93 citations · 127 across the 3 of their papers we have counts for
5 papers
Emission-line properties of IllustrisTNG galaxies: from local diagnostic diagrams to high-redshift predictions for JWST
Michaela Hirschmann, Stephane Charlot, Anna Feltre +8
We compute synthetic, rest-frame optical and ultraviolet (UV) emission-line properties of galaxy populations at redshifts from z0 to z=8 in a full cosmological framework.…
Stars and gas in the most metal-poor galaxies I: COS and MUSE observations of SBS 0335-052E
A. Wofford, A. Vidal-García, A. Feltre +5
Among the nearest most metal-poor starburst-dwarf galaxies known, SBS 0335-052E is the most luminous in integrated nebular He II λ4686 emission. This makes it a unique target to te…
Ultraviolet spectra of extreme nearby star-forming regions: evidence for an overabundance of very massive stars
Peter Senchyna, Daniel P. Stark, Stéphane Charlot +3
As deep spectroscopic campaigns extend to higher redshifts and lower stellar masses, the interpretation of galaxy spectra depends increasingly upon models for very young stellar po…
Extremely metal-poor galaxies with HST/COS: laboratories for models of low-metallicity massive stars and high-redshift galaxies
Peter Senchyna, Daniel P. Stark, Jacopo Chevallard +3
Ultraviolet (UV) observations of local star-forming galaxies have begun to establish an empirical baseline for interpreting the rest-UV spectra of reionization-era galaxies. Howeve…
Are LGRBs biased tracers of star formation? Clues from the host galaxies of the /BAT6 complete sample of bright LGRBs III: Stellar masses, star formation rates and metallicities at
J. T. Palmerio, S. D. Vergani, R. Salvaterra +11
(Abridged) Long gamma-ray bursts (LGRB) have been suggested as promising tracers of star formation owing to their association with the core-collapse of massive stars. The goal of t…