activity
20052010
most citedMeasurement of the Depth of Maximum of Extensive Air Showers above 10^18 eV

548 citations · 2.3k across the 14 of their papers we have counts for

collaborators

14 papers

gr-qc2010★ 143 cited

Calibration of the LIGO Gravitational Wave Detectors in the Fifth Science Run

LIGO Scientific Collaboration, J. Abadie, B. P. Abbott +538

The Laser Interferometer Gravitational Wave Observatory (LIGO) is a network of three detectors built to detect local perturbations in the space-time metric from astrophysical sourc…

astro-ph.HE2010★ 476 cited

Measurement of the energy spectrum of cosmic rays above 10^18 eV using the Pierre Auger Observatory

The Pierre Auger Collaboration

We report a measurement of the flux of cosmic rays with unprecedented precision and statistics using the Pierre Auger Observatory. Based on fluorescence observations in coincidence…

astro-ph.HE2010★ 548 cited

Measurement of the Depth of Maximum of Extensive Air Showers above 10^18 eV

The Pierre Auger Collaboration

We describe the measurement of the depth of maximum, Xmax, of the longitudinal development of air showers induced by cosmic rays. Almost four thousand events above 10^18 eV observe…

astro-ph.IM2009★ 58 cited

Atmospheric effects on extensive air showers observed with the Surface Detector of the Pierre Auger Observatory

The Pierre Auger Collaboration

Atmospheric parameters, such as pressure (P), temperature (T) and density, affect the development of extensive air showers initiated by energetic cosmic rays. We have studied the i…

astro-ph.CO2009★ 60 cited

First LIGO search for gravitational wave bursts from cosmic (super)strings

LIGO Scientific Collaboration, B. Abbott

We report on a matched-filter search for gravitational wave bursts from cosmic string cusps using LIGO data from the fourth science run (S4) which took place in February and March…

gr-qc2009★ 48 cited

Search for gravitational wave ringdowns from perturbed black holes in LIGO S4 data

The LIGO Scientific Collaboration, B. Abbott

According to general relativity a perturbed black hole will settle to a stationary configuration by the emission of gravitational radiation. Such a perturbation will occur, for exa…