Timing solutions and basic properties are presented for two new pulsars, PSR J0535-0231 (415 ms, likely disrupted recycled) and PSR J1816-0518 (1.93 s), with noted shortfalls in NE2001 and YMW16 electron density models for the first.
van Straten \ and\ author M
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A 4200-hour campaign on FRB 20240114A finds that the highest-energy bursts account for most of the observed radio energy release, with a break in the energy distribution at ~2×10^40 erg and a linear DM rise of +0.96 pc cm^{-3} over 318 days.
FAST observations confirm periodic nulling in PSR B0751+32 at 35 percent fraction with evolving periodicity, stable-then-declining pulse components, and no subpulse drifting, challenging geometric models.
Coherent timing solutions at 150 MHz for 17 pulsars from Irish LOFAR observations, including 7 without prior solutions.
Wave mode coupling reproduces diverse frequency evolutions of circular polarization in pulsar single pulses, constraining multiplicity to 1-100 and Lorentz factor to 3-100, though the model fails to quantitatively fit most observed spectra.
citing papers explorer
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Discovery and Timing Follow-Up of Two FAST-Discovered Pulsars from the FAST CRAFTS Survey
Timing solutions and basic properties are presented for two new pulsars, PSR J0535-0231 (415 ms, likely disrupted recycled) and PSR J1816-0518 (1.93 s), with noted shortfalls in NE2001 and YMW16 electron density models for the first.
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A 4200-hour HyperFlash and \'ECLAT campaign on the hyperactive FRB 20240114A: constraining energetics with the most brilliant bursts
A 4200-hour campaign on FRB 20240114A finds that the highest-energy bursts account for most of the observed radio energy release, with a break in the energy distribution at ~2×10^40 erg and a linear DM rise of +0.96 pc cm^{-3} over 318 days.
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A study of periodic nulling in PSR B0751+32 with FAST
FAST observations confirm periodic nulling in PSR B0751+32 at 35 percent fraction with evolving periodicity, stable-then-declining pulse components, and no subpulse drifting, challenging geometric models.
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Pulsar timing solutions for 17 pulsars at 150 MHz from the Irish LOFAR station
Coherent timing solutions at 150 MHz for 17 pulsars from Irish LOFAR observations, including 7 without prior solutions.
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On the Diversity of Pulsar's Frequency-Dependent Circular Polarization
Wave mode coupling reproduces diverse frequency evolutions of circular polarization in pulsar single pulses, constraining multiplicity to 1-100 and Lorentz factor to 3-100, though the model fails to quantitatively fit most observed spectra.