Identifying active galactic nuclei via brightness temperature with sub-arcsecond international LOFAR telescope observations
| dc.contributor.author | Morabito, Leah K. | |
| dc.contributor.author | Sweijen, F. | |
| dc.contributor.author | Radcliffe, Jack Frederick | |
| dc.contributor.author | Best, P.N. | |
| dc.contributor.author | Kondapally, Rohit | |
| dc.contributor.author | Bondi, Marco | |
| dc.contributor.author | Bonato, Matteo | |
| dc.contributor.author | Duncan, K.J. | |
| dc.contributor.author | Prandoni, Isabella | |
| dc.contributor.author | Shimwell, T.W. | |
| dc.contributor.author | Williams, W.L. | |
| dc.contributor.author | Van Weeren, R.J. | |
| dc.contributor.author | Conway, J.E. | |
| dc.contributor.author | Rivera, G. Calistro | |
| dc.date.accessioned | 2023-07-24T12:12:32Z | |
| dc.date.available | 2023-07-24T12:12:32Z | |
| dc.date.issued | 2022-10 | |
| dc.description | DATA AVAILABILITY : DATA AVAILABILITY The data used in this paper come from Sweijen et al. (2022) and the LoTSS Deep Fields Data Release 1, for which the radio data are presented in Tasse et al. (2021) and made publicly available through both the Centre de Données astronomiques de Strasbourg (CDS) and through the LOFAR Surveys website (https://lofar-surveys.org/deepfields.html). Multiwavelength photometric catalogues and photometric redshifts come from Kondapally et al. (2021) and Duncan et al. (2021), respectively, both of which are also available through CDS and the LOFAR Surveys website. The radio data from Sweijen et al. (2022) are also available on the LOFAR Surveys website (https://lofar-surveys.org/hdfields.html) and we make additional use of the deconvolved sizes which are available upon request. These data were supplemented with SED fitting results presented in Best et al. (in preparation), which are available on request and will be published with the Best et al. paper, through https://lofar-surveys.org/deepfields.html. Supporting information was taken from tables published in Middelberg et al. (2013) and Woo & Urry (2002), and are available in csv format at https://github.com/lmorabit/AGNdetect, where the publicly available code for the analysis presented here can also be found. The data used in this paper come from Sweijen et al. (2022) and the LoTSS Deep Fields Data Release 1, for which the radio data are presented in Tasse et al. (2021) and made publicly available through both the Centre de Données astronomiques de Strasbourg (CDS) and through the LOFAR Surveys website (https://lofar-surveys.org/deepfields.html). Multiwavelength photometric catalogues and photometric redshifts come from Kondapally et al. (2021) and Duncan et al. (2021), respectively, both of which are also available through CDS and the LOFAR Surveys website. The radio data from Sweijen et al. (2022) are also available on the LOFAR Surveys website (https://lofar-surveys.org/hdfields.html) and we make additional use of the deconvolved sizes which are available upon request. These data were supplemented with SED fitting results presented in Best et al. (in preparation), which are available on request and will be published with the Best et al. paper, through https://lofar-surveys.org/deepfields.html. Supporting information was taken from tables published in Middelberg et al. (2013) and Woo & Urry (2002), and are available in csv format at https://github.com/lmorabit/AGNdetect, where the publicly available code for the analysis presented here can also be found. | en_US |
| dc.description.abstract | Please read abstract in the article. | en_US |
| dc.description.department | Physics | en_US |
| dc.description.librarian | hj2023 | en_US |
| dc.description.sponsorship | The European Union’s Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie grant agreement; the Medical Research Council ; the UK STFC via grant; INAF under the SKA/CTA PRIN ‘FORECaST’ and the PRIN MAIN STREAM ‘SAuROS’ projects; the CAS-NWO programme for radio astronomy which is financed by the Netherlands Organisation for Scientific Research (NWO); the ERC Starting Grant. | en_US |
| dc.description.uri | https://academic.oup.com/mnras | en_US |
| dc.identifier.citation | Leah K. Morabito and others, Identifying active galactic nuclei via brightness temperature with sub-arcsecond international LOFAR telescope observations, Monthly Notices of the Royal Astronomical Society, Volume 515, Issue 4, October 2022, Pages 5758–5774, https://doi.org/10.1093/mnras/stac2129. | en_US |
| dc.identifier.issn | 0035-8711 (print) | |
| dc.identifier.issn | 1365-2966 (online) | |
| dc.identifier.other | 10.1093/mnras/stac2129 | |
| dc.identifier.uri | http://hdl.handle.net/2263/91599 | |
| dc.language.iso | en | en_US |
| dc.publisher | Oxford University Press | en_US |
| dc.rights | © 2020 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society. This article is distributed under the Creative Commons Attribution License. | en_US |
| dc.subject | Acceleration of particles | en_US |
| dc.subject | Radiation mechanisms: non-thermal | en_US |
| dc.subject | Galaxies: active | en_US |
| dc.subject | Galaxies: jets | en_US |
| dc.subject | Radio continuum: galaxies | en_US |
| dc.title | Identifying active galactic nuclei via brightness temperature with sub-arcsecond international LOFAR telescope observations | en_US |
| dc.type | Article | en_US |