activity
19952026
most citedThe Near-Infrared Spectrograph (NIRSpec) on the James Webb Space Telescope I. Overview of the instrument and its capabilities

665 citations · 17.8k across the 389 of their papers we have counts for

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Showing 2013 · astro-ph.COShow all

8 papers · 2 filters

astro-ph.CO2013★ 157 cited

Spectroscopy of z ~ 7 candidate galaxies: Using Lyman-alpha to constrain the neutral fraction of hydrogen in the high-redshift universe

Joseph Caruana, Andrew J. Bunker, Stephen M. Wilkins +4

Following our previous spectroscopic observations of galaxies with Gemini/GNIRS and VLT/XSHOOTER, which targeted a total of 8 objects, we present here our results from a deep…

astro-ph.CO2013★ 125 cited

Low Masses and High Redshifts: The Evolution of the Mass-Metallicity Relation

Alaina Henry, Claudia Scarlata, Alberto Dominguez +15

We present the first robust measurement of the high redshift mass-metallicity (MZ) relation at 10^{8}< M/M_{\sun} < 10^{10}, obtained by stacking spectra of 83 emission-line galaxi…

astro-ph.CO2013★ 40 cited

Theoretical predictions for the effect of nebular emission on the broad band photometry of high-redshift galaxies

Stephen M. Wilkins, William Coulton, Joseph Caruana +6

By combining optical and near-IR observations from the Hubble Space Telescope with NIR photometry from the Spitzer Space Telescope it is possible to measure the rest-frame UV-optic…

astro-ph.CO2013★ 85 cited

Predicting Future Space Near-IR Grism Surveys using the WFC3 Infrared Spectroscopic Parallels Survey

James W. Colbert, Harry Teplitz, Hakim Atek +13

We present near-infrared emission line counts and luminosity functions from the HST WFC3 Infrared Spectroscopic Parallels (WISP) program for 29 fields (0.037 deg^2) observed using…

astro-ph.CO2013★ 69 cited

Interpreting the observed UV continuum slopes of high-redshift galaxies

Stephen M. Wilkins, Andrew Bunker, William Coulton +4

The observed UV continuum slope of star forming galaxies is strongly affected by the presence of dust. Its observation is then a potentially valuable diagnostic of dust attenuation…

astro-ph.CO2013★ 24 cited

VLT/XSHOOTER & Subaru/MOIRCS Spectroscopy of HUDF-YD3: No Evidence for Lyman-alpha Emission at z=8.55

Andrew J. Bunker, Joseph Caruana, Stephen M. Wilkins +5

We present spectroscopic observations with VLT/XSHOOTER and Subaru/MOIRCS of a relatively bright Y-band drop-out galaxy in the Hubble Ultra Deep Field, first selected by Bunker et…

astro-ph.CO2013★ 7 cited

Confronting predictions of the galaxy stellar mass function with observations at high-redshift

Stephen M. Wilkins, Tiziana Di Matteo, Rupert Croft +4

We investigate the evolution of the galaxy stellar mass function at high-redshift () using a pair of large cosmological hydrodynamical simulations: {\em MassiveBlack} and {…

astro-ph.CO2013

Luminosities, Masses and Star Formation Rates of Galaxies at High Redshift (IAU279 conference proceedings)

Andrew Bunker

There has been great progress in recent years in discovering star forming galaxies at high redshifts (z>5), close to the epoch of reionization of the intergalactic medium (IGM). Th…