activity
20102018
most citedObservation of Coherent Elastic Neutrino-Nucleus Scattering

775 citations · 1.8k across the 18 of their papers we have counts for

collaborators

18 papers

nucl-ex2018★ 60 cited

COHERENT Collaboration data release from the first observation of coherent elastic neutrino-nucleus scattering

COHERENT Collaboration, D. Akimov, J. B. Albert +91

This release includes data and information necessary to perform independent analyses of the COHERENT result presented in Akimov et al., arXiv:1708.01294 [nucl-ex]. Data is shared i…

physics.ins-det2018★ 28 cited

COHERENT 2018 at the Spallation Neutron Source

D. Akimov, J. B. Albert, P. An +76

The primary goal of the COHERENT collaboration is to measure and study coherent elastic neutrino-nucleus scattering (CEvNS) using the high-power, few-tens-of-MeV, pulsed source of…

nucl-ex2017★ 184 cited

Search for Zero-Neutrino Double Beta Decay in 76Ge with the Majorana Demonstrator

C. E. Aalseth, N. Abgrall, E. Aguayo +126

The \MJ\ Collaboration is operating an array of high purity Ge detectors to search for neutrinoless double-beta decay in Ge. The \MJ\ \DEM\ comprises 44.1~kg of Ge detectors…

nucl-ex2017★ 775 cited

Observation of Coherent Elastic Neutrino-Nucleus Scattering

D. Akimov, J. B. Albert, P. An +78

The coherent elastic scattering of neutrinos off nuclei has eluded detection for four decades, even though its predicted cross-section is the largest by far of all low-energy neutr…

physics.ins-det2015★ 26 cited

The COHERENT Experiment at the Spallation Neutron Source

COHERENT Collaboration, D. Akimov, P. An +64

The COHERENT collaboration's primary objective is to measure coherent elastic neutrino-nucleus scattering (CEvNS) using the unique, high-quality source of tens-of-MeV neutrinos pro…

physics.ins-det2014★ 88 cited

Coherent neutrino-nucleus scattering detection with a CsI[Na] scintillator at the SNS spallation source

J. I. Collar, N. E. Fields, E. Fuller +5

We study the possibility of using CsI[Na] scintillators as an advantageous target for the detection of coherent elastic neutrino-nucleus scattering (CENNS), using the neutrino emis…

physics.ins-det2014

Update on the MiniCLEAN Dark Matter Experiment

K. Rielage, M. Akashi-Ronquest, M. Bodmer +43

The direct search for dark matter is entering a period of increased sensitivity to the hypothetical Weakly Interacting Massive Particle (WIMP). One such technology that is being ex…

physics.ins-det2013★ 1 cited

The MAJORANA DEMONSTRATOR: A Search for Neutrinoless Double-beta Decay of Germanium-76

MAJORANA Collaboration, S. R. Elliott, N. Abgrall +80

The {\sc Majorana} collaboration is searching for neutrinoless double beta decay using Ge, which has been shown to have a number of advantages in terms of sensitivities and…

nucl-ex2012★ 1 cited

The MAJORANA DEMONSTRATOR: Progress towards showing the feasibility of a tonne-scale 76Ge neutrinoless double-beta decay experiment

P. Finnerty, E. Aguayo, M. Amman +80

The MAJORANA DEMONSTRATOR will search for the neutrinoless double-beta decay of the 76Ge isotope with a mixed array of enriched and natural germanium detectors. The observation of…

physics.ins-det2012★ 2 cited

Characteristics of Signals Originating Near the Lithium-Diffused N+ Contact of High Purity Germanium P-Type Point Contact Detectors

The MAJORANA Collaboration, E. Aguayo, M. Amman +83

A study of signals originating near the lithium-diffused n+ contact of p-type point contact (PPC) high purity germanium detectors (HPGe) is presented. The transition region between…

nucl-ex2011★ 17 cited

The Majorana experiment: an ultra-low background search for neutrinoless double-beta decay

D. G. Phillips, E. Aguayo, F. T. Avignone +86

The observation of neutrinoless double-beta decay would resolve the Majorana nature of the neutrino and could provide information on the absolute scale of the neutrino mass. The in…

nucl-ex2011★ 10 cited

The Majorana Demonstrator

E. Aguayo, J. E. Fast, E. W. Hoppe +90

A brief review of the history and neutrino physics of double beta decay is given. A description of the MAJORANA DEMONSTRATOR research and development program including background r…

nucl-ex2011★ 21 cited

The MAJORANA DEMONSTRATOR: A Search for Neutrinoless Double-beta Decay of Germanium-76

MAJORANA Collaboration, A. G. Schubert, E. Aguayo +90

The observation of neutrinoless double-beta decay would determine whether the neutrino is a Majorana particle and provide information on the absolute scale of neutrino mass. The MA…

astro-ph.EP2011★ 69 cited

HAT-P-27b: A hot Jupiter transiting a G star on a 3 day orbit

Bence Béky, Gáspár Á. Bakos, Joel Hartman +21

We report the discovery of HAT-P-27b, an exoplanet transiting the moderately bright G8 dwarf star GSC 0333-00351 (V=12.214). The orbital period is 3.039586 +/- 0.000012 d, the refe…

astro-ph.EP2010★ 81 cited

HAT-P-17b,c: A Transiting, Eccentric, Hot Saturn and a Long-period, Cold Jupiter

A. W. Howard, G. Á. Bakos, J. Hartman +18

We report the discovery of HAT-P-17b,c, a multi-planet system with an inner transiting planet in a short-period, eccentric orbit and an outer planet in a 4.8 yr, nearly circular or…

astro-ph.EP2010★ 44 cited

HAT-P-25b: a Hot-Jupiter Transiting a Moderately Faint G Star

S. N. Quinn, G. Á. Bakos, J. Hartman +19

We report the discovery of HAT-P-25b, a transiting extrasolar planet orbiting the V = 13.19 G5 dwarf star GSC 1788-01237, with a period P = 3.652836 +/- 0.000019 days, transit epoc…

astro-ph.EP2010★ 38 cited

HAT-P-24b: An inflated hot-Jupiter on a 3.36d period transiting a hot, metal-poor star

D. M. Kipping, G. A. Bakos, J. Hartman +17

We report the discovery of HAT-P-24b, a transiting extrasolar planet orbiting the moderately bright V=11.818 F8 dwarf star GSC 0774-01441, with a period P = 3.3552464 +/- 0.0000071…

astro-ph.EP2010★ 370 cited

HAT-P-16b: A 4 Mj Planet Transiting A Bright Star On An Eccentric Orbit

L. A. Buchhave, G. A. Bakos, J. D. Hartman +19

We report the discovery of HAT-P-16b, a transiting extrasolar planet orbiting the V = 10.8 mag F8 dwarf GSC 2792-01700, with a period P = 2.775960 +- 0.000003 d, transit epoch Tc =…