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X-ray - Infrared relation of AGNs and search for highly obscured accretion in the AKARI NEP Field

Published online by Cambridge University Press:  10 June 2020

Takamitsu Miyaji Open the ORCID record for Takamitsu Miyaji [Opens in a new window]  and
AKARI NEP Survey Team
Takamitsu Miyaji
Affiliation:
Instituto de Astronomía, Universidad Nacional Autónoma de México, Km. 103 Carret. Tijuana-Ensendada, Ensenada, 22860 Mexico email: [email protected]
AKARI NEP Survey Team
Affiliation:
Instituto de Astronomía, Universidad Nacional Autónoma de México, Km. 103 Carret. Tijuana-Ensendada, Ensenada, 22860 Mexico email: [email protected]
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Abstract

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The infrared Astronomical Satellite AKARI conducted deep (∼0.4 deg2) and wide (∼ 5.4 deg2) surveys around the North Ecliptic Pole (NEP) with its InfraRed Camera (IRC) with nine filters continuously covering the 2–25 μm range. These photometric bands include three filters that fill the “ Spitzer gap” between the wavelength coverages of IRAC and MIPS. This unique feature has enabled us to make sensitive mid-infrared detection of AGN candidates at z∼1-2, based on the Spectral Energy Distribution (SED) fitting including hot dust emission in the AGN torus. This enables us to compare X-rays and the AGN torus component of the infrared emission to help us identify highly absorbed AGNs, including Compton-thick ones. We report our results of the Chandra observation of the AKARI NEP Deep Field and discuss the prospects for upcoming Spectrum-RG (eROSITA+ART-XC) on the AKARI Wide field.

Keywords

galaxies: activeinfrared: galaxiesX-rays: galaxies
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S341: Challenges in Panchromatic Modelling with Next Generation Facilities , November 2019 , pp. 172 - 176
Copyright
© International Astronomical Union 2020

References

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