TY - JOUR
T1 - Gravitational waves
T2 - search results, data analysis and parameter estimation: Amaldi 10 Parallel session C2
AU - Astone, Pia
AU - Weinstein, Alan
AU - Agathos, Michalis
AU - Bejger, Michał
AU - Christensen, Nelson
AU - Dent, Thomas
AU - Graff, Philip
AU - Klimenko, Sergey
AU - Mazzolo, Giulio
AU - Nishizawa, Atsushi
AU - Robinet, Florent
AU - Schmidt, Patricia
AU - Smith, Rory
AU - Veitch, John
AU - Wade, Madeline
AU - Aoudia, Sofiane
AU - Bose, Sukanta
AU - Calderon Bustillo, Juan
AU - Canizares, Priscilla
AU - Capano, Colin
AU - Clark, James
AU - Colla, Alberto
AU - Cuoco, Elena
AU - Da Silva Costa, Carlos
AU - Dal Canton, Tito
AU - Evangelista, Edgar
AU - Goetz, Evan
AU - Gupta, Anuradha
AU - Hannam, Mark
AU - Keitel, David
AU - Lackey, Benjamin
AU - Logue, Joshua
AU - Mohapatra, Satyanarayan
AU - Piergiovanni, Francesco
AU - Privitera, Stephen
AU - Prix, Reinhard
AU - Pürrer, Michael
AU - Re, Virginia
AU - Serafinelli, Roberto
AU - Wade, Leslie
AU - Wen, Linqing
AU - Wette, Karl
AU - Whelan, John
AU - Palomba, C.
AU - Prodi, G.
N1 - Publisher Copyright:
© 2015, The Author(s).
PY - 2015/2
Y1 - 2015/2
N2 - The Amaldi 10 Parallel Session C2 on gravitational wave (GW) search results, data analysis and parameter estimation included three lively sessions of lectures by 13 presenters, and 34 posters. The talks and posters covered a huge range of material, including results and analysis techniques for ground-based GW detectors, targeting anticipated signals from different astrophysical sources: compact binary inspiral, merger and ringdown; GW bursts from intermediate mass binary black hole mergers, cosmic string cusps, core-collapse supernovae, and other unmodeled sources; continuous waves from spinning neutron stars; and a stochastic GW background. There was considerable emphasis on Bayesian techniques for estimating the parameters of coalescing compact binary systems from the gravitational waveforms extracted from the data from the advanced detector network. This included methods to distinguish deviations of the signals from what is expected in the context of General Relativity.
AB - The Amaldi 10 Parallel Session C2 on gravitational wave (GW) search results, data analysis and parameter estimation included three lively sessions of lectures by 13 presenters, and 34 posters. The talks and posters covered a huge range of material, including results and analysis techniques for ground-based GW detectors, targeting anticipated signals from different astrophysical sources: compact binary inspiral, merger and ringdown; GW bursts from intermediate mass binary black hole mergers, cosmic string cusps, core-collapse supernovae, and other unmodeled sources; continuous waves from spinning neutron stars; and a stochastic GW background. There was considerable emphasis on Bayesian techniques for estimating the parameters of coalescing compact binary systems from the gravitational waveforms extracted from the data from the advanced detector network. This included methods to distinguish deviations of the signals from what is expected in the context of General Relativity.
KW - Compact binary merger
KW - Gravitational waves
KW - Neutron stars
KW - Parameter estimation
KW - Stochastic background
KW - Tests of general relativity
UR - http://www.scopus.com/inward/record.url?scp=84921901513&partnerID=8YFLogxK
U2 - 10.1007/s10714-014-1796-x
DO - 10.1007/s10714-014-1796-x
M3 - Review article
AN - SCOPUS:84921901513
SN - 0001-7701
VL - 47
JO - General Relativity and Gravitation
JF - General Relativity and Gravitation
IS - 2
ER -