qiang.,Tong, Hao.,Zhou, Xia.,...&Liu, Jie.(2024).Observations of Nine Millisecond Pulsars at 8600 MHz Using the TMRT.ASTROPHYSICAL JOURNAL,961(1),48.
MLA Wang, Xiao-Wei,et al."Observations of Nine Millisecond Pulsars at 8600 MHz Using the TMRT".ASTROPHYSICAL JOURNAL 961.1(2024):48.
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