نتایج جستجو برای: gw code

تعداد نتایج: 172713  

2012
F. ROBINET Albert Einstein

In 2011, the Virgo gravitational wave (GW) detector will definitively end its science program following the shut-down of the LIGO detectors the year before. The years to come will be devoted to the development and installation of second generation detectors. It is the opportune time to review what has been learned from the GW searches in the kilometric interferometers data. Since 2007, data hav...

2013
J. Abadie B. P. Abbott R. Abbott T. Abbott M. R. Abernathy T. Accadia J. Aasi F. Acernese C. Adams T. Adams R. X. Adhikari C. Affeldt M. Agathos N. Aggarwal O. D. Aguiar P. Ajith B. Allen A. Allocca E. Amador Ceron D. Amariutei R. A. Anderson S. B. Anderson W. G. Anderson K. Arai M. C. Araya C. Arceneaux J. Areeda S. Ast S. M. Aston P. Astone P. Aufmuth C. Aulbert L. Austin B. E. Aylott S. Babak P. T. Baker G. Ballardin S. W. Ballmer J. C. Barayoga D. Barker S. H. Barnum F. Barone B. Barr L. Barsotti M. Barsuglia M. A. Barton I. Bartos R. Bassiri A. Basti M. G. Beker A. S. Bell C. Bell I. Belopolski G. Bergmann J. M. Berliner A. Bertolini D. Bessis J. Betzwieser P. T. Beyersdorf T. Bhadbhade I. A. Bilenko M. A. Bizouard E. Black J. K. Blackburn F. Bondu L. Bonelli R. Bonnand R. Bork M. Born S. Bose L. Bosi J. Bowers C. Bradaschia P. R. Brady V. B. Braginsky M. Branchesi C. A. Brannen J. E. Brau J. Breyer T. Briant D. O. Bridges A. Brillet M. Brinkmann V. Brisson M. Britzger A. F. Brooks D. A. Brown D. D. Brown F. Brückner T. Bulik H. J. Bulten A. Buonanno D. Buskulic C. Buy R. L. Byer L. Cadonati G. Cagnoli J. Calderón K. C. Cannon B. Canuel J. Cao C. D. Capano F. Carbognani L. Carbone S. Caride A. Castiglia S. Caudill M. Cavaglià F. Cavalier R. Cavalieri G. Cella C. Cepeda E. Cesarini R. Chakraborty T. Chalermsongsak S. Chao P. Charlton E. Chassande-Mottin X. Chen Y. Chen A. Chincarini A. Chiummo H. S. Cho J. Chow N. Christensen Q. Chu S. S. Y. Chua S. Chung G. Ciani

During the Laser Interferometer Gravitational-wave Observatory and Virgo joint science runs in 2009–2010, gravitational wave (GW) data from three interferometer detectors were analyzed within minutes to select GW candidate events and infer their apparent sky positions. Target coordinates were transmitted to several telescopes for follow-up observations aimed at the detection of an associated op...

2015
Sudarshana Nandi Surjya Kumar Saikia

Factor and multiple regression analysis were used to extract the morphometric variables that contributed to feeding success in three small freshwater fishes. Of the first two factors, factor 1, showed high loading of gut weight (GW), length of the upper (UJ), and lower jaws (LJ) in mola, Amblypharyngodon mola (Hamilton), and GW and vertical mouth opening (VMO) in punti, Puntius ticto (Hamilton)...

Journal: :Journal of psychosomatic research 2006
Dominic Murphy Richard Hooper Claire French Margaret Jones Roberto Rona Simon Wessely

BACKGROUND Following the 1991 Gulf War (GW) there was much controversy surrounding service-related health effects. Evidence from the Vietnam experience suggested that self-reported ill health following that conflict might be related to how service during the conflict is framed. The aim of this article is to determine if a GW health effect persisted when the same questions were asked in a "non-G...

Journal: :Molecular biology of the cell 2002
Theophany Eystathioy Edward K L Chan Scott A Tenenbaum Jack D Keene Kevin Griffith Marvin J Fritzler

A novel human cellular structure has been identified that contains a unique autoimmune antigen and multiple messenger RNAs. This complex was discovered using an autoimmune serum from a patient with motor and sensory neuropathy and contains a protein of 182 kDa. The gene and cDNA encoding the protein indicated an open reading frame with glycine-tryptophan (GW) repeats and a single RNA recognitio...

1993
Wilsin Gosti Giao Nguyen Marlene Wan Min Zhou

In this project, we investigated several approximation algorithms for the Max-Cut problem. Our main approach to this problem is a semideenite program (GW) based algorithm that has a performance guarantee of at least 0.878 of the optimal cut. We also show that we can perform exhaustive local search on top of the GW to enhance the result. Our results show that the running time of the local search...

2011
J.-P. Berger J. D. Monnier R. Millan-Gabet S. Renard E. Pedretti W. Traub K. Perraut S. Ragland P. Schloerb P. A. Schuller

Context. Young and close multiple systems are unique laboratories to probe the initial dynamical interactions between forming stellar systems and their dust and gas environment. Their study is a key building block to understanding the high frequency of main-sequence multiple systems. However, the number of detected spectroscopic young multiple systems that allow dynamical studies is limited. GW...

2009
Riccardo DeSalvo

Accelerometers were and are being developed to instrument the seismic attenuation chains of gravitational wave (GW) interferometric detectors. The main requirements of these instruments are strong directionality (>10 rejection of signal from orthogonal directions for feedback) and vacuum compatibility as well as high low-frequency sensitivity. Because of the directionality requirements, GW acce...

2002
Demetrios Papadopoulos

The equations which determine the response of a charged particle moving in a magnetic field to an incident gravitational wave(GW) are derived in the linearized approximation to general relativity. We briefly discuss several astrophysical applications of the derived formulae taking into account the resonance between the wave and the particle’s motion which occurs at ωg = 2Ω, whenever the GW is p...

2006
G. Branduardi-Raymont

We discuss astrophysical scenarios relevant to the generation of gravitational waves (GW) and effects expected to arise from the interaction of GW and electromagnetic (EM) radiation. A strong programme of coordinated GW and EM astrophysical studies must be established in order to ensure the exploitation of the full scientific potential of the LISA mission. We describe on-going astrophysical wor...

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