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- 2017
- Multi-Grid detector for neutron spectroscopy : Results obtained on time-of-flight spectrometer CNCS (
- 2016
- Neutron reflectometry on highly absorbing films and its application to (B4C)-B-10-based neutron detectors (
- Multi-Grid boron-10 detector for time-of-flight spectrometers in neutron scattering science (
- 2015
- Growth and oxidization stability of cubic Zr1-xGdxN solid solution thin films (
- The mu TPC method: improving the position resolution of neutron detectors based on MPGDs (
- Investigation of background in large-area neutron detectors due to alpha emission from impurities in aluminium (
- 2013
- A B-10-based neutron detector with stacked MultiWire Proportional Counters and macrostructured cathodes (
- Development of a novel macrostructured cathode for large-area neutron detectors based on the B-10-containing solid converter (
- (B4C)-B-10 Multi-Grid as an Alternative to He-3 for Large Area Neutron Detectors (
- B-10 multi-grid proportional gas counters for large area thermal neutron detectors (
- Parameter estimation for compact binary coalescence signals with the first generation gravitational-wave detector network (
- Search for gravitational waves from binary black hole inspiral, merger, and ringdown in LIGO-Virgo data from 2009-2010 (
- Einstein@Home all-sky search for periodic gravitational waves in LIGO S5 data (
- A first search for coincident gravitational waves and high energy neutrinos using LIGO, Virgo and ANTARES data from 2007 (
- 2012
- Implementation and testing of the first prompt search for gravitational wave transients with electromagnetic counterparts (
- Search for Gravitational Waves Associated with Gamma-Ray Bursts during LIGO Science Run 6 and Virgo Science Runs 2 and 3 (
- All-sky search for gravitational-wave bursts in the second joint LIGO-Virgo run (
- The characterization of Virgo data and its impact on gravitational-wave searches (
- Search for gravitational waves from intermediate mass binary black holes (
- Upper limits on a stochastic gravitational-wave background using LIGO and Virgo interferometers at 600-1000 Hz (