activity
20022023
most citedThe Hubble Diagram of Type Ia Supernovae as a Function of Host Galaxy Morphology

139 citations · 733 across the 13 of their papers we have counts for

collaborators

13 papers

hep-ex2023★ 6 cited

First measurement of discrimination between helium and electron recoils in liquid xenon for low-mass dark matter searches

S. J. Haselschwardt, R. Gibbons, H. Chen +5

We report the first measurement of discrimination between low-energy helium recoils and electron recoils in liquid xenon. This result is relevant to proposed low-mass dark matter s…

hep-ex2023★ 56 cited

A search for new physics in low-energy electron recoils from the first LZ exposure

The LZ Collaboration, J. Aalbers, D. S. Akerib +200

The LUX-ZEPLIN (LZ) experiment is a dark matter detector centered on a dual-phase xenon time projection chamber. We report searches for new physics appearing through few-keV-scale…

physics.ins-det2020

Understanding the Enhancement of Scintillation Light in Xenon-Doped Liquid Argon

D. E. Fields, and R. Gibbons M. Gold, N. McFadden +2

Measuring the scintillation light in noble gases is an important detection technique in particle physics. Numerous rare event searches like neutrino beam experiments, neutrino-less…

physics.ins-det2020★ 6 cited

Large-Scale, Precision Xenon Doping of Liquid Argon

N. McFadden, S. R. Elliott, M. Gold +4

The detection of scintillation light from liquid argon is an experimental technique key to a number of current and future nuclear/particle physics experiments, such as neutrino phy…

astro-ph2007★ 71 cited

A New Determination of the High Redshift Type Ia Supernova Rates with the Hubble Space Telescope Advanced Camera for Surveys

N. Kuznetsova, K. Barbary, B. Connolly +27

We present a new measurement of the volumetric rate of Type Ia supernova up to a redshift of 1.7, using the Hubble Space Telescope (HST) GOODS data combined with an additional HST…

astro-ph2007★ 64 cited

Quantitative comparison between Type Ia supernova spectra at low and high redshifts: A case study

G. Garavini, G. Folatelli, S. Nobili +44

We develop a method to measure the strength of the absorption features in Type Ia supernova (SN Ia) spectra and use it to make a quantitative comparison between the spectra of Type…