activity
20112026
most citedModelling and interpreting spectral energy distributions of galaxies with BEAGLE

418 citations · 7.8k across the 146 of their papers we have counts for

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Showing 2020Show all

11 papers · 1 filter

astro-ph.GA2020★ 50 cited

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…

astro-ph.GA2020★ 17 cited

Metal-THINGS: On the metallicity and ionization of ULX sources in NGC 925

Maritza A. Lara-López, Igor A. Zinchenko, Leonid S. Pilyugin +13

We present an analysis of the optical properties of three Ultra Luminous X-ray (ULX) sources identified in NGC 925. We use Integral field unit data from the George Mitchel spectrog…

astro-ph.GA2020★ 46 cited

How robustly can we constrain the low-mass end of the stellar mass function? -- The limits of lensing models and stellar population assumptions in the Hubble Frontier Fields

Lukas J. Furtak, Hakim Atek, Matthew D. Lehnert +2

We present new measurements of the very low-mass end of the galaxy stellar mass function (GSMF) at computed from a rest-frame ultraviolet selected sample of dropout gala…

astro-ph.GA2020★ 14 cited

Investigating Clumpy Galaxies in the Sloan Digital Sky Survey Stripe 82 using the Galaxy Zoo

Vihang Mehta, Claudia Scarlata, Lucy Fortson +7

Giant, star-forming clumps are a common feature prevalent amongst high-redshift star-forming galaxies and play a critical role in shaping their chaotic morphologies and yet, their…

astro-ph.GA2020★ 34 cited

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…

astro-ph.GA2020★ 87 cited

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…

astro-ph.GA2020★ 51 cited

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…

astro-ph.GA2020★ 49 cited

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 …

astro-ph.GA2020★ 157 cited

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…

astro-ph.GA2020★ 31 cited

Simulating JWST deep extragalactic imaging surveys and physical parameter recovery

O. B. Kauffmann, O. Le Fèvre, O. Ilbert +7

We present a new prospective analysis of deep multi-band imaging with the James Webb Space Telescope (JWST). In this work, we investigate the recovery of high-redshift gal…

astro-ph.GA2020★ 27 cited

Modelling the M*-SFR relation at high redshift: untangling factors driving biases in the intrinsic scatter measurement

E. Curtis-Lake, J. Chevallard, S. Charlot +1

We present a method to self-consistently propagate M and SFR () uncertainties onto intercept, slope and intrinsic scatter estimates for a simple model of the main sequence…