@Article{AstoneWABCDGKMNRSSVWABBCCCCCCCEGGHKLLMPPPPRSWWWWPP:2015:SeReDa,
author = "Astone, Pia and Weinstein, Alan and Agathos, Michalis and Bejger,
Michal and Christensen, Nelson and Dent, Thomas and Graff, Philip
and Klimenko, Sergey and Mazzolo, Giulio and Nishizawa, Atsushi
and Robinet, Florent and Schmidit, Patricia and Smith, Rory and
Veitch, John and Wade, Madeline and Aoudia, Sofiane and Bose,
Sukanta and Bustillo, Juan Calderon and Canizares, Priscilla and
Capano, Colin and Clark, James and Colla, Alberto and Cuoco, Elena
and Costa, Carlos da Silva and Canton, Tito dal and Evangelista,
Edgard de Freitas Diniz and Goetz, Evan and Gupta, Anuradha and
Hannam, Mark and Keitel, David and Lackey, Benjamin and Logue,
Joshua and Mohapatra, Satyanarayan and Piergiovanni, Francesco and
Privitera, Stephen and Prix, Reinhard and Purrer, Michael and Re,
Virginia and Serafinelli, Roberto and Wade, Leslie and Wen,
Linqing and Wette, Karl and Whelan, John and Palomba, C. and
Prodi, G.",
affiliation = "INFN and 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 and Nikhef and {N.
Copernicus Astronomical Center} and {Carleton College Northfield}
and Albert-Einstein-Institut and {NASA Goddard Space Flight
Center} and {University of Florida} and Albert-Einstein-Institut
and {Kyoto University} and {Universite Paris} and {Cardiff
University} and {University of Birmingham} and Nikhef and
{University of Wisconsin} and Albert-Einstein-Institut and
{Washington State University} and {University of the Balearic} and
{Madingley Road Cambridge} and {University of Maryland} and
{University of Massachusetts} and {University of Rome “Sapienza”}
and {European Gravitational Observatory (EGO)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and
Albert-Einstein-Institut and {Instituto Nacional de Pesquisas
Espaciais (INPE)} and Albert-Einstein-Institut and {Tata Institute
for Fundamental Research} and {Cardiff University School of
Physics and Astronomy} and Albert-Einstein-Institut and {Princeton
University} and {University of Glasgow} and {Syracuse University}
and INFN and {California Institute of Technology} and
Albert-Einstein-Institut and {Cardiff University} and
{Universit{\'a} di Roma Tor Vergata} and {University of Rome
“Sapienza”} and {University of Wisconsin} and {University of
Western Australia} and Albert-Einstein-Institut and {Rochester
Institute of Technology} and INFN and INFN",
title = "Gravitational waves: search results, data analysis and parameter
estimation: Amaldi 10 Parallel session C2",
journal = "General Relativity and Gravitation",
year = "2015",
volume = "47",
number = "2",
keywords = "Compact binary merger, Gravitational waves, Neutron stars,
Parameter estimation, Stochastic background, Tests of general
relativity.",
abstract = "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.",
doi = "10.1007/s10714-014-1796-x",
url = "http://dx.doi.org/10.1007/s10714-014-1796-x",
issn = "0001-7701",
language = "en",
targetfile = "Astone_Gravitational.pdf",
urlaccessdate = "27 abr. 2024"
}