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19912026
most citedObservation of Gravitational Waves from a Binary Black Hole Merger

14.2k citations

Showing 2012 · astro-ph.IMShow all

8 papers · 2 filters

astro-ph.IM2012★ 6 cited

The distributed Slow Control System of the XENON100 Experiment

E. Aprile, M. Alfonsi, K. Arisaka +72

The XENON100 experiment, in operation at the Laboratori Nazionali del Gran Sasso (LNGS) in Italy, was designed to search for evidence of dark matter interactions inside a volume of…

astro-ph.IM2012★ 148 cited

Antennas for the Detection of Radio Emission Pulses from Cosmic-Ray induced Air Showers at the Pierre Auger Observatory

P. Abreu, M. Aglietta, M. Ahlers +512

The Pierre Auger Observatory is exploring the potential of the radio detection technique to study extensive air showers induced by ultra-high energy cosmic rays. The Auger Engineer…

astro-ph.IM2012★ 24 cited

Prospects for observing ultra-compact binaries with space-based gravitational wave interferometers and optical telescopes

Tyson B. Littenberg, Shane L. Larson, Gijs Nelemans +1

Space-based gravitational wave interferometers are sensitive to the galactic population of ultra-compact binaries. An important subset of the ultra-compact binary population are th…

astro-ph.IM2012★ 61 cited

Using electromagnetic observations to aid gravitational-wave parameter estimation of compact binaries observed with LISA

Sweta Shah, Marc van der Sluys, Gijs Nelemans

We present a first-stage study of the effect of using knowledge from electromagnetic (EM) observations in the gravitational wave (GW) data analysis of Galactic binaries that are pr…

astro-ph.IM2012★ 62 cited

The QUIET Instrument

QUIET Collaboration, C. Bischoff, A. Brizius +52

The Q/U Imaging ExperimenT (QUIET) is designed to measure polarization in the Cosmic Microwave Background, targeting the imprint of inflationary gravitational waves at large angula…

astro-ph.IM2012★ 60 cited

Analysis of the XENON100 Dark Matter Search Data

The XENON100 Collaboration, E. Aprile, M. Alfonsi +71

The XENON100 experiment, situated in the Laboratori Nazionali del Gran Sasso, aims at the direct detection of dark matter in the form of weakly interacting massive particles (WIMPs…