Detection of Radio Emissions from Magnetar RX J1605.3+3249 at Frequency of 111 MHz

Abstract

For the first time, pulsed radio emission from the RX J1605.3+3249 magnetar, which is part of the Magnificent Seven, has been detected. Data obtained at the BSA LPI radio telescope at a frequency of 111 MHz in the period from 2012 to 2024 were processed. The peak flux density of \(S = 50{\kern 1pt} - {\kern 1pt} 100\) mJy and the dispersion measure of \(DM = 4.7 \pm 0.5\) pc/cm³ have been measured.