396 citations · 4.9k across the 117 of their papers we have counts for
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Simulating and interpreting deep observations in the Hubble Ultra Deep Field with the JWST/NIRSpec low-resolution 'prism'
Jacopo Chevallard, Emma Curtis-Lake, Stephane Charlot +16
The James Webb Space Telescope (JWST) will enable the detection of optical emission lines in galaxies spanning a broad range of luminosities out to redshifts z>10. Measurements of…
SILVERRUSH. V. Census of Lya, [OIII]5007, Ha, and [CII]158um Line Emission with ~1000 LAEs at z=4.9-7.0 Revealed with Subaru/HSC
Yuichi Harikane, Masami Ouchi, Takatoshi Shibuya +23
We investigate Lya, [OIII]5007, Ha, and [CII]158um emission from 1124 galaxies at z=4.9-7.0. Our sample is composed of 1092 Lya emitters (LAEs) at z=4.9, 5.7, 6.6, and 7.0 identifi…
The MUSE Hubble Ultra Deep Field Survey: III. Testing photometric redshifts to 30th magnitude
J. Brinchmann, H. Inami, R. Bacon +14
We tested the performance of photometric redshifts for galaxies in the Hubble Ultra Deep field down to 30th magnitude. We compared photometric redshift estimates from three spectra…
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…