First radio detection of PSR J2238+5903 yields DM = 247.5 ± 3.0 pc cm^{-3} and a model distance of 7.4 ± 3.9 kpc that anchors the physical scale and TeV efficiency of candidate halo 1LHAASO J2238+5900.
Searching for radio pulses from radio-quiet gamma-ray pulsars with FAST
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abstract
We present periodicity and single-pulse searches at 1250 MHz for 22 radio-quiet gamma-ray pulsars, conducted using the Five-hundred-meter Aperture Spherical Radio Telescope (FAST). For PSR J1813$-$1246, we successfully detected pulsed signals with a spin period of 48.08 ms and a dispersion measure of 209.85 ${\rm pc cm^{-3}}$, consistent with the spin period measured at gamma-ray wavelengths. The estimated flux density is approximately 9 $\mu$Jy. For the remaining 21 sources, no radio emission was detected, with flux density upper limits of several $ \mu$Jy. The capability to detect pulsars with such low flux densities provides the opportunity to determine if and how these faint sources differ from much radio-brighter pulsars.
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FAST Discovery of $\mu$Jy Radio Pulsations from PSR J2238+5903, Providing a DM Distance Anchor for the Candidate TeV Halo 1LHAASO J2238+5900
First radio detection of PSR J2238+5903 yields DM = 247.5 ± 3.0 pc cm^{-3} and a model distance of 7.4 ± 3.9 kpc that anchors the physical scale and TeV efficiency of candidate halo 1LHAASO J2238+5900.