We report on the results of a search for radio pulsars in five supernova remnants (SNRs) with FAST. The observations were made using the 19-beam receiver in the Snapshot mode. The integration time for each pointing is 10 min. We discovered a new pulsar PSR J1845−0306 which has a spin period of 983.6 ms and a dispersion measure of 444.6±2.0 cm−3 pc in observations of SNR G29.6+0.1. To judge the association between the pulsar and the SNR, further verification is needed. We also re-detected some known pulsars in the data from SNRs G29.6+0.1 and G29.7−0.3. No pulsars were detected in observations of other three SNRs.
@article{arxiv.2402.17365,
title = {A Search for Radio Pulsars in Supernova Remnants Using FAST with One Pulsar Discovered},
author = {Zhen Zhang and Wen-Ming Yan and Jian-Ping Yuan and Na Wang and Jun-Tao Bai and Zhi-Gang Wen and Bao-Da Li and Jin-Tao Xie and De Zhao and Yu-Bin Wang and Nan-Nan Zhai},
journal= {arXiv preprint arXiv:2402.17365},
year = {2024}
}