activity
20202024
most citedThe Ultraluminous Lyman Alpha Luminosity Function at z=6.6

30 citations · 89 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2024

Spectroscopic Confirmation of a Massive Protocluster with Two Substructures at

Michael J. Nicandro Rosenthal, Amy J. Barger, Lennox L. Cowie +3

We present the results of a Keck and NOEMA spectroscopic survey of 507 galaxies, where we confirm the presence of two massive overdensities at and $z = 3.133 -…

astro-ph.GA2024

A Spectral Atlas of Lyman Alpha Emitters at z = 5.7 and z = 6.6

A. Songaila, L. L. Cowie, A. J. Barger +2

We present two uniformly observed spectroscopic samples of Ly-alpha emitters (LAEs) (127 at z = 5.7 and 82 at z = 6.6), which we use to investigate the evolution of the LAE populat…

astro-ph.GA2023★ 2 cited

JWST/NIRSpec Measurements of Extremely Low Metallicities in High Equivalent Width Lyman- Emitters

Michael V. Maseda, Zach Lewis, Jorryt Matthee +19

Deep VLT/MUSE optical integral field spectroscopy has recently revealed an abundant population of ultra-faint galaxies (; 0.01 ) at 2.96.7 due…

astro-ph.GA2023★ 15 cited

HEROES: The Hawaii eROSITA Ecliptic Pole Survey Catalog

A. J. Taylor, A. J. Barger, L. L. Cowie +3

We present a seven band (g, r, i, z, y, NB816, NB921) catalog derived from a Subaru Hyper Suprime-Cam (HSC) imaging survey of the North Ecliptic Pole (NEP). The survey, known as HE…

astro-ph.GA2022★ 3 cited

X-ray Sources in the SSA22 Chandra Field

Brandon T. Radzom, Anthony J. Taylor, Amy J. Barger +1

The Hawaii Survey Field SSA22 is the fourth deepest Chandra X-ray field. To allow for the fullest exploration of this field, we present new optical spectroscopy from Keck/DEIMOS an…

astro-ph.GA2022★ 6 cited

Properties of the Lowest Metallicity Galaxies Over the Redshift Range z = 0.2 to z = 1

Isaac H. Laseter, Amy J. Barger, Lennox L. Cowie +1

Low-metallicity galaxies may provide key insights into the evolutionary history of galaxies. Galaxies with strong emission lines and high equivalent widths (rest-frame EW(H-beta) >…