AGN candidates in the VVV near-IR galaxy catalogue

Author:

Baravalle Laura D12,Schmidt Eduardo O12,Alonso M Victoria12,Pichel Ana3,Minniti Dante45,Rodríguez-Kamenetzky Adriana R1,Masetti Nicola46,Villalon Carolina1ORCID,Smith Leigh C7ORCID,Lucas Philip W8ORCID

Affiliation:

1. Instituto de Astronomía Teórica y Experimental (IATE, CONICET-UNC) , Córdoba, Argentina

2. Observatorio Astronómico de Córdoba, Universidad Nacional de Córdoba , Laprida 854, X5000BGR, Córdoba, Argentina

3. Instituto de Astronomía y Física del Espacio, CONICET-UBA , C1428ZAA Buenos Aires, Argentina

4. Instituto de Astrofísica, Facultad de Ciencias Exactas, Universidad Andrés Bello , Avenue Fernandez Concha 700, Las Condes, Santiago, 7591538 Chile

5. Vatican Observatory , V00120 Vatican City State, Italy

6. INAF - Osservatorio di Astrofisica e Scienza dello Spazio , via Piero Gobetti 101, I-40129 Bologna, Italy

7. Institute of Astronomy, University of Cambridge , Madingley Road, Cambridge CB3 0HA, UK

8. Centre for Astrophysics, University of Hertfordshire , College Lane, Hatfield AL10 9AB, UK

Abstract

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.

Funder

ESO

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 2 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Searching for globular clusters in the inner halo of the Circinus galaxy;Monthly Notices of the Royal Astronomical Society;2024-03-07

2. High energy gamma-ray sources in the VVV survey - II. The AGN counterparts;Monthly Notices of the Royal Astronomical Society;2024-03-06

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