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Unveiling the nature of the "Green Pea" galaxies

R. Amorín, J. Vílchez, and E. Pérez-Montero. (2011)cite arxiv:1105.1477Comment: To appear in JENAM Symposium "Dwarf Galaxies: Keys to Galaxy Formation and Evolution", P. Papaderos, G. Hensler, S. Recchi (eds.). Lisbon, September 2010, Springer Verlag, in press.
DOI: 10.1007/978-3-642-22018-0_28

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Other publications of authors with the same name

The Bursty Star Formation Histories of Low-mass Galaxies at $0.4<z<1$ Revealed by Star Formation Rates Measured from FUV and H$\beta$Y. Guo, M. Rafelski, S. Faber, D. Koo, M. Krumholz, J. Trump, S. Willner, R. Amorín, G. Barro, E. Bell and 10 other author(s). (2016)cite arxiv:1604.05314Comment: 10 pages, 7 figures. Submitted to ApJ. Comments welcome.Analogs of primeval galaxies two billion years after the Big BangR. Amorín, A. Fontana, E. Pérez-Montero, M. Castellano, L. Guaita, A. Grazian, O. Fèvre, B. Ribeiro, D. Schaerer, L. Tasca and 23 other author(s). (2017)cite arxiv:1701.04416Comment: 25 pages, 8 figs, 2 tables. Accepted for publication.The Synchrony of Production & Escape: Half the Bright Ly$\alpha$ Emitters at $z\approx2$ have Lyman Continuum Escape Fractions $\approx50\%$R. Naidu, J. Matthee, P. Oesch, C. Conroy, D. Sobral, G. Pezzulli, M. Hayes, D. Erb, R. Amorín, M. Gronke and 7 other author(s). (2021)cite arxiv:2110.11961Comment: Submitted to MNRAS. Figure 4 and Table 2 show key results from the stacks. Figure 8 presents a unifying scheme for the LyC duty cycle. Our companion paper (Matthee & Naidu et al. 2021) works out implications of these results for the cosmic UV background at $z\approx2-8$. Comments warmly welcomed and greatly appreciated!.(Re)Solving Reionization with Ly\alpha: How Bright Ly\alpha Emitters account for the $z\approx2-8$ Cosmic Ionizing BackgroundJ. Matthee, R. Naidu, G. Pezzulli, M. Gronke, D. Sobral, P. Oesch, M. Hayes, D. Erb, D. Schaerer, R. Amorín and 5 other author(s). (2021)cite arxiv:2110.11967Comment: Submitted to MNRAS. Figure 2 shows the main result -- the comoving emissivity due to bright LAEs. Our fiducial model is based on results presented in our companion paper -- Naidu & Matthee et al. 2021. Comments welcome.Evidence of very low metallicity and high ionization state in a strongly lensed, star-forming dwarf galaxy at z=3.417R. Amorín, A. Grazian, M. Castellano, L. Pentericci, A. Fontana, V. Sommariva, A. van der Wel, M. Maseda, and E. Merlin. (2014)cite arxiv:1403.6470Comment: 5 pages, 3 figures and 1 table. Accepted for publication in ApJ Letters.Unveiling the nature of the "Green Pea" galaxiesR. Amorín, J. Vílchez, and E. Pérez-Montero. (2011)cite arxiv:1105.1477Comment: To appear in JENAM Symposium "Dwarf Galaxies: Keys to Galaxy Formation and Evolution", P. Papaderos, G. Hensler, S. Recchi (eds.). Lisbon, September 2010, Springer Verlag, in press.The Physical Conditions of Emission-Line Galaxies at Cosmic Dawn from JWST/NIRSpec Spectroscopy in the SMACS 0723 Early Release ObservationsJ. Trump, P. Haro, R. Simons, B. Backhaus, R. Amorín, M. Dickinson, V. Fernández, C. Papovich, D. Nicholls, L. Kewley and 54 other author(s). (2022)cite arxiv:2207.12388Comment: 13 pages, 6 figures. Submitted to AAS Journals. Comments welcome. Figure 3 set available https://www.dropbox.com/s/go83wpbq1nk5vfe/linefits.ps.The Low-Redshift Lyman Continuum Survey: Optically Thin and Thick Mg II Lines as Probes of Lyman Continuum EscapeX. Xu, A. Henry, T. Heckman, J. Chisholm, R. Marques-Chaves, F. Leclercq, D. Berg, A. Jaskot, D. Schaerer, G. Worseck and 7 other author(s). (2023)cite arxiv:2301.04087Comment: 12 pages, 5 figures, 2 tables, accepted to ApJ.Simulating and interpreting deep JWST/NIRSpec observations in the Hubble Ultra Deep FieldJ. Chevallard, E. Curtis-Lake, S. Charlot, P. Ferruit, G. Giardino, M. Franx, M. Maseda, R. Amorin, S. Arribas, A. Bunker and 9 other author(s). (2017)cite arxiv:1711.07481Comment: 20 pages, 14 figures, submitted to MNRAS.First Results from the KMOS Lens-Amplified Spectroscopic Survey (KLASS): Kinematics of Lensed Galaxies at Cosmic NoonC. Mason, T. Treu, A. Fontana, T. Jones, T. Morishita, R. Amorin, M. Bradac, E. Finney, A. Henry, A. Hoag and 4 other author(s). (2016)cite arxiv:1610.03075Comment: Submitted to ApJ.