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Multifrequency quasi-simultaneous observations of six low-synchrotron peaked blazars
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| dc.contributor.author | Mufakharov T. | |
| dc.contributor.author | Sotnikova Y. | |
| dc.contributor.author | Mingaliev M. | |
| dc.contributor.author | Erkenov A. | |
| dc.date.accessioned | 2018-09-18T20:31:00Z | |
| dc.date.available | 2018-09-18T20:31:00Z | |
| dc.date.issued | 2015 | |
| dc.identifier.issn | 1990-3413 | |
| dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/140684 | |
| dc.description.abstract | © Pleiades Publishing, Ltd., 2015. We made an estimation of the synchrotron peak frequency (ν<sup>s</sup><inf>peak</inf>) of the spectral energy distribution (SED) for six blazars. These objects were selected as very-low-synchrotron peaked (VLSP) blazar candidates (with ν<sup>s</sup><inf>peak</inf> ≤ 10<sup>13</sup> Hz).We have built the SED of the studied objects using quasi-simultaneous observations on the SAO RAS Zeiss-1000 and RATAN-600 telescopes and made an estimation of the synchrotron peak frequency. As a result, three sources (PKS0446+11, [HB89] 1308+326, and 3C345) were confirmed as VLSP, for the three remaining blazars the calculations have shown ν<sup>s</sup><inf>peak</inf> > 10<sup>13</sup> Hz. | |
| dc.relation.ispartofseries | Astrophysical Bulletin | |
| dc.subject | Galaxies | |
| dc.subject | General-BL Lacertae objects | |
| dc.subject | General-galaxies | |
| dc.subject | Jets-radio continuum | |
| dc.subject | Nuclei-galaxies | |
| dc.subject | Quasars | |
| dc.title | Multifrequency quasi-simultaneous observations of six low-synchrotron peaked blazars | |
| dc.type | Article | |
| dc.relation.ispartofseries-issue | 3 | |
| dc.relation.ispartofseries-volume | 70 | |
| dc.collection | Публикации сотрудников КФУ | |
| dc.relation.startpage | 273 | |
| dc.source.id | SCOPUS19903413-2015-70-3-SID84943255390 |
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Публикации сотрудников КФУ Scopus [24551]
Коллекция содержит публикации сотрудников Казанского федерального (до 2010 года Казанского государственного) университета, проиндексированные в БД Scopus, начиная с 1970г.