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arXiv · 2407.01285

Search for rotating radio transients in monitoring data for three years

S. A. Tyul'bashev·M. A. Kitaeva·D. V. Pervoukhin·G. E. Tyul'basheva·E. A. Brylyakova·A. V. Chernosov·I. L. Ovchinnikov
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Abstract

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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S. A. Tyul'bashev, M. A. Kitaeva, D. V. Pervoukhin, G. E. Tyul'basheva, E. A. Brylyakova, A. V. Chernosov, I. L. Ovchinnikov. 2024-07-01. Search for rotating radio transients in monitoring data for three years. https://arxiv.org/abs/2407.01285

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