Gravitational waves: search results, data analysis and parameter estimation: Amaldi 10 Parallel session C2

Pia Astone, Alan Weinstein, Michalis Agathos, Michał Bejger, Nelson Christensen, Thomas Dent, Philip Graff, Sergey Klimenko, Giulio Mazzolo, Atsushi Nishizawa, Florent Robinet, Patricia Schmidt, Rory Smith, John Veitch, Madeline Wade, Sofiane Aoudia, Sukanta Bose, Juan Calderon Bustillo, Priscilla Canizares, Colin CapanoJames Clark, Alberto Colla, Elena Cuoco, Carlos Da Silva Costa, Tito Dal Canton, Edgar Evangelista, Evan Goetz, Anuradha Gupta, Mark Hannam, David Keitel, Benjamin Lackey, Joshua Logue, Satyanarayan Mohapatra, Francesco Piergiovanni, Stephen Privitera, Reinhard Prix, Michael Pürrer, Virginia Re, Roberto Serafinelli, Leslie Wade, Linqing Wen, Karl Wette, John Whelan, C. Palomba, G. Prodi

Research output: Contribution to journalReview articlepeer-review

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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.

Original languageEnglish
JournalGeneral Relativity and Gravitation
Volume47
Issue number2
DOIs
Publication statusPublished - Feb 2015

Bibliographical note

Funding Information:
We wish to thank the organizers of the GR 20/Amaldi 10 conference, and our hosts at the University of Warsaw, for an excellently organized, smoothly run and extremely stimulating meeting. The authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory, the Science and Technology Facilities Council of the United Kingdom, the Max-Planck-Society, and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector, and the Italian Istituto Nazionale di Fisica Nucleare and the French Centre National de la Recherche Scientifique for the construction and operation of the Virgo detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the International Science Linkages program of the Commonwealth of Australia, the Council of Scientific and Industrial Research of India, the Istituto Nazionale di Fisica Nucleare of Italy, the Spanish Ministerio de Economía y Competitividad, the Conselleria d’Economia Hisenda i Innovació of the Govern de les Illes Balears, the Foundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific Research, the Polish Ministry of Science and Higher Education, the FOCUS Programme of Foundation for Polish Science, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, The National Aeronautics and Space Administration, OTKA of Hungary, the Lyon Institute of Origins (LIO), the National Research Foundation of Korea, Industry Canada and the Province of Ontario through the Ministry of Economic Development and Innovation, the National Science and Engineering Research Council Canada, the Carnegie Trust, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation. P. Canizares acknowledges support from a Marie Curie Intra-European Fellowship within the 7th European Community Framework Programme (PIEF-GA-2011-299190). N. Christensen acknowledges support from NSF grant PHY-1204371. T. Dal Canton acknowledges support from the IMPRS on Gravitational Wave Astronomy. P. Schmidt is a recipient of a DOC-fFORTE-fellowship of the Austrian Academy of Sciences and was also partially supported by the STFC. M Hannam acknowledges support from STFC grants ST/H008438/1 and ST/I001085/1”. J. Veitch acknowledges support from the research programme of the Foundation for Fundamental Research on Matter (FOM), which is partially supported by the Netherlands Organisation for Scientific Research (NWO). M. Wade would acknowledges support from NSF Grants No. PHY-0970074, No. PHY-1307429, and the Wisconsin Space Grant Consortium. Philip Graff acknowledges support from the NASA Postdoctoral Program at the Goddard Space Flight Center, administered by Oak Ridge Associated Universities through a contract with NASA. L. Wen acknowledges support from the Australian Research Council.

Publisher Copyright:
© 2015, The Author(s).

Keywords

  • Compact binary merger
  • Gravitational waves
  • Neutron stars
  • Parameter estimation
  • Stochastic background
  • Tests of general relativity

ASJC Scopus subject areas

  • Physics and Astronomy (miscellaneous)

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