March 17, 2008LSC-Virgo meeting1/12 Virgo Status B. Mours.

Slides:



Advertisements
Similar presentations
Status of the Virgo Commissioning G.Losurdo – INFN Firenze/Urbino for the Virgo Collaboration.
Advertisements

September 21, 2005Virgo Status – ESF Workshop1 Status of Virgo B. Mours.
Cascina, January 25th, Coupling of the IMC length noise into the recombined ITF output Raffaele Flaminio EGO and CNRS/IN2P3 Summary - Recombined.
Andrea Paoli AdV 1 st Project Review Cascina, November 3 rd, 2008 IME – infrastructure modifications for environmental noise reduction.
VIRGO: WHERE WE COME FROM WHERE WE ARE GOING GIOVANNI LOSURDO - INFN Firenze Advanced Virgo Project Leader for the Virgo Collaboration (and the LIGO Scientific.
1 Virgo commissioning status M.Barsuglia LAL Orsay.
Virgo commissioning update - VSR1 first month summary E. Tournefier WG1 meeting, Cascina June 20 th,2007.
F. Frasconi I.N.F.N. Pisa for the Virgo Collaboration TAUP2007 Sendai, September 11-15, 2007 VIRGO EXPERIMENT VIRGO: a large interferometer for Gravitational.
1 Virgo Commissioning progress and plans ILIAS, Jan 23 rd 2007 Matteo Barsuglia on behalf of the Commissioning Team.
VSR1 summary - post VSR1 Commissioning plans E. Tournefier (LAPP-CNRS) LSC-Virgo meeting Oct 22 nd, 2007.
rd ILIAS-GW annual general meeting 1 VIRGO Commissioning progress J. Marque (EGO)
COMMISSIONING PROGRESS G.LOSURDO – INFN Firenze for the Virgo Collaboration.
Present Superatttenuator performance vs. AdV & ET Requirements S.Braccini for Virgo Suspension group.
1 Virgo commissioning since the end of VSR1 E. Tournefier for the commissioning team ILIAS WG1, Cascina March 5 th,2008.
Virgo Control Noise Reduction
GWADW 2010 in Kyoto, May 19, Development for Observation and Reduction of Radiation Pressure Noise T. Mori, S. Ballmer, K. Agatsuma, S. Sakata,
Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut) Institut für Atom- und Molekülphysik Detector Characterization of GEO 600 during.
Status of Virgo Gabriele Vajente INFN Pisa and Scuola Normale Superiore di Pisa On behalf of the Virgo Collaboration 11 th Gravitational Wave Data Analysis.
Interferometric detector for GW: status and perspectives Giovanni Losurdo INFN Firenze-Urbino
Plans for Advanced Virgo
Optical Configuration Advanced Virgo Review Andreas Freise for the OSD subsystem.
Francesco Fidecaro STAC meeting, Cascina, May 28, 2009 Virgo status report.
The status of Giovanni Losurdo - INFN Firenze-Urbino on behalf of the Virgo Collaboration Workshop on GW detection– Gingin, Oct. 4-7, 2005.
Virgo Commissioning update Gabriele Vajente for the Virgo Collaboration LSC/VIRGO Meeting – MIT 2007, July LIGO-G Z.
Advanced VIRGO WG1: Status VIRGO, Cascina Andreas Freise University of Birmingham.
Environmental noise studies at VIRGO Environmental contributions to Virgo readout noise (C-runs) many sources identified through coherency analyses with.
Status of Virgo A. Viceré INFN-Firenze – Università di Urbino.
1 Virgo commissioning: Next steps December 12 st 2005 Hannover, ILIAS-GWA WG1 Matteo Barsuglia, LAL/CNRS.
1 Virgo Commissioning progress ILIAS, Nov 13 th 2006 Matteo Barsuglia on behalf of the Commissioning Team.
Advanced Virgo Optical Configuration ILIAS-GW, Tübingen Andreas Freise - Conceptual Design -
January 12, 2006ILIAS-WG3 Frascati1 Virgo+ & Advanced Virgo B. Mours With material from G. Losurdo, M. Punturo, A. Viceré and others.
Paolo La Penna Injection optics for Advanced VirgoLSC/VIRGO joint meeting, Cascina, 25/05/ Advanced VIRGO Input optics LIGO-G Z.
1 The Virgo noise budget Romain Gouaty For the Virgo collaboration GWADW 2006, Isola d’Elba.
Loïc Rolland LSC-Virgo, Orsay- June 11th Virgo ‘timing’ calibration Loïc Rolland Note: Timing calibration during VSR1 in the Virgo codifier (VIR-028A-08,
Paolo La Penna ILIAS N5-WP1 meeting Noise analysis in Virgo Cascina, 7-8 July 2004 Analysis of noise in VIRGO.
Status of VIRGO Lisa Barsotti - University and INFN Pisa – on behalf of the VIRGO collaboration ANNECY - December 15 th, 2004  Status of the Commissioning.
Nov 3, 2008 Detection System for AdV 1/8 Detection (DET) Subsystem for AdV  Main tasks and requirements for the subsystem  DC readout  Design for: the.
Advanced Virgo Giovanni Losurdo Advanced Virgo Coordinator for the Virgo Collaboration.
1 LESSONS FROM VIRGO+ May 17th 2010 E. Calloni for the Virgo collaboration.
Virgo+ Commissioning Status. Main upgrades and activities Laser system: from 10  25 watt output power at the IMC TCS: ring + Central Heating Electronics:
The status of VIRGO Edwige Tournefier (LAPP-Annecy ) for the VIRGO Collaboration HEP2005, 21st- 27th July 2005 The VIRGO experiment and detection of.
1 Virgo Commissioning Status WG1 meeting Potsdam, 21 st July 2006.
Paolo La Penna ILIAS N5-WP1 meeting Commissioning Progress Hannover, July 2004 VIRGO commissioning progress report.
International Gravitational Wave Network 11/9/2008 Building an Stefan Ballmer, for the LIGO / VIRGO Scientific Collaboration LIGO G
LIGO-G M LIGO Status Gary Sanders GWIC Meeting Perth July 2001.
Initial and Advanced LIGO Status Gregory Harry LIGO/MIT March 24, 2006 March 24, th Eastern Gravity Meeting G R.
Status of Virgo GWDAW12 Status of Virgo GWDAW Dec Leone B. Bosi INFN and University of Perugia (Italy) On behalf of the Virgo Collaboration.
1 Locking in Virgo Matteo Barsuglia ILIAS, Cascina, July 7 th 2004.
Status of Virgo a short update Michele Punturo. A bit of History July 29 – August –C6 run Duty cycle: Locking 89%, Science Mode 86% September.
Caltech, February 12th1 Virgo central interferometer: commissioning and engineering runs Matteo Barsuglia Laboratoire de l’Accelerateur Lineaire, Orsay.
Monica VarvellaIEEE - GW Workshop Roma, October 21, M.Varvella Virgo LAL Orsay / LIGO CalTech Time-domain model for AdvLIGO Interferometer Gravitational.
Advanced Towards Advanced Virgo Giovanni Losurdo – INFN Firenze Advanced Virgo Coordinator on behalf of the Virgo Collaboration.
SAT Plans for System R&D Signal Recycling Construction and A&I Short Suspension Upgrade Roberto Passaquieti Università di Pisa and INFN-Pisa AdV Review.
Sensitivity of Virgo E. Tournefier (LAPP-CNRS) LSC-Virgo week May 23 rd,2007 LIGO-G Z.
Advanced Advanced Virgo BASELINE DESIGN advanced Giovanni Losurdo – INFN Firenze Advanced Virgo Coordinator for the Virgo Collaboration.
The VIRGO detection system
Advanced Virgo advanced Giovanni Losurdo – INFN Firenze Advanced Virgo Coordinator for the Virgo Collaboration Requires the font “calibri”. DOWNLOAD.
GEO Status and Prospects Harald Lück ILIAS / ETmeeting Cascina November 2008.
MG 11 - Berlin Virgo status Marie-Anne Bizouard (LAL-Orsay) on behalf of the Virgo Collaboration.
Edwige Tournefier for the Virgo Collaboration The status of Virgo.
THE NEXT GENERATIONS OF GRAVITATIONAL WAVE DETECTORS (*) Giovanni Losurdo INFN Firenze – Virgo collaboration (*) GROUND BASED, INTERFEROMETRIC.
VIRGO Second part. Advanced VIRGO and the INFN VIRGO activity in 2010 Fulvio Ricci
Reaching the Advanced LIGO Detector Design Sensitivity
THE NEXT GENERATION OF GRAVITATIONAL WAVE DETECTORS
Evolution of the Virgo detector: The Virgo+ plans
Status of Virgo GWDAW Dec 13-16
Virgo Update B. Mours LIGO-G Z August 15, 2006 LSC meeting.
Virgo Update – LSC meeting
3rd generation ITF sensitivity curve
Status at the Prague meeting
Presentation transcript:

March 17, 2008LSC-Virgo meeting1/12 Virgo Status B. Mours

March 17, 2008LSC-Virgo meeting2/12 Post-VSR1 activities Commissioning/Detector work:  Characterization of ITF controls, Calibration,  Improving the injection system (Temp., Alignment, PZT…)  Investigation of the resonances  Study the Environmental noises  Diffuse light reduction  Reduction of control noises at low frequency  Air conditioning upgrade in DAQ room  Replace some mirror magnets  … See Edwige talk this morning

March 17, 2008LSC-Virgo meeting3/12 Post-VSR1 Duty Cycles ITF Lock: 42% Science Mode: 14% → Astrowatch data

March 17, 2008LSC-Virgo meeting4/12 Virgo Sensitivity progress May 18: Inspiral range: 3.6 Mpc Nov 27 and AC OFF: Inspiral range 5.1 Mpc March 8 Inspiral range 5.5 Mpc

March 17, 2008LSC-Virgo meeting5/12 Robustness improvement Stay locked under stormy weather (strong wind) thanks to:  “Global Inverted Pendulum Control” (“GIPC”)  Angular control improvements  Multiple low noise setting for the actuators March 5: Wind speed close to the maximum level ever observed on site. Wind Speed (MPH) 18 Hours Inspiral BNS range (MPC)

March 17, 2008LSC-Virgo meeting6/12 From now to Virgo+ Next months commissioning  Environmental noise coupling to the dark fringe »Brewster → Cryogenic trap (Last week)  Install the Thermal Compensation System and commission it  More magnets change Q2/Q3-2008:  Install the Laser amplifier, Mode Cleaner, New control electronics Second half of 2008 to Q  Global commissioning Q  Start VSR2 with the existing mirrors Late 2009/2010  Install the new mirrors/monolithic suspension when ready

March 17, 2008LSC-Virgo meeting7/12 Advanced Virgo (AdV) GOALS: Sensitivity: about 10x better than Virgo Timeline: be back online with AdvLIGO MAIN CHANGES: ITF topology

March 17, 2008LSC-Virgo meeting8/12 BEAM - DETECTION see talk by A.Freise OPT. LAYOUT BASELINE: TEM 00 WAIST IN THE CAVITY CENTER LARGER BEAM: requires changing the vacuum links in the central area. DET. BASELINE: PHOTODIODES IN VACUUM DC DETECTION  remark: to be tried in Virgo+ ALTERNATIVE OPTION: HIGH ORDER LAGUERRE MODES SIGNAL RECYCLING

March 17, 2008LSC-Virgo meeting9/12 AdV Baseline Summary heavier mirrors (42 kg) high finesse (≈1000) larger beam waist DC detection signal recycling new IP tilt control new payload fused silica suspensions high power SSL (200 W)

March 17, 2008LSC-Virgo meeting10/12 BNS range: 121 Mpc BBH range: 856 Mpc 1 kHz sens.: /√Hz AdV Sensitivity Curve - Preliminary This example: DESIGN PARAMETERS:  SR mirror transmittance: 0.04  Input mirror transm:  Finesse: 885  PR factor: 23.5  Power on BS: 2.9 kW

March 17, 2008LSC-Virgo meeting11/12 Advanced Virgo Status Last October:  Conceptual Design and Preliminary Cost Plan and Project Execution Plan submitted to the STAC and funding agencies.  Estimate AdV capital investment 16M€ over 3-4 years EGO Council reaction (end of November): “The Council supports the Advanced Virgo project and takes note of the proposed milestones. Not yet a formal approval with financial commitment  But the first AdVirgo expenses are expected to be made only in  Real decision to be made next November when approving the 2009 EGO Budget We are now preparing the detailed design  System managers appointment in progress

March 17, 2008LSC-Virgo meeting12/12 Collaboration News Next Virgo Spokesperson;  A new spokesperson will start his 3 year term on May 3rd  The candidate selected by the Collaboration is Francesco Fidecaro  The EGO Council is likely to go along the Collaboration choice in April New group  The POLGRAW (A. Krolak et al.) apply for membership »To be decided during the April Virgo week Next Virgo (and LV) meetings  April 21 EGO Council (EGO Scientific Director appointment, Budget issues,…)  April 21-24: VirgoWeek; Cascina (One day for R&D review at the beginning)  May 6: VSC meeting to review the Virgo R&D proposition  June 9-12: LV meeting; Orsay (D.A. focus)  June 23-24: EGO Council meeting (R&D Budget?)  July 15-17: V Week; Cascina  Sep 15-20: LV meeting Amsterdam (With “Instrument Science” topics) Sep ?