Correction to: Follow-up timing of 24 pulsars discovered in commensal radio astronomy FAST survey

In the published paper (Q.D. Wu et al. 2023 ), linear polarization position angles (PAs) and the signs of Faraday rotation measurements were incorrect due to errors in data processing during the polarization calibration process (specifically, the sign flip of Stokes Q was omitted in the data processing).The corrected values of the rotation measure are presented here in Table 2 .The integrated polarization profiles and viewing geometry were also corrected, as shown here in Fig. 3 , 7 , and 8 .Since these values are only presented in subsection 3.2, and are not related to other sections, these corrections do not affect the results or conclusions of the published paper.The PSR J1617 + 1123 has a Faraday rotation measure of 24(1) rad m -2 .We measured the magnetic inclination angle, reference position angle, longitude of the fiducial plane, and viewing angle are = 75(3) , 0 = -12 .8(1) , 0 = 178 .07(1) , and = 72(3) , respectively.We obtained the RM of 30.7(8) rad m -2 for PSR J1631 + 1252.Through the RVM method, we find 0 = 43 .8(6) , 0 = 179 .56(6) , = 49(8) , and = 52(9) .PSR J1900 + 4221 has a Faraday rotation measure of 19(4) rad m -2 .We find The RM of PSR J2032 + 0701 is -96(22) rad m -2 .Through the RVM method, we find 0 = 86(6) , 0 = 183 .3(7) , = 94(4) , and = 88(4) .

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Publication Details

Journal
Monthly Notices of the Royal Astronomical Society
Published
2025-11-19
DOI
https://doi.org/10.1093/mnras/staf1986
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
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article

Correction to: Follow-up timing of 24 pulsars discovered in commensal radio astronomy FAST survey

Zhidong Tu, Chenhui Niu, Shijun You, Xueli Miao et al.
Monthly Notices of the Royal Astronomical Society
Pulsars and Gravitational Waves Research
article

Correction to: Follow-up timing of 24 pulsars discovered in commensal radio astronomy FAST survey

Zhidong Tu, Chenhui Niu, Shijun You, Xueli Miao, Youling Yue, Ru-Shuang Zhao, Z J Liu, Zhichen Pan, Jiarui Niu, Weiwei Zhu, Xiaoyao Xie, J T Xie, Mao Yuan, Yi Feng, Z. G. Wen, Mengyao Xue, Lingqi Meng, Lei Qian, Xuhong Yu, J B Wang, Habtamu Menberu Tedila, W. M. Yan, S. N. Sun, S. J. Dang, Degang Zhao, Q. D. Wu, R. Yuen, Lei Zhang, Di Li, Na Wang, Pei Wang, Jumei Yao, J. P. Yuan, Y F Xiao, Shuangqiang Wang, F. F. Kou, Chenchen Miao, Y T Chen
article en

Abstract

In the published paper (Q.D. Wu et al. 2023 ), linear polarization position angles (PAs) and the signs of Faraday rotation measurements were incorrect due to errors in data processing during the polarization calibration process (specifically, the sign flip of Stokes Q was omitted in the data processing).The corrected values of the rotation measure are presented here in Table 2 .The integrated polarization profiles and viewing geometry were also corrected, as shown here in Fig. 3 , 7 , and 8 .Since these values are only presented in subsection 3.2, and are not related to other sections, these corrections do not affect the results or conclusions of the published paper.The PSR J1617 + 1123 has a Faraday rotation measure of 24(1) rad m -2 .We measured the magnetic inclination angle, reference position angle, longitude of the fiducial plane, and viewing angle are = 75(3) , 0 = -12 .8(1) , 0 = 178 .07(1) , and = 72(3) , respectively.We obtained the RM of 30.7(8) rad m -2 for PSR J1631 + 1252.Through the RVM method, we find 0 = 43 .8(6) , 0 = 179 .56(6) , = 49(8) , and = 52(9) .PSR J1900 + 4221 has a Faraday rotation measure of 19(4) rad m -2 .We find The RM of PSR J2032 + 0701 is -96(22) rad m -2 .Through the RVM method, we find 0 = 86(6) , 0 = 183 .3(7) , = 94(4) , and = 88(4) .

Monthly Notices of the Royal Astronomical SocietyVol. 545(1)
Jiujiang University (CN), Guizhou Normal University (CN), Guizhou University (CN), Chinese Academy of Sciences (CN), Fudan University (CN), Beijing Normal University (CN), Xinjiang Astronomical Observatory (CN), Lishui University (CN), National Space Science Center (CN), Zhejiang Lab (CN), Astronomy and Space (AU), National Astronomical Observatories (CN), University of Chinese Academy of Sciences (CN), University of KwaZulu-Natal (ZA)
Openalex Percentile: Top 72%
Pulsars and Gravitational Waves Research
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