Results 101 to 110 of about 78,206 (262)

Identifying Pulsar Candidates in Interferometric Radio Images Using Scintillation

open access: yesThe Astrophysical Journal
Pulsars have been primarily detected by their narrow pulses or periodicity in time domain data. Interferometric surveys for pulsars are challenging due to the trade-off between beam sensitivity and beam size and the corresponding tradeoff between survey ...
Jitendra Salal   +2 more
doaj   +1 more source

Timing the Parkes Multibeam Pulsars [PDF]

open access: yes, 1999
Measurement of accurate positions, pulse periods and period derivatives is an essential follow-up to any pulsar survey. The procedures being used to obtain timing parameters for the pulsars discovered in the Parkes multibeam pulsar survey are described ...
Bell, J. F.   +8 more
core   +1 more source

Searching for Gravitational-Wave Bursts from Cosmic String Cusps with the Parkes Pulsar Timing Array’s Third Data Release

open access: yesUniverse
Pulsar timing arrays (PTAs) are designed to detect nanohertz-frequency gravitational waves (GWs). Since GWs are anticipated from cosmic strings, PTAs offer a viable approach to testing their existence.
Yong Xia   +13 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

Observations of Anomalous X-ray Pulsars [PDF]

open access: green, 2001
G. L. Israel, S. Mereghetti, L. Stella
openalex   +1 more source

Measuring a Gravitomagnetic Effect with the Triple Pulsar PSR J0337+1715

open access: yesUniverse
To the first post-Newtonian order, the orbital angular momentum of the fast-revolving inner binary of the triple system PSR J0337+1715, made of a millisecond pulsar and a white dwarf, induces an annular gravitomagnetic field which displaces the line of ...
Lorenzo Iorio
doaj   +1 more source

Cracking the Endothelial Calcium (Ca2+) Code: A Matter of Timing and Spacing. [PDF]

open access: yesInt J Mol Sci, 2023
Moccia F   +4 more
europepmc   +1 more source

A binary pulsar in a 53-minute orbit. [PDF]

open access: yesNature, 2023
Pan Z   +17 more
europepmc   +1 more source

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