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NICER X-ray Observations of Seven Nearby Rotation-Powered Millisecond Pulsars

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arxiv 1912.05708 v1 pith:OL4ZRQZB submitted 2019-12-12 astro-ph.HE

classification astro-ph.HE
keywords x-raypulsarspulsationsdetectedmillisecondsigmabroadexhibit
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

NICER observed several rotation-powered millisecond pulsars to search for or confirm the presence of X-ray pulsations. When broad and sine-like, these pulsations may indicate thermal emission from hot polar caps at the magnetic poles on the neutron star surface. We report confident detections ($\ge4.7\sigma$ after background filtering) of X-ray pulsations for five of the seven pulsars in our target sample: PSR J0614-3329, PSR J0636+5129, PSR J0751+1807, PSR J1012+5307, and PSR J2241-5236, while PSR J1552+5437 and PSR J1744-1134 remain undetected. Of those, only PSR J0751+1807 and PSR J1012+5307 had pulsations previously detected at the 1.7$\sigma$ and almost 3$\sigma$ confidence levels, respectively, in XMM-Newton data. All detected sources exhibit broad sine-like pulses, which are indicative of surface thermal radiation. As such, these MSPs are promising targets for future X-ray observations aimed at constraining the neutron star mass-radius relation and the dense matter equation of state using detailed pulse profile modeling. Furthermore, we find that three of the detected millisecond pulsars exhibit a significant phase offset between their X-ray and radio pulses.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Fastest spinning millisecond pulsars: indicators for quark matter in neutron stars?

    nucl-th 2024-12 conditional novelty 6.0 of 10

    Hybrid stars with color-superconducting quark matter can reproduce the mass and spin of pulsar J0952-0607, whereas the hadronic-only model cannot, and the revised Kepler-frequency relation tightens radius bounds.

  2. A NICER view of the millisecond pulsar PSR J2124$-$3358: evidence for a helium atmosphere

    astro-ph.HE 2026-07 conditional novelty 5.5 of 10

    X-PSI modeling of NICER/Chandra data for PSR J2124−3358 substantially prefers a helium atmosphere, giving M = 1.8 ± 0.5 M⊙ and Req = 11.7^{+2.6}_{-3.0} km with two slightly non-antipodal hot spots.

  3. Rapidly Spinning Massive Pulsars as an Indicator of Quark Deconfinement

    nucl-th 2025-12 conditional novelty 4.0 of 10

    Within a tuned hybrid equation of state, a color-superconducting quark core—absent from the hyperonic hadronic model—is needed to reach the mass and spin of PSR J0952–0607.

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