Calibration of mid- to far-infrared spectral lines in galaxies

Mid- to far-infrared (IR) lines are suited to study dust obscured regions in galaxies, because IR spectroscopy allows us to explore the most hidden regions where heavily obscured star formation as well as accretion onto supermassive black-holes occur. This is mostly important at redshifts of 1

Keywords:

• Astrophysics
• Star formation
• accretion
• Dwarf galaxy
• Spectral line
• Metallicity
• Population
• Physics
• Galaxy
• Redshift

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