Identifying active galactic nuclei via brightness temperature with sub-arcsecond international LOFAR telescope observations

Morabito, Leah K.; Sweijen, F.; Radcliffe, Jack Frederick; Best, P.N.; Kondapally, Rohit; Bondi, Marco; Bonato, Matteo; Duncan, K.J.; Prandoni, Isabella; Shimwell, T.W.; Williams, W.L.; Van Weeren, R.J.; Conway, J.E.; Rivera, G. Calistro

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