Molecular gas content in strongly lensed z ~ 1.5−3 star-forming galaxies with low infrared luminosities
A&A, 577 (2015) A50
Published online: 2015-04-30
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H. Nayyeri, A. Cooray, E. Jullo, D. A. Riechers, T. K. D. Leung, D. T. Frayer, M. A. Gurwell, A. I. Harris, R. J. Ivison, M. Negrello, I. Oteo, S. Amber, A. J. Baker, J. Calanog, C. M. Casey, H. Dannerbauer, G. De Zotti, S. Eales, H. Fu, M. J. Michałowski, N. Timmons and J. L. WardlowThe Astrophysical Journal 844 (1) 82 (2017)
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Evolution of Cosmic Molecular Gas Mass Density from z ∼ 0 to z = 1–1.5
Fumiya Maeda, Kouji Ohta and Akifumi SekoThe Astrophysical Journal 835 (2) 120 (2017)
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A complete census ofHerschel-detected infrared sources within theHSTFrontier Fields
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Early science with the Large Millimeter Telescope: observations of extremely luminous high-zsources identified byPlanck
K. C. Harrington, Min S. Yun, R. Cybulski, et al.Monthly Notices of the Royal Astronomical Society 458 (4) 4383 (2016)
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GAS FRACTION AND DEPLETION TIME OF MASSIVE STAR-FORMING GALAXIES AT z ∼ 3.2: NO CHANGE IN GLOBAL STAR FORMATION PROCESS OUT TO z > 3
E. Schinnerer, B. Groves, M. T. Sargent, A. Karim, P. A. Oesch, B. Magnelli, O. LeFevre, L. Tasca, F. Civano, P. Cassata and V. SmolčićThe Astrophysical Journal 833 (1) 112 (2016)
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The Fundamental Plane of star formation in galaxies revealed by the EAGLE hydrodynamical simulations
Claudia del P. Lagos, Tom Theuns, Joop Schaye, et al.Monthly Notices of the Royal Astronomical Society 459 (3) 2632 (2016)
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Coevolution of metallicity and star formation in galaxies toz≃ 3.7 – II. A theoretical model
Leslie Hunt, Pratika Dayal, Laura Magrini and Andrea FerraraMonthly Notices of the Royal Astronomical Society 463 (2) 2020 (2016)
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Observational evidence of a slow downfall of star formation efficiency in massive galaxies during the past 10 Gyr
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New emerging results on molecular gas, stars, and dust at z ~ 2, as revealed by low star formation rate and low stellar mass star-forming galaxies
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Molecular gas, stars, and dust in sub-L ⋆ star-forming galaxies at z ~ 2: Evidence for universal star formation and non-universal dust-to-gas ratio
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A consistent view on star-forming galaxies at high redshift from multi-wavelength observations and SED modeling
Daniel Schaerer, Stephane de Barros and Frederic BooneProceedings of the International Astronomical Union 11 (S319) 45 (2015)
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ALMA detection of [C ii] 158μm emission from a strongly lensedz= 2.013 star-forming galaxy
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Molecular hydrogen abundances of galaxies in the EAGLE simulations
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A lower fragmentation mass scale in high-redshift galaxies and its implications on giant clumps: a systematic numerical study
Valentina Tamburello, Lucio Mayer, Sijing Shen and James WadsleyMonthly Notices of the Royal Astronomical Society 453 (3) 2491 (2015)
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Massive star clusters in high-redshift star-forming galaxies seen at a 100 pc scale thanks to strong gravitational lensing
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Early Science with the Large Millimeter Telescope: observations of dust continuum and CO emission lines of cluster-lensed submillimetre galaxies atz=2.0–4.7
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Evolution of the ISM in main-sequence versus starburst galaxies: A motivation for molecular deep fields
Manuel AravenaProceedings of the International Astronomical Union 11 (S315) 228 (2015)
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