A transitional millisecond pulsar showed a brief shift to a single-peaked optical pulse profile with increased amplitude and flaring before returning to its standard double-peaked shape.
Title resolution pending
5 Pith papers cite this work. Polarity classification is still indexing.
years
2026 5verdicts
UNVERDICTED 5representative citing papers
SDSSJ110546.07+145202.4 is the first known long-duration radio changing-look NLS1 galaxy whose outburst is explained by an accretion-rate change that triggered a powerful radio jet.
XRISM Resolve measures the lowest turbulent velocity yet in a cluster core, indicating Abell 496 is dynamically quiescent despite prior cold fronts and weak radio activity.
Simulations show that iterative source removal and maximum likelihood decoding can recover point-source positions and fluxes from 1.5D coded-aperture data with 5-arcmin resolution in one axis and 5-degree resolution in the other.
A catalog of 251 soft X-ray counterparts for 250 unassociated Swift-BAT hard X-ray sources classifies 94 as AGN and 58 as galaxies with supporting redshift and limited optical data.
citing papers explorer
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There and back again: Mysterious optical pulse profile behavior of the transitional millisecond pulsar PSR J1023+0038
A transitional millisecond pulsar showed a brief shift to a single-peaked optical pulse profile with increased amplitude and flaring before returning to its standard double-peaked shape.
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SDSSJ110546.07+145202.4: The first long-duration radio changing-look NLS1 galaxy
SDSSJ110546.07+145202.4 is the first known long-duration radio changing-look NLS1 galaxy whose outburst is explained by an accretion-rate change that triggered a powerful radio jet.
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The Quiescent Sloshing Core of Abell 496 with XRISM
XRISM Resolve measures the lowest turbulent velocity yet in a cluster core, indicating Abell 496 is dynamically quiescent despite prior cold fronts and weak radio activity.
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Simulations of a 2 x 1.5D coded aperture camera for X-ray astronomy
Simulations show that iterative source removal and maximum likelihood decoding can recover point-source positions and fluxes from 1.5D coded-aperture data with 5-arcmin resolution in one axis and 5-degree resolution in the other.
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Source identification for the Swift-BAT 150-month hard X-ray catalog using soft X-ray observations
A catalog of 251 soft X-ray counterparts for 250 unassociated Swift-BAT hard X-ray sources classifies 94 as AGN and 58 as galaxies with supporting redshift and limited optical data.