Discovery of a radio emitting neutron star with an ultra-long spin period of 76 seconds. [PDF]
Caleb M +21 more
europepmc +1 more source
OUT OF THE FRYING PAN: A YOUNG PULSAR WITH A LONG RADIO TRAIL EMERGING FROM SNR G315.9-0.0 [PDF]
F. Camilo +6 more
openalex +1 more source
Pulsar Gleaners: Discovery of 19 Pulsars in FAST Archival Data at ∣b∣ < 5° and Decl. < −5°
We report the discovery of 19 new pulsars identified from archival observations of the Five-hundred-meter Aperture Spherical radio Telescope (FAST) within Galactic latitudes ∣ b ∣ < 5° and declinations decl. < −5°. The dataset was recorded using FAST’s L
Shi-Jie Gao, Yi-Xuan Shao, Xiang-Dong Li
doaj +1 more source
Radio emission from polar caps in pulsars [PDF]
J. Kuijpers, M. Volwerk
openalex +1 more source
Discovery of a Periodic Radio Signal from the Formerly Radio-quiet γ-Ray Pulsar J0359+5414 with FAST
In this paper, we report the detection of a periodic radio signal from the radio-quiet γ -ray pulsar PSR J0359+5414, using the Five-hundred-meter Aperture Spherical radio Telescope. This pulsar has a rotational period of 79.42 ms determined in the γ -ray
Ruobin Ding +10 more
doaj +1 more source
Upgraded antennas for pulsar observations in the Argentine Institute of Radio astronomy [PDF]
G. Gancio +11 more
openalex +1 more source
Radio timing constraints on the mass of the binary pulsar PSR J1528−3146 [PDF]
A. Berthereau +9 more
openalex +1 more source
FAST Observation of Polarized Radio Emission of Rotating Radio Transient J2325−0530
In this study, we present a detailed analysis of single-pulse emission from the rotating radio transient (RRAT) J2325−0530, observed at 1250 MHz using the Five-hundred-meter Aperture Spherical Radio Telescope.
Shi-jun Dang +8 more
doaj +1 more source
An updated nuclear-physics and multi-messenger astrophysics framework for binary neutron star mergers. [PDF]
Pang PTH +20 more
europepmc +1 more source
Electric Field Screening in Pair Discharges and Generation of Pulsar Radio Emission
Elizabeth A. Tolman +2 more
openalex +1 more source

