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The far-infrared, UV, and molecular gas relation in galaxies up to z = 2.5

MPS-Authors
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Lutz,  D.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Saintonge,  A.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Berta,  S.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Wuyts,  S.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Förster Schreiber,  N. M.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Genzel,  R.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Magnelli,  B.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Poglitsch,  A.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Popesso,  P.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Rosario,  D.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Sturm,  E.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Tacconi,  L. J.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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引用

Nordon, R., Lutz, D., Saintonge, A., Berta, S., Wuyts, S., Förster Schreiber, N. M., Genzel, R., Magnelli, B., Poglitsch, A., Popesso, P., Rosario, D., Sturm, E., & Tacconi, L. J. (2013). The far-infrared, UV, and molecular gas relation in galaxies up to z = 2.5. The Astrophysical Journal, 762(2):, pp. 1-15. doi:10.1088/0004-637X/762/2/125.


引用: https://hdl.handle.net/11858/00-001M-0000-000E-B573-A
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