activity
19962017
most citedBig-Bang nucleosynthesis (Particle Data Group mini-review)

4.1k citations · 12.5k across the 32 of their papers we have counts for

collaborators

32 papers

physics.app-ph2017★ 18 cited

Quantum efficiency modeling for a thick back-illuminated astronomical CCD

D. E. Groom, S. Haque, S. E. Holland +1

The quantum efficiency and reflectivity of thick, back-illuminated CCD's being fabricated at LBNL for astronomical applications are modeled and compared with experiment. The treatm…

physics.ins-det2012★ 5 cited

Degradation of resolution in a homogeneous dual readout hadronic calorimeter

Donald E. Groom

If the response to a hadronic shower in a semi-infinite uniform calorimeter structure is relative to the electronic response, then $S/E = [\fem + (1-\fem)(h/e)]$, where is…

physics.ins-det2012★ 4 cited

Simplification of the DREAM collaboration's "Q/S method" in dual readout calorimetry analysis

Donald E. Groom

The DREAM collaboration has introduced the "Q/S Method" for obtaining the energy estimator from simultaneous Cherenkov and scintillator readouts of individual hadronic events. We s…

astro-ph.CO2010★ 1.4k cited

Spectra and Light Curves of Six Type Ia Supernovae at 0.511 < z < 1.12 and the Union2 Compilation

R. Amanullah, C. Lidman, D. Rubin +42

We report on work to increase the number of well-measured Type Ia supernovae (SNe Ia) at high redshifts. Light curves, including high signal-to-noise HST data, and spectra of six S…

astro-ph2008★ 1.6k cited

Improved Cosmological Constraints from New, Old and Combined Supernova Datasets

M. Kowalski, D. Rubin, G. Aldering +67

We present a new compilation of Type Ia supernovae (SNe Ia), a new dataset of low-redshift nearby-Hubble-flow SNe and new analysis procedures to work with these heterogeneous compi…

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…