GWDAW-14
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Europe/Rome
Physics Department, University of Rome
Physics Department, University of Rome
Piazzale Aldo Moro 2, 00185 Rome
Description
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The Gravitational Wave Data Analysis Workshop is an annual meeting devoted to data analysis for current and future gravitational wave detectors and studies of potential gravitational wave sources. The 14th Gravitational Wave Data Analysis Workshop (GWDAW-14) will be held from January 26th to 29th, 2010, in Rome, Italy. It will take place at the Department of Physics of the University of Rome "Sapienza". Conference home page: http://www.roma1.infn.it/GWDAW14 The workshop is organized
by the INFN, Universities of Rome Sapienza and Tor Vergata and the University of Sannio.
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18:30
Welcome Party
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18:30
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Welcome Session Aula Amaldi, 1st Floor
Aula Amaldi, 1st Floor
Physics Department, University of Rome
Piazzale Aldo Moro 2, 00185 Rome-
1
Welcome of the Faculty Dean Aula Amaldi, 1st Floor
Aula Amaldi, 1st Floor
Physics Department, University of Rome
Piazzale Aldo Moro 2, 00185 Rome -
2
Welcome of the Director of the Department of Physics Aula Amaldi, 1st Floor
Aula Amaldi, 1st Floor
Physics Department, University of Rome
Piazzale Aldo Moro 2, 00185 Rome -
3
Welcome of the Director of the INFN Section of Rome Aula Amaldi, 1st Floor
Aula Amaldi, 1st Floor
Physics Department, University of Rome
Piazzale Aldo Moro 2, 00185 Rome - 4
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Detector Status Aula Amaldi, 1st Floor
Aula Amaldi, 1st Floor
Physics Department, University of Rome
Piazzale Aldo Moro 2, 00185 Rome- 5
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10:15
Coffee break Coffee TBD (Physics Department, University of Rome)
Coffee TBD
Physics Department, University of Rome
Piazzale Aldo Moro 2, 00185 Rome -
6
Space-borne Gravitational Wave Observatories Aula Amaldi, 1st Floor
Aula Amaldi, 1st Floor
Physics Department, University of Rome
Piazzale Aldo Moro 2, 00185 RomeSpeaker: Stefano Vitale (Department of Physics, University of Trento, and INFN Gruppo di Trento, Italy) -
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Pulsar timing measurements Aula Amaldi, 1st Floor
Aula Amaldi, 1st Floor
Physics Department, University of Rome
Piazzale Aldo Moro 2, 00185 RomeSpeaker: David Champion (Max-Plank-Institute für Radioastronomie) - 8
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12:35
Lunch break
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Noise analysis methods, data characterization and instrumental artifacts (Part I) Aula Amaldi, 1st Floor
Aula Amaldi, 1st Floor
Physics Department, University of Rome
Piazzale Aldo Moro 2, 00185 Rome- 10
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Noise and data characterization - Poster presentations (Part I)
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15:45
Coffee break
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Noise analysis methods, data characterization and instrumental artifacts (Part II) Aula Amaldi, 1st Floor
Aula Amaldi, 1st Floor
Physics Department, University of Rome
Piazzale Aldo Moro 2, 00185 Rome- 18
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Noise and data characterization - Poster presentations (Part II) Aula
Aula
Physics Department, University of Rome
Piazzale Aldo Moro 2, 00185 Rome-
20
Direction independent null streams in multiple co-located gravitational wave detectorsSpeaker: Birjoo Vaishnav (CGWA, University of Texas, Brownsville)
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21
Classification of Glitch Waveforms in Gravitational Wave detector characterizationSpeaker: Razib Obaid (University of Texas at Brownsville)
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26
A Neural Net for Glitch-Burst Discrimination and Glitch ClassificationSpeakers: Innocenzo Pinto (WavesGroup, INFN and LSC), Luigi Troiano (University of Sannio at Benevento), Maria Principe (University of Sannio at Benevento), Salvatore Rampone (University of Sannio at Benevento), Vincenzo Pierro (University of Sannio at Benevento)
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27
Impact of Residual non-Gaussianity after Line Removal in Interferometric Data on Detection PerformanceSpeakers: Innocenzo Pinto (University of Sannio at Benevento, LSC and INFN), Maurizio Longo (University of Salerno and LSC), Roberto Conte (University of Salerno and LSC), Vincenzo Matta (University of Salerno andLSC)
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20
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Round table: What evidence would make a convincing case for the first GW detection claim? Aula Amaldi, 1st Floor
Aula Amaldi, 1st Floor
Physics Department, University of Rome
Piazzale Aldo Moro 2, 00185 RomeConvener: Nobuyuki Kanda (Univ. of Osaka, Japan)-
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Round table: What evidence would make a convincing case for the first GW detection claim? Aula Amaldi, 1st Floor
Aula Amaldi, 1st Floor
Physics Department, University of Rome
Piazzale Aldo Moro 2, 00185 RomeSpeakers: Benoit Mours (LAPP - Annecy, France), Ettore Fiorini (MI), Francis Halzen (University of Wisconsin Madison), James Cordes (Univ. of Cornell, Ithaca, NY, USA), Neil Gehrels (NASA-GSFC), Nobuyuki Kanda (Department of Physics, Osaka City University)
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28
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Short GW transient events Aula Amaldi, 1st Floor
Aula Amaldi, 1st Floor
Physics Department, University of Rome
Piazzale Aldo Moro 2, 00185 Rome- 29
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Short GW transient events - Poster presentations Aula Amaldi, 1st Floor
Aula Amaldi, 1st Floor
Physics Department, University of Rome
Piazzale Aldo Moro 2, 00185 Rome- 32
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10:35
Coffe break
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Short GW transient events II Aula Amaldi, 1st Floor
Aula Amaldi, 1st Floor
Physics Department, University of Rome
Piazzale Aldo Moro 2, 00185 Rome- 35
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- 37
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Short GW transient events II - Poster presentations Aula Amaldi, 1st Floor
Aula Amaldi, 1st Floor
Physics Department, University of Rome
Piazzale Aldo Moro 2, 00185 Rome- 40
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41
Accretion Induced Collapse of WDs as a potential GW source for LIGOSpeaker: John Cannizzo (UMBC/CRESST/GSFC)
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One More Technique for Burst Source Position Identification: X-Wigner SpectraSpeakers: Fabio Postiglione (DIIIE, University of Salerno, INFN and LSC), Innocenzo Pinto (WavesGroup, University of Sannio, IT, INFN and LSC), Maria Principe (WavesGroup, University of Sannio, IT, INFN and LSC), Rocco Croce (WavesGroup, University of Sannio, IT), Vincenzo Pierro (WavesGroup, University of Sannio, IT, INFN and LSC)
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13:00
Lunch break Rome (Rome)
Rome
Rome
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Short GW transient events III Aula Amaldi, 1st Floor
Aula Amaldi, 1st Floor
Physics Department, University of Rome
Piazzale Aldo Moro 2, 00185 Rome- 45
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16:00
Coffee break
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Long and Short GW transients - Poster presentations Aula Amaldi, 1st Floor
Aula Amaldi, 1st Floor
Physics Department, University of Rome
Piazzale Aldo Moro 2, 00185 Rome- 52
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Long GW transient events Aula Amaldi, 1st Floor
Aula Amaldi, 1st Floor
Physics Department, University of Rome
Piazzale Aldo Moro 2, 00185 Rome- 68
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10:20
Coffe break
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73
Status of the search for untriggered gravitational wave signals from compact binary coalescences in LIGO and Virgo data during S5/VSR1Speakers: For the LSC and Virgo (many), Ian Harry (Cardiff University)
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Overview of the search for gravitational wave signals from compact binary coalescences in LIGO and Virgo data during S6/VSR2Speaker: Andrew (for LSC collaboration and Virgo collaboration) Lundgren (Syracuse University)
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13:00
Lunch break Rome (Rome)
Rome
Rome
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SOC lunch TBD
TBD
Physics Department, University of Rome
Piazzale Aldo Moro 2, 00185 RomeDiscussion on GWDAW 15/16 organization
EVO connection provided if needed -
Continuous waves and Neutron star structure Aula Amaldi, 1st Floor
Aula Amaldi, 1st Floor
Physics Department, University of Rome
Piazzale Aldo Moro 2, 00185 Rome-
79
Radio Pulsar observationsSpeaker: James Cordes (Univ. of Cornell, Ithaca, NY, USA)
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16:05
Coffe break
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79
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Continuous Waves and Neutron star structure - Poster presentations Aula Amaldi, 1st Floor
Aula Amaldi, 1st Floor
Physics Department, University of Rome
Piazzale Aldo Moro 2, 00185 Rome-
87
A directed search for continuous gravitational waves from unknown isolated neutron starsSpeaker: Berit Behnke (Albert Einstein Institut)
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20:00
Social Dinner at Casina Valadier Casina Valadier (Casina Valadier)
Casina Valadier
Casina Valadier
For more info: http://www.roma1.infn.it/GWDAW14/ -> Events
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Stochastic Gravitational Wave Background Aula Amaldi, 1st Floor
Aula Amaldi, 1st Floor
Physics Department, University of Rome
Piazzale Aldo Moro 2, 00185 Rome- 94
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95
CMB and B-modes : Planck and future perspectivesSpeaker: Paolo De Bernardis (INFN Roma, Italy)
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10:40
Coffe break
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E4 Computer Engineering Award Ceremony Aula Amaldi, 1st Floor
Aula Amaldi, 1st Floor
Physics Department, University of Rome
Piazzale Aldo Moro 2, 00185 Rome -
Concluding remarks Aula Amaldi, 1st Floor
Aula Amaldi, 1st Floor
Physics Department, University of Rome
Piazzale Aldo Moro 2, 00185 Rome-
100
Perspectives of GW data analysis
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100
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