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Journal Article

Near-infrared Emission Lines in Starburst Galaxies at 0.5 < z < 0.9: Discovery of a Merger Sequence of Extreme Obscurations

MPS-Authors

Calabrò,  A.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Daddi,  E.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Cassata,  P.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Onodera,  M.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Gobat,  R.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Puglisi,  A.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Jin,  S.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Liu,  D.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Amorín,  R.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Arimoto,  N.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Boquien,  M.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Carraro,  R.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Elbaz,  D.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Ibar,  E.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Juneau,  S.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Mannucci,  F.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Méndez Hernánez,  H.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Oliva,  E.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Rodighiero,  G.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Valentino,  F.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Zanella,  A.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

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Citation

Calabrò, A., Daddi, E., Cassata, P., Onodera, M., Gobat, R., Puglisi, A., et al. (2018). Near-infrared Emission Lines in Starburst Galaxies at 0.5 < z < 0.9: Discovery of a Merger Sequence of Extreme Obscurations. The Astrophysical Journal, 862.


Cite as: https://hdl.handle.net/21.11116/0000-0005-CE9A-6
Abstract
We obtained optical/near-IR rest-frame Magellan FIRE spectra (including Paβ and Paγ) of 25 starburst galaxies at 0.5 &lt; z &lt; 0.9, with average star formation rates (SFRs) seven times above the main sequence (MS). We find that Paschen-to-Balmer line ratios saturate around a constant value corresponding to A V ̃ 2-3 mag, while line-to-