559 citations · 17.3k across the 183 of their papers we have counts for
12 papers · 1 filter
Evidence for GN-z11 as a luminous galaxy at redshift 10.957
Linhua Jiang, Nobunari Kashikawa, Shu Wang +9
GN-z11 was photometrically selected as a luminous star-forming galaxy candidate at redshift z > 10 based on Hubble Space Telescope (HST) imaging data. Follow-up HST near-infrared g…
Lyman-alpha spectroscopy of extreme [OIII] emitting galaxies at : Implications for Ly visibility and LyC leakage at
Mengtao Tang, Daniel Stark, Jacopo Chevallard +3
Spectroscopic observations of massive galaxies selected to have extremely large [OIII]+H equivalent width (EW Å) have recently revealed large Ly detection ra…
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…
MMT Spectroscopy of Lyman-alpha at z7: Evidence for Accelerated Reionization Around Massive Galaxies
Ryan Endsley, Daniel P. Stark, Jacopo Chevallard +4
Reionization-era galaxies tend to exhibit weak Ly emission, likely reflecting attenuation from an increasingly neutral IGM. Recent observations have begun to reveal exceptions t…
The Lyman Continuum Escape Survey: Connecting Time-Dependent [OIII] and [OII] Line Emission with Lyman Continuum Escape Fraction in Simulations of Galaxy Formation
Kirk S. S. Barrow, Brant E. Robertson, Richard S. Ellis +4
Escaping Lyman continuum photons from galaxies likely reionized the intergalactic medium at redshifts . However, the Lyman continuum is not directly observable at these…
RELICS: Properties of z>5.5 Galaxies Inferred from Spitzer and Hubble Imaging Including A Candidate z~6.8 Strong [OIII] Emitter
Victoria Strait, Marusa Bradac, Dan Coe +26
We present constraints on the physical properties (including stellar mass, age, and star formation rate) of 207 galaxy candidates from the Reionization Lens…
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…
Rest-frame UV spectroscopy of extreme [OIII] emitters at : Toward a high-redshift UV reference sample for JWST
Mengtao Tang, Daniel Stark, Jacopo Chevallard +3
Deep spectroscopy of galaxies in the reionization-era has revealed intense CIII] and CIV line emission (EW Å). In order to interpret the nebular emission emerging at …
Exploring Chemical Homogeneity in Dwarf Galaxies: A VLT-MUSE study of JKB 18
Bethan L. James, Nimisha Kumari, Andrew Emerick +5
Deciphering the distribution of metals throughout galaxies is fundamental in our understanding of galaxy evolution. Nearby, low-metallicity, star-forming dwarf galaxies in particul…
Kinematics of the Circumgalactic Medium of a Galaxy from MgII Tomography
Kris Mortensen, Keerthi Vasan G. C., Tucker Jones +5
Galaxy evolution is thought to be driven in large part by the flow of gas between galaxies and the circumgalactic medium (CGM), a halo of metal-enriched gas extending out to $\gtrs…
Effects of self-consistent rest-ultraviolet colours in semi-empirical galaxy formation models
Jordan Mirocha, Charlotte Mason, Daniel P. Stark
Connecting the observed rest-ultraviolet (UV) luminosities of high- galaxies to their intrinsic luminosities (and thus star formation rates) requires correcting for the presence…
The [OIII]H Equivalent Width Distribution at z7: Implications for the Contribution of Galaxies to Reionization
Ryan Endsley, Daniel P. Stark, Jacopo Chevallard +1
We quantify the distribution of [OIII]+H line strengths at z7 using a sample of 20 bright (M 21) galaxies. We select these systems over wid…