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Search for rotating radio transients in monitoring data for three years

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arxiv 2407.01285 v1 pith:ZCLYEEUA submitted 2024-07-01 astro-ph.HE

S.A. Tyul'bashev , M.A. Kitaeva , D.V. Pervoukhin , G.E. Tyul'basheva , E.A. Brylyakova , A.V. Chernosov , I.L. Ovchinnikov This is my paper · ORCID
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The search for rotating radio transients (RRAT) was done at a frequency of 111 MHz, in daily observations carried out on the radio telescope, a Large Phased Array (LPA) at declinations -9o < decj < +42o. 19 new RRATs were discovered for dispersion measures (DM) from 2.5 to 72.6 pc cm^{-3}. Estimates of the periods were obtained for three RRATs. Two of them (J0408+28; J0440+35) are located at distances of 134 and 136 pc from Sun and are among the closest of all known RRATs.

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  1. Low-frequency observations of low-mass binary systems with neutron star candidates

    astro-ph.HE 2025-09 conditional novelty 5.0 of 10

    A 111 MHz archival search finds no periodic radio emission from five compact-object binaries and one ambiguous 13 Jy, 0.13 s burst toward J1527+3536.

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