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The MUSE Hubble Ultra Deep Field Survey: VII. FeII* Emission in Star-Forming Galaxies
Hayley Finley, Nicolas Bouché, Thierry Contini +15
Non-resonant FeII* 2365, 2396, 2612, 2626 emission can potentially trace galactic winds in emission and provide useful constraints to wind models. From the 3'x3' mosaic of the Hubb…
The MUSE Hubble Ultra Deep Field Survey: IV. Global properties of C III] emitters
Michael V. Maseda, Jarle Brinchmann, Marijn Franx +12
The C III] 1907,1909 emission doublet has been proposed as an alternative to Lyman-alpha in redshift confirmations of galaxies at z > 6 since it is not attenuated by the largely ne…
Physical properties and H-ionizing-photon production rates of extreme nearby star-forming regions
Jacopo Chevallard, Stéphane Charlot, Peter Senchyna +7
Measurements of the galaxy UV luminosity function at z>6 suggest that young stars hosted in low-mass star-forming galaxies produced the bulk of hydrogen-ionizing photons necessary…
Ultraviolet spectra of extreme nearby star-forming regions --- approaching a local reference sample for JWST
Peter Senchyna, Daniel P. Stark, Alba Vidal-García +7
Nearby dwarf galaxies provide a unique laboratory in which to test stellar population models below . Such tests are particularly important for interpreting the surprisin…
Synthetic nebular emission from massive galaxies I: origin of the cosmic evolution of optical emission-line ratios
Michaela Hirschmann, Stephane Charlot, Anna Feltre +4
Galaxies occupy different regions of the [OIII]/H-versus-[NII]/H emission-line ratio diagram in the distant and local Universe. We investigate the o…