AGN and starburst in bright Seyfert galaxies: from IR photometry to IR spectroscopy

TL;DR

This paper reviews the development of infrared photometry and spectroscopy techniques used to distinguish between AGN and starburst activity in Seyfert galaxies, highlighting key findings from IRAS, ISO, and Spitzer data.

Contribution

It provides a comprehensive review of multi-wavelength infrared studies of 12um Seyfert galaxies, integrating historical and recent spectroscopic data to inform unification and evolution models.

Findings

Infrared diagnostics effectively differentiate AGN and starburst emissions.

Spitzer spectroscopy has advanced understanding of galaxy energy sources.

Future missions will extend studies to higher redshifts.

Abstract

Infrared photometry and later infrared spectroscopy provided powerful diagnostics to distinguish between the main emission mechanisms in galaxies: AGN and Starburst. After the pioneering work on infrared photometry with IRAS in the far-IR and the S.Pedro Martir and ESO ground-based work in the near-IR, ISO photometry extended up to 200um the coverage of the galaxies energy distributions. Then Spitzer collected accurate mid-infrared spectroscopy on different samples of galaxies. We will review the work done on the 12um galaxy sample since the times of IRAS photometry to the new Spitzer spectroscopy. The main results on the multifrequency data of 12um selected Seyfert galaxies are presented and discussed in the light of unification and evolution models. The spectroscopic work of Spitzer will soon be complemented at longer wavelengths by the Herschel spectrometers and in the future by SPICA at higher redshift.