TY - JOUR
T1 - Deep searches for radio pulsations and bursts from four magnetar and a magnetar-like pulsar with FAST
AU - Bai, Juntao
AU - Wang, Na
AU - Dai, Shi
AU - Wang, Shuangqiang
AU - Yuan, Jianping
AU - Yan, Wenming
AU - Shang, Lunhua
AU - Xu, Xin
AU - Dang, Shijun
AU - Zhang, Zhen
PY - 2025
Y1 - 2025
N2 - We report on radio observations of four magnetars SGR 0501+4516, Swift 1834.9-0846, 1E 1841-045, SGR 1900+14, and a magnetar-like pulsar PSR J1846-0258 with the Five-hundred-meter Aperture Spherical radio Telescope at 1250 MHz. Notably, PSR J1846-0258 was observed 1 month after its 2020 X-ray outburst. The data from these observations were searched for periodic emissions and single pulses. No radio emission was detected for any of our targets. After accounting for the effect of red noise, the nondetections yield stringent upper limits on the radio flux density, with S1250 ≤ 16.9 μJy for the four magnetars and the magnetar-like pulsar, along with constraints on single-pulse flux densities. Our deep radio observations suggest that these magnetars and the magnetar-like pulsar are indeed radio-quiet sources or unfavorably beamed. The resulting flux upper limits, along with previous findings, are discussed, highlighting the significance of further radio observations of radio-quiet magnetars and the high-B magnetar-like pulsar.
AB - We report on radio observations of four magnetars SGR 0501+4516, Swift 1834.9-0846, 1E 1841-045, SGR 1900+14, and a magnetar-like pulsar PSR J1846-0258 with the Five-hundred-meter Aperture Spherical radio Telescope at 1250 MHz. Notably, PSR J1846-0258 was observed 1 month after its 2020 X-ray outburst. The data from these observations were searched for periodic emissions and single pulses. No radio emission was detected for any of our targets. After accounting for the effect of red noise, the nondetections yield stringent upper limits on the radio flux density, with S1250 ≤ 16.9 μJy for the four magnetars and the magnetar-like pulsar, along with constraints on single-pulse flux densities. Our deep radio observations suggest that these magnetars and the magnetar-like pulsar are indeed radio-quiet sources or unfavorably beamed. The resulting flux upper limits, along with previous findings, are discussed, highlighting the significance of further radio observations of radio-quiet magnetars and the high-B magnetar-like pulsar.
UR - http://www.scopus.com/inward/record.url?scp=85217099633&partnerID=8YFLogxK
U2 - 10.3847/1538-4357/ada3c4
DO - 10.3847/1538-4357/ada3c4
M3 - Article
AN - SCOPUS:85217099633
SN - 0004-637X
VL - 979
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 2
M1 - 122
ER -