Status of GEO600. Benno Willke. for the GEO600 team. ESF ... Spectrogram of h(t) Calibration. Data quality. Chi2. Calibration parameters. Bursts (HACRmon) ...
LSC Boston 19.11.05. The Status of GEO600. Joshua Smith for the GEO 600 team ... Joshua Smith, Boston, 19.11.05. Work Ahead, S5 Plans. Period of intense noise hunting ...
New MI SR servo. SR bench scattering. GWDAW 9, Annecy 2004. Target sensitivity ... Optimisation routine is used to quasi-continuously estimate parameters of ...
... Smith, the GEO600 team, Albert-Einstein-Institute, Syracuse University, Glasgow ... Thermal Noise sets a fundamental limit on how still the mirrors that we are ...
Searches for continuous gravitational waves with LIGO and GEO600 M. Landry for the LIGO Scientific Collaboration LIGO Hanford Observatory, Richland WA 99352
Silica Research in Glasgow Gianpietro Cagnoli IGR - University of Glasgow GEO Collaboration Ginzton Lab, Stanford Caltech Summary Silica suspensions in GEO600 ...
LIGO, VIRGO (Pisa), GEO600,...$1 Billion Worldwide. We need results from numerical relativity to: ... backgrounds, different personalities, on different ...
LIGO, VIRGO (Pisa), GEO600,... $1 Billion Worldwide. Was Einstein right? 5-10 ... of people in 'seed' community, with different backgrounds, personalities, on ...
Title: Folie 1 Last modified by: stefan hild Document presentation format: Benutzerdefiniert Other titles: Times New Roman StarSymbol Arial Wingdings Symbol ...
... = more fluctuating radiation pressure P=1 MW F=3 mN dF=1.5 Readout noise The Standard Quantum Limit For a simple ... Harmonic Oscillator Lower T ... Excel ...
Gravitational Wave Detectors Course in Inflation, Structure formation and CMB 7 November 2002 Silvio Orsi GW: My presentation GW production Upper bounds on GW ...
Title: Folie 1 Last modified by: stefan hild Document presentation format: Benutzerdefiniert Other titles: Times New Roman StarSymbol Arial Wingdings Symbol ...
... LO and GW pass the same optical system (identical delay, filtering, spatial profile) = This advantage is especially important for detectors with arm cavities.
What is the smallest value L, if the waves are to end up ... Fresnel's Spot. 36-3. Single-Slit Diffraction. Destructive Interference. Pair-wise Cancellation ...
Title: PowerPoint Presentation Author: Joan M. Centrella Last modified by: Joan Centrella Created Date: 9/7/2001 3:31:51 PM Document presentation format
Passing GW causes changes in the interferometer arm lengths. ... Of known pulsars Crab pulsar is most promising source, also possible pulsar in SN1987A remnant. ...
People Needed! To compute wave forms. To run the detectors. To analyze the data ... Waves from a deformed rotating NS. Solid crust deformations (Curt at AEI ! ...
LIGO-G030546-00-D. Gravitational Wave Observations with Interferometers: Results and Prospects ... Prospects for improvement: 100-1000x from detector ...
LIGO is taking data for the 2nd time and it's only a factor of 10 from design ... Bernd Brugmann professor in Penn Stare. There is room for more!! 10/18/09 ...
DRMI gives 2 output signals, each containing GW information P(t) and Q(t) There is a transfer function from h(t) ... Undoing the effect of the optical response ...
Title: PowerPoint Presentation Author: Michael Landry Last modified by: Staff Created Date: 11/3/2003 12:43:07 AM Document presentation format: On-screen Show
... [ee]e^e_e`eaebecedeeefegeheiejekelemeneoepeqereseteuevewexeyeze{e|e}e~ee e e e ... DllDddLllTttTllttTddlldttdd8JHv G[XT|tDlbLtjLldTtl|t dY y Tld ...
Elba, Italy 31.05.06. Joshua Smith for the GEO 600 team. Picture of GEO in stormy weather? ... Joshua Smith, Elba, Italy 31.05.06. Power glitches vs. dust ...
Waves created by (likely) astrophysical sources cause relative length changes ... by some force (eg., buoyancy storm updraft, mountain) and restored by gravity. ...
Make something cheap (comparatively), expandable and versatile ... Each module connects directly to a data collecting computer via TCP/IP. GEO meeting Sept 2004 ...
Daily modulation. G060531-00-M. Matched-filtering. Suppose we have a ... Neutron star search results. Directed searches Crab pulsar. Crab limit now below the ...
The LIGO Scientific Collaboration is an international effort to ... Search for binary neutron star coalescences in the Local Group of galaxies (in preparation) ...
GORU E TEME U ASTROFIZICI Bojan Arbutina Katedra za astronomiju Matemati kog fakulteta Univerziteta u Beogradu arbo@math.rs nere eni problemi u astrofizici gama ...
lensing in our own Galaxy have revealed a large population of black holes made ... Lensing by a cluster of galaxies ... formation of galaxies. the creation of ...
Need 100kW of laser power in arms, use power recycling so that laser ... Crab Spindown. Upper Limit. Known Pulsars: First Interferometers: 3x10-6 (1000Hz/f) ...
Homodyne readout of an interferometer with Signal Recycling. Stefan Hild ... Laser power noise is not as bad as rumors suggest (due to filtering of PR cavity pole) ...
Using Gravitational Waves Detectors to detect something ... http://elmer.tapir.caltech.edu/ph237. Very high resolution ... 2x1.5Gb/lecture. Normal resolution .