Search for rotating radio transients in monitoring data for three years
Fuente:
arXiv
Enregistré dans:
| Auteurs principaux: | , , , , , , |
|---|---|
| Format: | Preprint |
| Publié: |
2024
|
| Sujets: | |
| Accès en ligne: | |
| Tags: |
Ajouter un tag
Pas de tags, Soyez le premier à ajouter un tag!
|
| _version_ | 1866913411774808064 |
|---|---|
| author | Tyul'bashev, S. A. Kitaeva, M. A. Pervoukhin, D. V. Tyul'basheva, G. E. Brylyakova, E. A. Chernosov, A. V. Ovchinnikov, I. L. |
| author_facet | Tyul'bashev, S. A. Kitaeva, M. A. Pervoukhin, D. V. Tyul'basheva, G. E. Brylyakova, E. A. Chernosov, A. V. Ovchinnikov, I. L. |
| contents | 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. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2407_01285 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Search for rotating radio transients in monitoring data for three years Tyul'bashev, S. A. Kitaeva, M. A. Pervoukhin, D. V. Tyul'basheva, G. E. Brylyakova, E. A. Chernosov, A. V. Ovchinnikov, I. L. High Energy Astrophysical Phenomena 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. |
| title | Search for rotating radio transients in monitoring data for three years |
| topic | High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2407.01285 |