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dc.contributor.authorBaravalle, Laura D.
dc.contributor.authorSchmidt, Eduardo O.
dc.contributor.authorAlonso, M. Victoria
dc.contributor.authorPichel, Ana
dc.contributor.authorMinniti, Dante
dc.contributor.authorRodríguez-Kamenetzky, Adriana R.
dc.contributor.authorMasetti, Nicola
dc.contributor.authorVillalon, Carolina
dc.contributor.authorSmith, Leigh C.
dc.contributor.authorLucas, Philip W.
dc.date.accessioned2024-03-25T13:32:54Z
dc.date.available2024-03-25T13:32:54Z
dc.date.issued2023-04-30
dc.identifier.citationBaravalle , L D , Schmidt , E O , Alonso , M V , Pichel , A , Minniti , D , Rodríguez-Kamenetzky , A R , Masetti , N , Villalon , C , Smith , L C & Lucas , P W 2023 , ' AGN candidates in the VVV near-IR galaxy catalogue ' , Monthly Notices of the Royal Astronomical Society , vol. 520 , no. 4 , stad490 , pp. 5950-5959 . https://doi.org/10.1093/mnras/stad490
dc.identifier.issn1365-2966
dc.identifier.otherArXiv: http://arxiv.org/abs/2302.05595v1
dc.identifier.otherORCID: /0000-0002-8872-4462/work/152250010
dc.identifier.urihttp://hdl.handle.net/2299/27578
dc.description© 2023 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society. This is the accepted manuscript version of an article which has been published in final form at https://doi.org/10.1093/mnras/stad490
dc.description.abstractThe goal of this work is to search for Active Galactic Nuclei (AGN) in the Galactic disc at very low latitudes with |b|< 2°. For this, we studied the five sources from the VVV near-infrared (IR) galaxy catalogue that have also WISE counterparts and present variability in the VIrac VAriable Classification Ensemble (VIVACE) catalogue. In the near-IR colour-colour diagrams, these objects have in general redder colours compared to the rest of the sources in the field. In the mid-IR ones, they are located in the AGN region, however, there is a source that presents the highest interstellar extinction and different mid-IR colours to be a young stellar object (YSO). We also studied the source variability using two different statistical methods. The fractional variability amplitude σrms ranges from 12.6 to 33.8, being in concordance with previous results found for type-1 AGNs. The slopes of the light curves are in the range (2.6 - 4.7) × 10-4 mag d-1, also in agreement with results reported on quasars variability. The combination of all these results suggest that four galaxies are type-1 AGN candidates, whereas the fifth source likely a YSO candidate.en
dc.format.extent10
dc.format.extent7996443
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.subjectastro-ph.GA
dc.titleAGN candidates in the VVV near-IR galaxy catalogueen
dc.contributor.institutionCentre for Astrophysics Research (CAR)
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Climate Change Research (C3R)
dc.contributor.institutionCentre for Future Societies Research
dc.description.statusPeer reviewed
rioxxterms.versionofrecord10.1093/mnras/stad490
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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