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dc.contributor.author | Mufakharov T. | |
dc.contributor.author | Mikhailov A. | |
dc.contributor.author | Sotnikova Y. | |
dc.contributor.author | Mingaliev M. | |
dc.contributor.author | Stolyarov V. | |
dc.contributor.author | Erkenov A. | |
dc.contributor.author | Nizhelskij N. | |
dc.contributor.author | Tsybulev P. | |
dc.date.accessioned | 2022-02-09T20:31:55Z | |
dc.date.available | 2022-02-09T20:31:55Z | |
dc.date.issued | 2021 | |
dc.identifier.issn | 0035-8711 | |
dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/168799 | |
dc.description.abstract | We report the first detection at 4.7 and 8.2 GHz with the RATAN-600 radio telescope of the source PSO J047.4478+27.2992, which has been announced as a blazar at z = 6.1. The average flux densities are 12 ± 3 and 8 ± 4 mJy at 4.7 and 8.2 GHz respectively, and an upper limit is estimated as 3 mJy at 11.2 GHz. The light curve at 4.7 GHz, obtained on a time-scale of four months, exhibits moderate variability of the source (fractional variability Fvar = 0.28 ± 0.02). The new RATAN-600 measurements extend previous literature data to higher frequencies, indicating a single power-law radio spectrum with α0.147-8.2 = −0.51 ± 0.1. The monochromatic radio luminosity at 4.7 GHz Pν ∼ 2 × 1027 W Hz−1 is consistent with values for high-redshift quasars at z ≥ 3. | |
dc.relation.ispartofseries | Monthly Notices of the Royal Astronomical Society | |
dc.subject | Galaxies: high-redshift | |
dc.subject | Quasars: general | |
dc.subject | Quasars: individual: NVSS J030947+271757 | |
dc.subject | Radio continuum: galaxies | |
dc.title | Flux-density measurements of the high-redshift blazar PSO J047.4478+27.2992 at 4.7 and 8.2 GHz with RATAN-600 | |
dc.type | Article | |
dc.relation.ispartofseries-issue | 3 | |
dc.relation.ispartofseries-volume | 503 | |
dc.collection | Публикации сотрудников КФУ | |
dc.relation.startpage | 4662 | |
dc.source.id | SCOPUS00358711-2021-503-3-SID85116321525 |