Results 81 to 90 of about 16,242 (188)

A Systematic Search for Redback and Black Widow Candidates Based on the 4FGL-DR3 Unassociated Sources and the Zwicky Transient Facility Data

open access: yesThe Astrophysical Journal
Spider pulsars represent a unique subclass of radio millisecond pulsars in binaries, and are further categorized into black widows and redbacks according to the mass of the low-mass companion.
Chunyan Lu   +5 more
doaj   +1 more source

Investigation of Accuracy of TOA and SNR of Radio Pulsar Signals for Vehicles Navigation. [PDF]

open access: yesSensors (Basel), 2023
Kabakchiev H   +4 more
europepmc   +1 more source

Discovery of the Accretion-powered Millisecond X-Ray Pulsar IGR J00291+5934 [PDF]

open access: bronze, 2005
D. K. Galloway   +4 more
openalex   +1 more source

SAX J1808.4−3658, an accreting millisecond pulsar shining in gamma rays? [PDF]

open access: bronze, 2015
E. de Oña Wilhelmi   +9 more
openalex   +1 more source

Deciphering Profile Stability in Millisecond Pulsars: Timescales, Frequency Evolution, and Implications on Emission Mechanisms

open access: yesThe Astrophysical Journal
Pulse profile stability in millisecond pulsars (MSPs) is a key factor in achieving high-precision timing essential for detecting nanohertz gravitational waves with pulsar timing arrays (PTAs).
Ankita Ghosh   +5 more
doaj   +1 more source

Chandra observations of the millisecond X-ray pulsar IGR J00291+5934 in quiescence [PDF]

open access: bronze, 2005
P. G. Jonker   +7 more
openalex   +1 more source

Pulse Profile Variability of PSR J1022+1001 in NANOGrav Data

open access: yesThe Astrophysical Journal
Pulse profile stability is a central assumption of standard pulsar timing methods. Thus, it is important for pulsar timing array experiments such as the North American Nanohertz Observatory for Gravitational Waves (NANOGrav) to account for any pulse ...
William Fiore   +48 more
doaj   +1 more source

An Unusual Pulse Shape Change Event in PSR J1713+0747 Observed with the Green Bank Telescope and CHIME

open access: yesThe Astrophysical Journal
The millisecond pulsar J1713+0747 underwent a sudden and significant pulse shape change between 2021 April 16 and 17 (MJDs 59320 and 59321). Subsequently, the pulse shape gradually recovered over the course of several months.
Ross J. Jennings   +43 more
doaj   +1 more source

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