Results 161 to 170 of about 18,093 (220)

Low-latency gravitational wave alert products and their performance at the time of the fourth LIGO-Virgo-KAGRA observing run. [PDF]

Proc Natl Acad Sci U S A
Chaudhary SS, Toivonen A, Waratkar G, Mo G, Chatterjee D, Antier S, Brockill P, Coughlin MW, Essick R, Ghosh S, Morisaki S, Baral P, Baylor A, Adhikari N, Brady P, Cabourn Davies G, Dal Canton T, Cavaglia M, Creighton J, Choudhary S, Chu YK, Clearwater P, Davis L, Dent T, Drago M, Ewing B, Godwin P, Guo W, Hanna C, Huxford R, Harry I, Katsavounidis E, Kovalam M, Li AKY, Magee R, Marx E, Meacher D, Messick C, Morice-Atkinson X, Pace A, De Pietri R, Piotrzkowski B, Roy S, Sachdev S, Singer LP, Singh D, Szczepanczyk M, Tang D, Trevor M, Tsukada L, Villa-Ortega V, Wen L, Wysocki D.   +52 more
europepmc   +1 more source

High-<i>Q</i> microresonators unveil quantum rare events. [PDF]

Sci Adv
Raghavan-Chitra S, Koner A, Yuen-Zhou J.
europepmc   +1 more source

Cryo-EM SPR structures of Salmonella typhimurium ArnC; the key enzyme in lipid-A modification conferring polymyxin resistance. [PDF]

Protein Sci
Patel DH, Karimullina E, Guo Y, Semper C, Patel DT, Emde T, Borek D, Savchenko A.   +7 more
europepmc   +1 more source

Revealing the hidden sequence distribution of epitope-specific TCR repertoires and its influence on machine learning model performance

Gielis S, Chernigovskaya M, Pavlovic M, Van Deuren V, Vandoren R, Valkiers S, Laukens K, Greiff V, Meysman P.   +8 more
europepmc   +1 more source

Characterization of the LIGO detectors during their sixth science run [PDF]

Classical and Quantum Gravity, 2015
In 2009–2010, the Laser Interferometer Gravitational-Wave Observatory (LIGO) operated together with international partners Virgo and GEO600 as a network to search for gravitational waves (GWs) of astrophysical origin.
Tito Dal Canton, Robert Ward, Imre Bartos   +2 more
exaly   +2 more sources

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Calibration of the LIGO detectors for the First LIGO Science Run

Classical and Quantum Gravity, 2003
We describe the calibration procedures applied to the data taken by the three LIGO interferometric gravitational wave detectors in the LIGO Science Collaborations First Science Run, from 23 August to 9 September 2002. The calibration depends on corrections to feedback servos used in the instrument, and on changing optical gains.
Rana Adhikari, Gabriela Gonz lez, Michael Landry, Brian O Reilly (for the LIGO Scient Collaboration)   +3 more
openaire   +1 more source