The evolution of the IR luminosity function and dust-obscured star formation over the past 13 billion years

Zavala, J.A.; Casey, C.M.; Manning, S.M.; Aravena, M.; Bethermin, M.; Caputi, K.I.; ... ; Yun, M.S. (2021)

Article / Letter to editor

• Galaxy Evolution
• Galaxies
• Dust Continuum Emission
• Millimeter Astronomy
• Submillimeter Astronomy
• Star Formation
• High-Redshift Galaxies
• Surveys
• Galaxy Counts
• Luminosity Function
• 594
• 573
• 412
• 1061
• 1647
• 1569
• 734
• 1671
• 588
• 942
• Astrophysics - Astrophysics of Galaxies

• All authors: Zavala, J.A.; Casey, C.M.; Manning, S.M.; Aravena, M.; Bethermin, M.; Caputi, K.I.; Clements, D.L.; da Cunha, E.; Drew, P.; Finkelstein, S.L.; Fujimoto, S.; Hayward, C.; Hodge, J.A.; Kartaltepe, J.S.; Knudsen, K.; Koekemoer, A.M.; Long, A.S.; Magdis, G.E.; Man, A.W.S.; Popping, G.; Sanders, D.; Scoville, N.; Sheth, K.; Staguhn, J.; Toft, S.; Treister, E.; Vieira, J.D.; Yun, M.S.
• Date: 2021
• Journal: The Astrophysical Journal
• Volume: 909
• Issue: 2
• DOI: doi:10.3847/1538-4357/abdb27
• Link: https://ui.adsabs.harvard.edu/abs/2021ApJ...909..165Z