Searching for gravitational waves from known pulsars Matthew Pitkin for the LIGO Scientific Collaboration Summary of work to date There have been three science runs ...
Change mirrors, beam size, modulation frequency. Upgrade Mode Cleaner ... Build a set of ARMA filters. Follow optical gain. High pass filter. E4 data: ...
check out updates at conference main page, http://gwdaw12.mit.edu ... of the Hub at the Prudential Center: shuttle to/from will be provided check out ...
New MI SR servo. SR bench scattering. GWDAW 9, Annecy 2004. Target sensitivity ... Optimisation routine is used to quasi-continuously estimate parameters of ...
NAUTILUS and EXPLORER. Binary files: raw data sampled @ 5 kHz ... NAUTILUS: December 2004. SNR. Terr [ s ] GWDAW10 - December 14th, 2005 - Brownsville, Texas ...
Status of Virgo. Gabriele Vajente. INFN Pisa and Scuola Normale Superiore di Pisa. On ... (talk by G.Cella) GWDAW 11 December 18th , 2006 Gabriele Vajente. 17 ...
Washington State University, Pullman. GWDAW-2004, Annecy, France. NASA-NAG5-12837. 15 Dec 2004 ... no Doppler f-modulation, monochromatic sources (galactic ...
HETE error circle. Chandra (Fox et al, Nature, 2005) Dec 16, 2005. GWDAW ... j,k = detector 1, 2. Max-cc density depends on three scalar variables derived from ...
Derivation of F-Statistic for Multi-IFO. with independent noises: ... Defining the F-Statistic as the log of likelihood function: 'X' indicates different detectors ...
To distinguish GW signals, we should remove noises to be misidentified as GW signals. ... Transfer Function. HINT. DINT. FINT. AINT. WFINT. DINT. V3. Vs. V3 ...
C6: a posteriori vetoes. SNR distribution between low and high frequency bands ... Hardware injections, quality cuts, a posteriori vetoes. Pursue investigations ...
2 Associated Commissions-- AC2 General Relativity. 3 Working Groups: ICFA; PaNAGIC and Women in Physics ... Virgo and LIGO exchanging environmental data, and ...
Warren Johnson, Bill Hamilton, Peter Zhang, Andrew Weber, Damon Nettles, ... now have 200 days available for comparison with NAUTILUS, EXPLORER, and AURIGA. ...
Time coincidence. and. Frequency clustering. BlockNormal / AstroBurst ... Time & frequency coincidence, clustering. Q-pipeline. H null stream. H coherent sum ...
... statistic (Drasco et al. 2003), Probability Event Horizon (Coward et al. 2005) ... Neutron star formation: Blair & Ju 1996, Coward et al. 2001-02, Howell et al. ...
NAUTILUS (INFN-LNF) INFN of Roma and LNF. Universities of Roma, L'Aquila ... 5 AURIGA, EXPLORER, NAUTILUS amplitude range much wider than expected: ...
Long delays: (same example ... more from short delays (extremely short in example) ... Long delays: dP/dt. G070885-00-Z. Other factors: Systematics. Binary ...
... a department of the 'Observatoire de la C te d 'Azur ', affiliated with the CNRS ... (4) teaching assistant at the ' Universit de Nice Sophia Antipolis' ...
Overview of the Search. Searched triple-coincidence (H1 H2 L1) LIGO data ... 3 with glitches in H1 beam-splitter pick-off channels (H1:LSC-POB_I and/or H1:LSC-POB_Q) ...
LISA Update. Bernard Schutz. Albert Einstein Institute, Potsdam, Germany. and ... JPL (Tom Prince) is NASA focus, had workshop 13-15 October (http://www.tapir. ...
Inspiral search is very CPU-intensive ... ... but still need (eventually) to do real-time. Can we get comparable (or more) coverage w/ a fast search? ...
The GRB Coordinates Network (GCN) The third InterPlanetary Network (IPN3) ... Due to the sub-burst longitude and latitude and the geographical distribution of ...
In-spiral: last few minutes in the band accessible to LIGO and Virgo ... O(1050 ergs) would produce a GW signal that could be detected by the adv Virgo ...