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Update of the INTEGRAL/IBIS active galactic nuclei catalogue: Deeper on the Galactic plane and wider beyond
Indexado
WoS WOS:000953843800012
Scopus SCOPUS_ID:85150746320
DOI 10.1051/0004-6361/202245495
Año 2023
Tipo artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras


Abstract



In this work we have updated the list of active galactic nuclei (AGN) detected by INTEGRAL taking into account the new objects listed in the last published INTEGRAL/IBIS survey. We have collected 83 new AGN, increasing the number of INTEGRAL-detected active galaxies (436) by 19%. Half of these new additions are located behind the Galactic plane, and for most of them we have full X-ray coverage, obtained through archival data from Swift/XRT, XMM-Newton, and NuSTAR. The soft X-ray data allowed us to associate each high-energy emitter with a single or multiple X-ray counterpart(s) and characterise the spectral shape of these new AGN by estimating the photon index, the intrinsic absorption, and the 2-10 keV flux. A few cases where two soft X-ray counterparts fall within the INTEGRAL error circle and at least one is classified as an AGN have been found and discussed in detail. Thirty-four sources originally listed as AGN candidates or unidentified objects have been recognised as AGN by employing three diagnostic tests: WISE colours, radio emission, and morphology. For 12 sources among the 34 AGN candidates, we reduced the optical spectra and confirmed their AGN nature, providing also their optical class and redshift. This paper is part of an ongoing effort to keep the INTEGRAL AGN catalogue updated in order to provide the scientific community with a hard X-ray selected sample of well-classified and spectrally characterised active galaxies.

Revista



Revista ISSN
Astronomy & Astrophysics 0004-6361

Métricas Externas



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Disciplinas de Investigación



WOS
Astronomy & Astrophysics
Scopus
Sin Disciplinas
SciELO
Sin Disciplinas

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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional



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Autores - Afiliación



Ord. Autor Género Institución - País
1 Malizia, Angela Mujer Bologna Center - Italia
OAS Bologna - Italia
2 Bassani, L. Mujer Bologna Center - Italia
OAS Bologna - Italia
3 Landi, R. - Bologna Center - Italia
OAS Bologna - Italia
4 MOLINA-VILLAGRA, MATIAS Mujer INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan - Italia
IASF Milano - Italia
5 Masetti, N. Mujer Bologna Center - Italia
Universidad Nacional Andrés Bello - Chile
OAS Bologna - Italia
6 Palazzi, E. Mujer Bologna Center - Italia
OAS Bologna - Italia
7 Bruni, G. Mujer IAPS - Italia
IAPS Roma - Italia
8 Bazzano, A. Mujer IAPS - Italia
IAPS Roma - Italia
9 Ubertini, Pietro Hombre IAPS - Italia
IAPS Roma - Italia
10 Bird, Antony J. Hombre University of Southampton - Reino Unido
Univ Southampton - Reino Unido

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Financiamiento



Fuente
National Aeronautics and Space Administration
ASI
European Southern Observatory under ESO programs
American Sheep Industry Association

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos



Agradecimiento
The authors acknowledge financial support from ASI under contract n. 2019-35-HH.0. This research has made use of the NASA/IPAC Extragalactic Database (NED) and NASA/IPAC Infrared Science Archive, which are operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. This work made use of observations collected at the European Southern Observatory under ESO programs 0103.A-0521(A), 0102.D-0918(A), 0102.A-0433(A), and 0101.A-0765(A). The authors thank the anonymous referee for the useful comments.
The authors acknowledge financial support from ASI under contract n. 2019-35-HH.0. This research has made use of the NASA/IPAC Extragalactic Database (NED) and NASA/IPAC Infrared Science Archive, which are operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. This work made use of observations collected at the European Southern Observatory under ESO programs 0103.A-0521(A), 0102.D-0918(A), 0102.A-0433(A), and 0101.A-0765(A). The authors thank the anonymous referee for the useful comments.

Muestra la fuente de financiamiento declarada en la publicación.