Calibration of mid- to far-infrared spectral lines in galaxies. Mordini, S., Spinoglio, L., & Fernández-Ontiveros, J. A. arXiv e-prints, 2105:arXiv:2105.04584, May, 2021. Paper abstract bibtex 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
@article{mordini_calibration_2021,
title = {Calibration of mid- to far-infrared spectral lines in galaxies},
volume = {2105},
url = {http://adsabs.harvard.edu/abs/2021arXiv210504584M},
abstract = {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},
urldate = {2021-05-12},
journal = {arXiv e-prints},
author = {Mordini, Sabrina and Spinoglio, Luigi and Fernández-Ontiveros, Juan Antonio},
month = may,
year = {2021},
keywords = {Astrophysics - Astrophysics of Galaxies},
pages = {arXiv:2105.04584},
}
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