activity
20162022
most citedThe quantum efficiency and diffractive image artifacts of Si:As IBC mid-IR detector arrays at 5 10 m: Implications for the JWST/MIRI detectors

49 citations · 118 across the 5 of their papers we have counts for

collaborators

12 papers

astro-ph.GA20227 cited

Measuring the Total Ultraviolet Light from Galaxy Clusters at z=0.5-1.6: The Balance of Obscured and Unobscured Star-Formation

Jed McKinney, Vandana Ramakrishnan, Kyoung-Soo Lee +4

Combined observations from UV to IR wavelengths are necessary to fully account for the star-formation in galaxy clusters. Low mass (log M/Msun<10) galaxies are typically not indivi…

astro-ph.GA202217 cited

Significant Molecular Gas Deficiencies in Star-forming Cluster Galaxies at

Stacey Alberts, Jéa Adams, Benjamin Gregg +3

We present the average gas properties derived from ALMA Band 6 dust continuum imaging of 126 massive (log ), star-forming cluster galaxies acros…

astro-ph.GA20221 cited

ALMA measures molecular gas reservoirs comparable to field galaxies in a low-mass galaxy cluster at z=1.3

Christina C. Williams, Stacey Alberts, Justin S. Spilker +6

We report the serendipitous discovery of an overdensity of CO emitters in an X-ray-identified cluster (LogM at z=1.3188) using ALMA. We presen…

astro-ph.IM202049 cited

The quantum efficiency and diffractive image artifacts of Si:As IBC mid-IR detector arrays at 5 10 m: Implications for the JWST/MIRI detectors

Andras Gaspar, George H. Rieke, Pierre Guillard +6

Arsenic doped back illuminated blocked impurity band (BIBIB) silicon detectors have advanced near and mid-IR astronomy for over thirty years; they have high quantum efficiency (QE)…

astro-ph.GA2020

Completing the Census of AGN in GOODS-S/HUDF: New Ultra-Deep Radio Imaging and Predictions for JWST

Stacey Alberts, Wiphu Rujopakarn, George Rieke +2

A global understanding of Active Galactic Nuclei (AGN) and their host galaxies hinges on completing a census of AGN activity without selection biases down to the low-luminosity reg…

astro-ph.GA2020

Measuring the total infrared light from galaxy clusters at z=0.5-1.6: connecting stellar populations to dusty star formation

Stacey Alberts, Kyoung-Soo Lee, Alexandra Pope +13

Massive galaxy clusters undergo strong evolution from z~1.6 to z~0.5, with overdense environments at high-z characterized by abundant dust-obscured star formation and stellar mass…