Name: GWDAW-14
Start: 2010-01-25T09:30:00+01:00
End: 2010-01-29T18:00:00+01:00
Location: Physics Department, University of Rome

Monday, 25 January
- 18:30 → 19:30
  
  Welcome Party 1h
Tuesday, 26 January
- 08:45 → 09:30
  Welcome Session Aula Amaldi, 1st Floor
  
  Aula Amaldi, 1st Floor
  
  Physics Department, University of Rome
  
  Piazzale Aldo Moro 2, 00185 Rome
  - 08:45
    
    Welcome of the Faculty Dean 10m Aula Amaldi, 1st Floor
    
    Aula Amaldi, 1st Floor
    
    Physics Department, University of Rome
    
    Piazzale Aldo Moro 2, 00185 Rome
  - 08:55
    
    Welcome of the Director of the Department of Physics 10m Aula Amaldi, 1st Floor
    
    Aula Amaldi, 1st Floor
    
    Physics Department, University of Rome
    
    Piazzale Aldo Moro 2, 00185 Rome
  - 09:05
    
    Welcome of the Director of the INFN Section of Rome 10m Aula Amaldi, 1st Floor
    
    Aula Amaldi, 1st Floor
    
    Physics Department, University of Rome
    
    Piazzale Aldo Moro 2, 00185 Rome
  - 09:15
    
    Introduction of the E4 Computer Engineering and announcement of the E4 Computer Engineering award 10m Aula Amaldi, 1st Floor
    
    Aula Amaldi, 1st Floor
    
    Physics Department, University of Rome
    
    Piazzale Aldo Moro 2, 00185 Rome
    
    Slides
- 09:30 → 12:30
  Detector Status Aula Amaldi, 1st Floor
  
  Aula Amaldi, 1st Floor
  
  Physics Department, University of Rome
  
  Piazzale Aldo Moro 2, 00185 Rome
  - 09:30
    
    Detectors on the Earth 35m Aula Amaldi, 1st Floor
    
    Aula Amaldi, 1st Floor
    
    Physics Department, University of Rome
    
    Piazzale Aldo Moro 2, 00185 Rome
    
    Speaker: Piero Rapagnani (RM1)
    
    Slides
    
    Video
  - 10:15
    
    Coffee break 25m Coffee TBD (Physics Department, University of Rome)
    
    Coffee TBD
    
    Physics Department, University of Rome
    
    Piazzale Aldo Moro 2, 00185 Rome
  - 10:40
    
    Space-borne Gravitational Wave Observatories 35m Aula Amaldi, 1st Floor
    
    Aula Amaldi, 1st Floor
    
    Physics Department, University of Rome
    
    Piazzale Aldo Moro 2, 00185 Rome
    
    Speaker: Stefano Vitale (Department of Physics, University of Trento, and INFN Gruppo di Trento, Italy)
  - 11:20
    
    Pulsar timing measurements 30m Aula Amaldi, 1st Floor
    
    Aula Amaldi, 1st Floor
    
    Physics Department, University of Rome
    
    Piazzale Aldo Moro 2, 00185 Rome
    
    Speaker: David Champion (Max-Plank-Institute für Radioastronomie)
  - 11:55
    
    3rd generation GW observatories: Science potentialities and new technologies 30m Aula Amaldi, 1st Floor
    
    Aula Amaldi, 1st Floor
    
    Physics Department, University of Rome
    
    Piazzale Aldo Moro 2, 00185 Rome
    
    Speaker: Michele Punturo (INFN Perugia)
    
    Slides
- 12:30 → 12:35
  
  Lunch & Social Events information 5m
  
  Speaker: Fulvio Ricci (RM1)
  
  Slides
- 12:35 → 14:30
  
  Lunch break 1h 55m
- 14:30 → 15:35
  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
  - 14:30
    
    Coherent Target Detection in Heavy-Tailed Compound-Gaussian Clutter: Survey and New Results 25m
    
    Speakers: Fulvio Gini (University of Pisa), Kevin Sangston (Atlanta, GA, USA), Maria Greco (DII, University of Pisa, IT)
    
    Slides
  - 15:00
    
    Back-scattered light noise in Virgo second science run data 15m
    
    Speaker: Irene Fiori (European Gravitational Observatory)
    
    Slides
  - 15:20
    
    Robust multi-detector statistics for coherently searching for signals from coalescing compact binaries 10m
    
    Speaker: Shaon Ghosh (Graduate student)
    
    Slides
- 15:35 → 15:45
  Noise and data characterization - Poster presentations (Part I)
  - 15:35
    
    High frequency band sensitivity of large gravitational wave interferometers. 2m
    
    Speaker: Valentin Rudenko (Sternberg Astronomical Institute of MSU, Moscow)
    
    Slides
  - 15:37
    
    Deep Underground Environmental Studies for 3rd Generation Gravitational Wave Detectors 2m
    
    Speaker: Nelson Christensen (Carleton College)
    
    Poster
  - 15:39
    
    Noise Line Searches for LIGO S6 2m
    
    Speaker: Michael Coughlin (Carleton College)
    
    Poster
  - 15:41
    
    The Used Percentage Veto for LIGO S6 and Virgo VSR2 Gravitational Wave Searches 2m
    
    Speaker: Tomoki Isogai (Carleton College)
    
    Poster
  - 15:43
    
    Background estimation by time slides in a network of gravitational wave detectors 2m
    
    Speaker: Michal Was (LAL - Orsay)
    
    Poster
- 15:45 → 16:05
  
  Coffee break 20m
- 16:05 → 16:55
  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
  - 16:05
    
    Data quality in gravitational wave burst and inspiral searches in the second Virgo science run 20m
    
    Speaker: Florent Robinet (LAL IN2P3)
    
    Slides
  - 16:30
    
    LIGO S6 Detector Characterization Studies 20m
    
    Speaker: Nelson Christensen (Carleton College)
    
    Slides
- 16:55 → 17:15
  Noise and data characterization - Poster presentations (Part II) Aula
  
  Aula
  
  Physics Department, University of Rome
  
  Piazzale Aldo Moro 2, 00185 Rome
  - 16:55
    
    Direction independent null streams in multiple co-located gravitational wave detectors 2m
    
    Speaker: Birjoo Vaishnav (CGWA, University of Texas, Brownsville)
  - 16:57
    
    Classification of Glitch Waveforms in Gravitational Wave detector characterization 2m
    
    Speaker: Razib Obaid (University of Texas at Brownsville)
  - 16:59
    
    Application of support vector machines to multivariate gravitational-wave veto analysis 2m
    
    Speaker: Xiaoge Wang (Tsinghua University)
    
    Slides
  - 17:01
    
    Tools for noise characterization in Virgo 2m
    
    Speaker: Elena Cuoco (PI)
    
    Poster
    
    Slides
  - 17:03
    
    Time Delay Interferometry and Clocknoise Removal 2m
    
    Speaker: Markus Otto (AEI Hannover)
    
    Slides
  - 17:05
    
    Data Quality studies for low frequency non-stationarity present in LIGO science data 2m
    
    Speaker: Robert Stone (The University of Texas at Brownsville and Texas Southmost College)
    
    Slides
  - 17:07
    
    A Neural Net for Glitch-Burst Discrimination and Glitch Classification 2m
    
    Speakers: 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)
    
    Slides
  - 17:09
    
    Impact of Residual non-Gaussianity after Line Removal in Interferometric Data on Detection Performance 2m
    
    Speakers: 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)
    
    Slides
- 17:15 → 18:15
  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 Rome
  
  Convener: Nobuyuki Kanda (Univ. of Osaka, Japan)
  - 17:15
    Round table: What evidence would make a convincing case for the first GW detection claim? 20m Aula Amaldi, 1st Floor
    
    Aula Amaldi, 1st Floor
    
    Physics Department, University of Rome
    
    Piazzale Aldo Moro 2, 00185 Rome
    
    Speakers: 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)
    
    Slides
    
    Gehrels_roundtable.ppt
    
    GWDAW14-round-table-v1.ppt
    
    GW_Detection_Roundtable.ppt
Wednesday, 27 January
- 09:00 → 10:25
  Short GW transient events Aula Amaldi, 1st Floor
  
  Aula Amaldi, 1st Floor
  
  Physics Department, University of Rome
  
  Piazzale Aldo Moro 2, 00185 Rome
  - 09:00
    
    Long Gamma Ray Burst Observations 25m
    
    Speaker: Luigi Piro (INAF - IAS)
    
    Slides
  - 09:35
    
    Results and Challenges in Astrophysically Triggered Gravitational Wave Searches 20m
    
    Speaker: Szabolcs Marka (Columbia University)
    
    Slides
  - 10:05
    
    LIGO-Virgo Triggered Follow-up with NASA High Energy Photon Survey Missions 15m
    
    Speaker: Jordan Camp (NASA)
    
    Paper
- 10:25 → 10:35
  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
  - 10:25
    
    Proposed Multi-messenger observation plan for Sco X-1 with RXTE and gravitational wave detectors 2m
    
    Speaker: Kazuhiro Hayama (National Astronomical Observatory of Japan)
    
    Slides
  - 10:27
    
    Search for Gravitational Waves from Soft Gamma Repeaters 2m
    
    Speaker: Zsuzsa Marka (Columbia University)
    
    Poster
    
    Slides
  - 10:29
    
    Selecting Candidate GW Detections for EM Follow-up Observations 2m
    
    Speaker: Laura Nuttall (Cardiff University)
    
    Slides
- 10:35 → 10:55
  
  Coffe break 20m
- 10:55 → 12:50
  Short GW transient events II Aula Amaldi, 1st Floor
  
  Aula Amaldi, 1st Floor
  
  Physics Department, University of Rome
  
  Piazzale Aldo Moro 2, 00185 Rome
  - 10:55
    
    Probing the physics of neutron stars with gravitational waves 30m
    
    Speaker: Valeria Ferrari (RM1)
    
    Slides
  - 11:30
    
    Testing scalar-tensor theory from observations of gravitational wave bursts with a network of interferometric detectors 15m
    
    Speaker: Kazuhiro Hayama (National Astronomical Observatory of Japan)
    
    Slides
  - 11:50
    
    Estimation of the False Alarm Rate for coherent searches of gravitational waves. 15m
    
    Speaker: Giovanni Andrea Prodi (Univ. of Trento and INFN)
    
    Slides
  - 12:10
    
    From the detection to the measurement of transient gravitational wave characteristics 15m
    
    Speaker: Gabriele Vedovato (INFN Padova)
    
    Slides
  - 12:30
    
    Matching Pursuit algorithm – an outline of possible usage for gravitational waves’ data analysis 15m
    
    Speaker: Adam Zadrozny (The Andrzej Soltan Institute for Nuclear Studies (IPJ))
    
    PDF
    
    Slides
- 12:50 → 13:00
  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
  - 12:50
    
    A chirplet pipeline for the detection of gravitational wave bursts 2m
    
    Speaker: Philip Charlton (Charles Sturt University)
    
    Slides
  - 12:52
    
    Accretion Induced Collapse of WDs as a potential GW source for LIGO 2m
    
    Speaker: John Cannizzo (UMBC/CRESST/GSFC)
  - 12:54
    
    Model selection using Bayesian evidence for LISA gravitational wave burst signals 2m
    
    Speaker: Philip Graff (University of Cambridge)
    
    Poster
    
    Slides
  - 12:56
    
    Detection of GW bursts with chirplet-like template families 2m
    
    Speakers: Eric Chassande-Mottin (CNRS AstroParticule et Cosmologie), Miriam Miele (AstroParticule et Cosmologie)
    
    Poster
    
    Slides
  - 12:58
    
    One More Technique for Burst Source Position Identification: X-Wigner Spectra 2m
    
    Speakers: 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)
    
    Slides
- 13:00 → 14:30
  
  Lunch break 1h 30m Rome (Rome)
  
  Rome
  
  Rome
- 14:30 → 18:00
  Short GW transient events III Aula Amaldi, 1st Floor
  
  Aula Amaldi, 1st Floor
  
  Physics Department, University of Rome
  
  Piazzale Aldo Moro 2, 00185 Rome
  - 14:30
    
    Toward the Computation of Gravitational Wave Signatures in Three-Dimensional Multi-Physics Simulations of Core Collapse Supernovae 25m
    
    Speaker: Anthony Mezzacappa (Oak Ridge National Laboratory, Oak Ridge, TN USA)
    
    Slides
  - 15:00
    
    All-sky search for gravitational-wave bursts in the first joint LIGO-GEO-Virgo run 25m
    
    Speaker: Sergey Klimenko (University of Florida)
    
    Slides
  - 15:30
    
    Real-time Astronomy with LIGO and Virgo: Status and Prospects 12m
    
    Speaker: Erik Katsavounidis (for the LIGO and Virgo Collaborations) (Massachusetts Institute of Technology)
    
    Slides
  - 15:45
    
    Directional searches for transient gravitational waves using a coherent analysis on a selectable sky region 12m
    
    Speaker: Francesco Salemi (AEI Hannover)
    
    Slides
  - 16:00
    
    Coffee break 30m
  - 16:30
    
    IceCube: Multiwavelenght Astronomy with Neutrinos 25m
    
    Speaker: Francis Halzen (University of Wisconsin Madison)
    
    Slides
  - 17:05
    
    The ANTARES Neutrino Telescope and Multi-Messenger Astronomy 25m
    
    Speaker: Thierry Pradier (IReS & Université Louis-Pasteur)
    
    Slides
  - 17:40
    
    Joint searches of gravitational waves and high-energy neutrinos 15m
    
    Speaker: Eric Chassande-Mottin (CNRS AstroParticule et Cosmologie)
    
    Slides
- 18:00 → 18:45
  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
  - 18:00
    
    Searching for Intermediate-Duration Gravitational-Wave Transients 2m
    
    Speaker: Eric Thrane (University of Minnesota)
    
    Poster
  - 18:02
    
    Parameter estimation on gravitational waves from multiple coalescing binaries 2m
    
    Speaker: Ilya Mandel (Northwestern University)
    
    Slides
  - 18:04
    
    Compact binary waveform recovery from the cross-correlated data of two detectors by matched filtering with spinning templates 2m
    
    Speaker: László Á Gergely (University of Szeged)
    
    Poster
  - 18:06
    
    Physical Templates in the Search for Gravitational Waves from Spinning Compact-Object Binaries with LIGO 2m
    
    Speaker: Diego Fazi (Northwestern University)
    
    Poster
    
    Slides
  - 18:08
    
    Gravitational waves from highly eccentric binary black hole encounters: first steps toward detection 2m
    
    Speaker: Birjoo Vaishnav (CGWA, University of Teas at Brownsville)
    
    Slides
  - 18:10
    
    Systematic errors in the construction of hybrid waveforms for binary black holes 2m
    
    Speaker: Frank Ohme (Albert Einstein Institute)
    
    Poster
    
    Slides
  - 18:12
    
    Test on simulated data of cuInspiral, the GPU high arithmetic intensity prototype library for coalescing binaries detection. 2m
    
    Speaker: Leone Battista Bosi (PG)
    
    Slides
  - 18:14
    
    Wet and dry mergers of binary black holes in the gravitational wave spectrum 2m
    
    Speaker: Birjoo Vaishnav (Center for Gravitational Wave Astronomy, University fo Texas, Brownsville, TX, USA.)
    
    Slides
  - 18:16
    
    The Impact of Mergers on Parameter Accuracy with LISA 2m
    
    Speaker: Sean McWilliams (NASA GSFC)
    
    Poster
    
    Summary
  - 18:18
    
    Hybrid spin Taylor waveforms with ring-down attached 2m
    
    Speaker: Riccardo Sturani (Università di Urbino - INFN Firenze)
    
    Slides
  - 18:20
    
    Measuring the black hole mass function using LISA capture sources 2m
    
    Speaker: Jonathan Gair (University of Cambridge)
    
    Poster
    
    Slides
  - 18:22
    
    An improved method for estimating the efficiency of detectors 2m
    
    Speaker: Craig Robinson (Cardiff University)
    
    Poster
    
    Slides
  - 18:24
    
    Measuring the precession during the inspiral of spinning Massive Black Hole binaries with LISA 2m
    
    Speaker: Antoine PETITEAU (Albert Einstein Institute - Potsdam)
    
    Poster
    
    Slides
  - 18:26
    
    Supermassive black hole spin-flip during the inspiral 2m
    
    Speaker: László Á Gergely (University of Szeged)
    
    Poster
  - 18:28
    
    Mapping the Galaxy with LISA 2m
    
    Speaker: Jose Mckinnon (University of Texas at Brownsville)
    
    Slides
  - 18:30
    
    Model selection with Markov-Chain Monte-Carlo results applied to Gravitational Waves 2m
    
    Speaker: Vivien Raymond (Dearborn Observatory, Northwestern University, Evanston, IL, USA)
    
    Poster
Thursday, 28 January
- 08:45 → 13:00
  Long GW transient events Aula Amaldi, 1st Floor
  
  Aula Amaldi, 1st Floor
  
  Physics Department, University of Rome
  
  Piazzale Aldo Moro 2, 00185 Rome
  - 08:45
    
    Short Gamma-Ray Bursts and Related Science 30m
    
    Speaker: Shiho Kobayashi (Liverpool John Moores University)
    
    Slides
  - 09:20
    
    What Are We Learning On Coalescing Binaries From Gamma Ray Bursts 10m
    
    Speaker: L. Juracy Rangel-Lemos (ICRA & Dip. di Fisica, Universita' di Roma "Sapienza")
    
    Slides
  - 09:35
    
    Search for gravitational waves associated with short gamma-ray bursts in LIGO's fifth and Virgo's first science run 10m
    
    Speaker: Alexander Dietz (LAPP Annecy-le-vieux)
    
    Slides
  - 09:50
    
    Very Low Latency Search for Low Mass Compact Binary Coalescences in the LIGO S6 and Virgo VSR2 Data 10m
    
    Speaker: Damir Buskulic (Université de Savoie / LAPP / IN2P3)
    
    Slides
  - 10:05
    
    Efficiently Enclosing the Signal Manifold: SVD Approximations of Compact Binary Coalesence Gravitational-Wave Signals 10m
    
    Speaker: Drew Keppel (LIGO Lab and Theoretical Astrophysics, California Institute of Techonology)
    
    Slides
  - 10:20
    
    Coffe break 20m
  - 10:40
    
    Status of the search for untriggered gravitational wave signals from compact binary coalescences in LIGO and Virgo data during S5/VSR1 15m
    
    Speakers: For the LSC and Virgo (many), Ian Harry (Cardiff University)
  - 10:55
    
    Overview of the search for gravitational wave signals from compact binary coalescences in LIGO and Virgo data during S6/VSR2 15m
    
    Speaker: Andrew (for LSC collaboration and Virgo collaboration) Lundgren (Syracuse University)
  - 11:15
    
    General Relativistic Simulations of Compact Binaries 25m
    
    Speaker: Bruno Giacomazzo (University of Maryland, USA)
    
    Slides
  - 11:45
    
    The interface between numerical relativity and gravitational wave data analysis 20m
    
    Speaker: Krishnan Badri (Albert Einstein Institute)
    
    Slides
  - 12:10
    
    The Mock LISA Data Challenges: Challenge 4 25m
    
    Speaker: Edward Porter (APC Laboratory)
    
    Slides
  - 12:40
    
    Measuring Massive Black Hole Binaries with LISA 15m
    
    Speaker: Ryan Lang (NASA Goddard Space Flight Center)
    
    Slides
- 13:00 → 14:30
  
  Lunch break 1h 30m Rome (Rome)
  
  Rome
  
  Rome
- 13:00 → 14:30
  
  SOC lunch TBD
  
  TBD
  
  Physics Department, University of Rome
  
  Piazzale Aldo Moro 2, 00185 Rome
  
  Discussion on GWDAW 15/16 organization
  EVO connection provided if needed
- 14:30 → 18:10
  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
  - 14:30
    
    Radio Pulsar observations 35m
    
    Speaker: James Cordes (Univ. of Cornell, Ithaca, NY, USA)
  - 15:10
    
    Continuous gravitational waves from neutron stars 25m
    
    Speaker: Benjamin Owen (The Pennsylvania State University)
    
    Slides
  - 15:40
    
    A method for detection of known sources of continuous gravitational wave signals in non-stationary data. 20m
    
    Speaker: Pia Astone (RM1)
    
    Slides
  - 16:05
    
    Coffe break 20m
  - 16:25
    
    Sequential Tests: a Tool for GW Detection 25m
    
    Speaker: Vincenzo Matta (University of Salerno)
    
    Slides
  - 16:55
    
    Search for gravitational waves from known pulsars using the F and G statistics 25m
    
    Speaker: Andrzej Krolak (Institute of Mathematics, Polish academy of Sciences)
    
    Paper
  - 17:25
    
    Discrete Resampling for Doppler and Spin Down correction in CW semitargeted searches 10m
    
    Speaker: Stefano Braccini (INFN - Pisa)
    
    Slides
  - 17:40
    
    Optimizing sensitivity of searches for continuous gravitational waves at fixed computing cost 10m
    
    Speaker: Miroslav Shaltev (AEI - Hannover)
    
    Slides
  - 17:55
    
    Detecting signatures of the cosmic thermal history through pulsar observations 10m
    
    Speaker: Massimiliano Lattanzi (ICRA & Dip. di Fisica, Universita' di Roma "Sapienza")
    
    Slides
- 18:10 → 18:30
  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
  - 18:10
    
    A directed search for continuous gravitational waves from unknown isolated neutron stars 2m
    
    Speaker: Berit Behnke (Albert Einstein Institut)
  - 18:12
    
    Coherent metric for continuous gravitational waves from isolated systems 2m
    
    Speaker: Reinhard Prix (Albert-Einstein-Institut Hannover)
    
    Slides
  - 18:14
    
    A Bayesian strategy for the generation of pulsar time-of-arrival measurements 2m
    
    Speaker: Chris Messenger (AEI Hannover)
    
    Poster
  - 18:16
    
    Parameter-space metric of semicoherent searches for continuous gravitational waves 2m
    
    Speaker: Holger Pletsch (Albert-Einstein-Institut Hannover)
    
    Slides
  - 18:18
    
    Search for continuous gravitational waves from PSR J2144-3933 using a magnetically-levitated torsion antenna 2m
    
    Speaker: Koji Ishidoshiro (Department of Physics, Graduate School of Science, University of Tokyo)
    
    Slides
  - 18:20
    
    An all-sky search for continuous gravitational waves from neutron stars in binary systems using the TwoSpect algorithm 2m
    
    Speaker: Evan Goetz (University of Michigan)
    
    Poster
    
    Slides
  - 18:22
    
    Polynomial search for continuous gravitational waves from neutron stars in binary systems 2m
    
    Speaker: henk J. bulten (Vrije Universiteit Amsterdam/Nikhef)
    
    Slides
- 20:00 → 22:00
  
  Social Dinner at Casina Valadier 2h Casina Valadier (Casina Valadier)
  
  Casina Valadier
  
  Casina Valadier
  
  For more info: http://www.roma1.infn.it/GWDAW14/ -> Events
Friday, 29 January
- 09:00 → 12:20
  Stochastic Gravitational Wave Background Aula Amaldi, 1st Floor
  
  Aula Amaldi, 1st Floor
  
  Physics Department, University of Rome
  
  Piazzale Aldo Moro 2, 00185 Rome
  - 09:00
    
    Cosmological stochastic backgrounds 30m
    
    Speaker: Michele Maggiore (University of Geneva, Switzerland)
    
    Slides
  - 09:35
    
    CMB and B-modes : Planck and future perspectives 30m
    
    Speaker: Paolo De Bernardis (INFN Roma, Italy)
  - 10:10
    
    Measuring the Stochastic Gravitational-Wave Background with LIGO-Virgo 25m
    
    Speaker: Eric Thrane (University of Minnesota)
    
    Slides
  - 10:40
    
    Coffe break 30m
  - 11:10
    
    Stochastic backgrounds of gravitational waves from extragalactic sources 25m
    
    Speaker: Raffaella Schneider (INAF/Osservatorio Astrofisico di Arcetri)
    
    Slides
  - 11:40
    
    Parameter estimation of massive black hole binaries with pulsar timing arrays. 15m
    
    Speaker: Alberto Sesana (Albert Einstein Institute, Golm)
    
    Slides
  - 12:00
    
    Cosmology with 300,000 Standard Sirens 15m
    
    Speaker: Curt Cutler (Jet Propulsion Lab)
    
    Slides
- 12:20 → 12:30
  
  E4 Computer Engineering Award Ceremony Aula Amaldi, 1st Floor
  
  Aula Amaldi, 1st Floor
  
  Physics Department, University of Rome
  
  Piazzale Aldo Moro 2, 00185 Rome
- 12:30 → 13:00
  Concluding remarks Aula Amaldi, 1st Floor
  
  Aula Amaldi, 1st Floor
  
  Physics Department, University of Rome
  
  Piazzale Aldo Moro 2, 00185 Rome
  - 12:30
    
    Perspectives of GW data analysis 30m

GWDAW-14

Physics Department, University of Rome

Aula Amaldi, 1st Floor

Physics Department, University of Rome

Aula Amaldi, 1st Floor

Physics Department, University of Rome

Aula Amaldi, 1st Floor

Physics Department, University of Rome

Aula Amaldi, 1st Floor

Physics Department, University of Rome

Aula Amaldi, 1st Floor

Physics Department, University of Rome

Aula Amaldi, 1st Floor

Physics Department, University of Rome

Aula Amaldi, 1st Floor

Physics Department, University of Rome

Coffee TBD

Physics Department, University of Rome

Aula Amaldi, 1st Floor

Physics Department, University of Rome

Aula Amaldi, 1st Floor

Physics Department, University of Rome

Aula Amaldi, 1st Floor

Physics Department, University of Rome

Aula Amaldi, 1st Floor

Physics Department, University of Rome

Aula Amaldi, 1st Floor

Physics Department, University of Rome

Aula

Physics Department, University of Rome

Aula Amaldi, 1st Floor

Physics Department, University of Rome

Aula Amaldi, 1st Floor

Physics Department, University of Rome

Aula Amaldi, 1st Floor

Physics Department, University of Rome

Aula Amaldi, 1st Floor

Physics Department, University of Rome

Aula Amaldi, 1st Floor

Physics Department, University of Rome

Aula Amaldi, 1st Floor

Physics Department, University of Rome

Rome

Rome

Aula Amaldi, 1st Floor

Physics Department, University of Rome

Aula Amaldi, 1st Floor

Physics Department, University of Rome

Aula Amaldi, 1st Floor

Physics Department, University of Rome

Rome

Rome

TBD

Physics Department, University of Rome

Aula Amaldi, 1st Floor

Physics Department, University of Rome

Aula Amaldi, 1st Floor

Physics Department, University of Rome

Casina Valadier

Casina Valadier

Aula Amaldi, 1st Floor

Physics Department, University of Rome

Aula Amaldi, 1st Floor

Physics Department, University of Rome

Aula Amaldi, 1st Floor

Physics Department, University of Rome