The Past and Future of Mid-Infrared Studies of AGN

Observational studies of AGN in the mid-infrared regime are crucial to our understanding of AGN and their role in the evolution of galaxies. Mid-IR-based selection of AGN is complementary to more traditional techniques allowing for a more complete census of AGN activity across cosmic time. Mid-IR ob...

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Main Authors: Anna Sajina, Mark Lacy, Alexandra Pope
Format: Article
Language:English
Published: MDPI AG 2022-06-01
Series:Universe
Subjects:
Online Access:https://www.mdpi.com/2218-1997/8/7/356
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author Anna Sajina
Mark Lacy
Alexandra Pope
author_facet Anna Sajina
Mark Lacy
Alexandra Pope
author_sort Anna Sajina
collection DOAJ
description Observational studies of AGN in the mid-infrared regime are crucial to our understanding of AGN and their role in the evolution of galaxies. Mid-IR-based selection of AGN is complementary to more traditional techniques allowing for a more complete census of AGN activity across cosmic time. Mid-IR observations including time variability and spatially resolved imaging have given us unique insights into the nature of the obscuring structures around AGN. The wealth of fine structure, molecular, and dust features in the mid-IR allow us to simultaneously probe multiple components of the ISM allowing us to explore in detail the impact on the host galaxy by the presence of an AGN—a crucial step toward understanding galaxy-SMBH co-evolution. This review gives a broad overview of this wide range of studies. It also aims to show the evolution of this field starting with its nascency in the 1960s, through major advances thanks to several generations of space-based and ground-based facilities, as well as the promise of upcoming facilities such as the James Webb Space Telescope (<i>JWST</i>).
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spelling doaj.art-257143ce92964248960cd9516cee85712023-11-30T22:01:59ZengMDPI AGUniverse2218-19972022-06-018735610.3390/universe8070356The Past and Future of Mid-Infrared Studies of AGNAnna Sajina0Mark Lacy1Alexandra Pope2Department of Physics & Astronomy, Tufts University, Medford, MA 02155, USANational Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903, USADepartment of Astronomy, University of Massachusetts, Amherst, MA 01003, USAObservational studies of AGN in the mid-infrared regime are crucial to our understanding of AGN and their role in the evolution of galaxies. Mid-IR-based selection of AGN is complementary to more traditional techniques allowing for a more complete census of AGN activity across cosmic time. Mid-IR observations including time variability and spatially resolved imaging have given us unique insights into the nature of the obscuring structures around AGN. The wealth of fine structure, molecular, and dust features in the mid-IR allow us to simultaneously probe multiple components of the ISM allowing us to explore in detail the impact on the host galaxy by the presence of an AGN—a crucial step toward understanding galaxy-SMBH co-evolution. This review gives a broad overview of this wide range of studies. It also aims to show the evolution of this field starting with its nascency in the 1960s, through major advances thanks to several generations of space-based and ground-based facilities, as well as the promise of upcoming facilities such as the James Webb Space Telescope (<i>JWST</i>).https://www.mdpi.com/2218-1997/8/7/356dusty galaxiesobscured AGNISM
spellingShingle Anna Sajina
Mark Lacy
Alexandra Pope
The Past and Future of Mid-Infrared Studies of AGN
Universe
dusty galaxies
obscured AGN
ISM
title The Past and Future of Mid-Infrared Studies of AGN
title_full The Past and Future of Mid-Infrared Studies of AGN
title_fullStr The Past and Future of Mid-Infrared Studies of AGN
title_full_unstemmed The Past and Future of Mid-Infrared Studies of AGN
title_short The Past and Future of Mid-Infrared Studies of AGN
title_sort past and future of mid infrared studies of agn
topic dusty galaxies
obscured AGN
ISM
url https://www.mdpi.com/2218-1997/8/7/356
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