Results 31 to 40 of about 200,534 (264)
Millisecond Conversion of Metastable 2D Materials by Flash Joule Heating.
ACS Nano, 2021 Controllable phase engineering is vital for precisely tailoring material properties since different phase structures have various electronic states and atomic arrangements.Weiyin Chen, Zhe Wang, Ksenia V. Bets, D. Luong, Muqing Ren, M. Stanford, E. McHugh, Wala A. Algozeeb, Hua Guo, G. Gao, Bing Deng, Jinhang Chen, J. T. Li, William T Carsten, B. Yakobson, J. Tour +15 moresemanticscholar +1 more sourceGravitational-wave Constraints on the Equatorial Ellipticity of Millisecond Pulsars [PDF]
Astrophysical Journal Letters, 2020 We present a search for continuous gravitational waves from five radio pulsars, comprising three recycled pulsars (PSR J0437−4715, PSR J0711−6830, and PSR J0737−3039A) and two young pulsars: the Crab pulsar (J0534+2200) and the Vela pulsar (J0835−4510 ...R. Abbott, T. Abbott, S. Abraham, F. Acernese, K. Ackley, A. Adams, C. Adams, R. Adhikari, V. Adya, C. Affeldt, M. Agathos, M. Agathos, K. Agatsuma, N. Aggarwal, O. Aguiar, L. Aiello, A. Ain, P. Ajith, G. Allen, A. Allocca, P. Altin, A. Amato, S. Anand, A. Ananyeva, S. Anderson, W. Anderson, S. Angelova, S. Ansoldi, J. Antelis, S. Antier, S. Appert, K. Arai, M. Araya, J. Areeda, M. Arène, N. Arnaud, S. Aronson, K. Arun, Y. Asali, S. Ascenzi, G. Ashton, S. Aston, P. Astone, F. Aubin, P. Aufmuth, K. AultONeal, C. Austin, V. Avendano, S. Babak, F. Badaracco, M. Bader, S. Bae, A. Baer, S. Bagnasco, M. Bailes, J. Baird, M. Ball, G. Ballardin, S. Ballmer, A. Bals, A. Balsamo, G. Baltus, S. Banagiri, D. Bankar, R. S. Bankar, J. Barayoga, Cesare Barbieri, Cesare Barbieri, B. Barish, D. Barker, P. Barneo, S. Barnum, F. Barone, B. Barr, L. Barsotti, M. Barsuglia, D. Barta, J. Bartlett, I. Bartos, R. Bassiri, A. Basti, M. Bawaj, J. Bayley, M. Bazzan, B. Becher, B. Bécsy, V. Bedakihale, M. Bejger, I. Belahcene, D. Beniwal, M. Benjamin, T. Bennett, J. Bentley, F. Bergamin, B. Berger, G. Bergmann, S. Bernuzzi, D. Bersanetti, A. Bertolini, J. Betzwieser, R. Bhandare, A. Bhandari, D. Bhattacharjee, J. Bidler, I. Bilenko, G. Billingsley, R. Birney, O. Birnholtz, S. Biscans, S. Biscans, M. Bischi, S. Biscoveanu, A. Bisht, M. Bitossi, M. Bizouard, J. Blackburn, J. Blackman, C. Blair, D. Blair, R. Blair, O. Blanch, F. Bobba, N. Bode, M. Boer, Y. Boetzel, G. Bogaert, M. Boldrini, F. Bondu, R. Bonnand, P. Booker, B. Boom, R. Bork, V. Boschi, S. Bose, V. Bossilkov, V. Boudart, Y. Bouffanais, A. Bozzi, C. Bradaschia, P. Brady, A. Bramley, M. Branchesi, J. Brau, M. Breschi, T. Briant, J. Briggs, F. Brighenti, A. Brillet, M. Brinkmann, P. Brockill, A. Brooks, J. Brooks, Daniel Brown, S. Brunett, G. Bruno, R. Bruntz, A. Buikema, T. Bulik, H. Bulten, A. Buonanno, A. Buonanno, D. Buskulic, R. Byer, M. Cabero, L. Cadonati, M. Caesar, G. Cagnoli, C. Cahillane, J. C. Bustillo, J. Callaghan, T. Callister, E. Calloni, J. Camp, M. Canepa, K. Cannon, H. Cao, Junwei Cao, G. Carapella, F. Carbognani, M. Carney, M. Carpinelli, G. Carullo, T. Carver, J. C. Diaz, C. Casentini, S. Caudill, M. Cavaglià, F. Cavalier, R. Cavalieri, G. Cella, P. Cerdá-Durán, E. Cesarini, W. Chaibi, K. Chakravarti, C. Chan, C. Chan, K. Chandra, P. Chanial, S. Chao, P. Charlton, E. Chase, É. Chassande-Mottin, D. Chatterjee, M. Chaturvedi, A. Chen, H. Chen, Xu Chen, Yan Chen, H. Cheng, C. Cheong, H. Chia, F. Chiadini, R. Chierici, A. Chincarini, A. Chiummo, G. Cho, H. Cho, M. Cho, S. Choate, N. Christensen, Q. Chu, S. Chua, K. Chung, S. Chung, G. Ciani, P. Ciecieląg, M. Cieślar, M. Cifaldi, A. Ciobanu, R. Ciolfi, F. Cipriano, A. Cirone, F. Clara, E. Clark, J. Clark, L. Clarke, P. Clearwater, S. Clesse, F. Cleva, E. Coccia, P. Cohadon, D. Cohen, M. Colleoni, C. Collette, C. Collins, M. Colpi, M. Constancio, L. Conti, S. Cooper, P. Corban, T. Corbitt, I. Cordero-Carrión, S. Corezzi, K. Corley, N. Cornish, D. Corre, A. Corsi, S. Cortese, C. A. Costa, R. Cotesta, M. Coughlin, M. Coughlin, S. Coughlin, S. Coughlin, J. Coulon, S. Countryman, P. Couvares, P. Covas, D. Coward, M. Cowart, D. Coyne, R. Coyne, J. Creighton, T. Creighton, M. Croquette, S. Crowder, J. Cudell, T. Cullen, A. Cumming, R. Cummings, L. Cunningham, E. Cuoco, M. Curylo, T. D. Canton, T. D. Canton, G. Dalya, A. Dana, L. M. Daneshgaran-Bajastani, Beatrice D'Angelo, S. Danilishin, S. D’Antonio, K. Danzmann, C. Darsow-Fromm, A. Dasgupta, L. Datrier, V. Dattilo, I. Dave, M. Davier, G. Davies, D. Davis, E. Daw, R. Dean, D. Debra, M. Deenadayalan, J. Degallaix, M. D. Laurentis, S. Deléglise, V. D. Favero, N. D. Lillo, W. D. Pozzo, L. Demarchi, F. Matteis, V. d’Emilio, N. Demos, T. Denker, T. Dent, A. Depasse, R. Pietri, R. Rosa, C. Rossi, R. DeSalvo, O. D. Varona, S. Dhurandhar, M. Díaz, M. Diaz-Ortiz, N. Didio, T. Dietrich, L. Fiore, C. DiFronzo, C. Giorgio, F. D. Giovanni, M. Giovanni, T. D. Girolamo, A. D. Lieto, B. Ding, S. D. Pace, I. Palma, F. Renzo, A. K. Divakarla, A. Dmitriev, Zoheyr Doctor, L. D’Onofrio, F. Donovan, K. Dooley, S. Doravari, I. Dorrington, T. P. Downes, M. Drago, J. Driggers, Zhi-hui Du, J. Ducoin, P. Dupej, O. Durante, D. D’Urso, P. Duverne, S. Dwyer, P. Easter, G. Eddolls, B. Edelman, T. Edo, O. Edy, A. Effler, J. Eichholz, S. Eikenberry, M. Eisenmann, R. Eisenstein, A. Ejlli, L. Errico, R. Essick, H. Estellés, D. Estevez, Z. Etienne, T. Etzel, M. Evans, T. Evans, B. Ewing, V. Fafone, H. Fair, S. Fairhurst, Xiaodan Fan, A. Farah, S. Farinon, B. Farr, W. Farr, E. Fauchon-Jones, Marc Favata, M. Fays, M. Fays, M. Fazio, J. Feicht, M. Fejer, F. Feng, E. Fenyvesi, D. Ferguson, Á. Fernández-Galiana, I. Ferrante, T. A. Ferreira, F. Fidecaro, P. Figura, I. Fiori, D. Fiorucci, M. Fishbach, R. Fisher, J. Fishner, R. Fittipaldi, M. Fitz-Axen, V. Fiumara, R. Flaminio, E. Floden, E. Flynn, H. Fong, J. Font, P. Forsyth, J. Fournier, S. Frasca, F. Frasconi, Z. Frei, A. Freise, R. Frey, V. Frey, P. Fritschel, V. Frolov, G. Fronzé, P. Fulda, M. Fyffe, H. Gabbard, B. Gadre, S. Gaebel, J. Gair, J. Gais, S. Galaudage, R. Gamba, D. Ganapathy, A. Ganguly, S. Gaonkar, B. Garaventa, C. García-Quirós, F. Garufi, B. Gateley, S. Gaudio, V. Gayathri, G. Gemme, A. Gennai, D. George, J. George, L. '. Gergely, S. Ghonge, A. Ghosh, A. Ghosh, S. Ghosh, S. Ghosh, B. Giacomazzo, B. Giacomazzo, L. Giacoppo, J. Giaime, J. Giaime, K. Giardina, D. Gibson, C. Gier, K. Gill, P. Giri, J. Glanzer, A. Gleckl, P. Godwin, E. Goetz, R. Goetz, N. Gohlke, B. Goncharov, G. González, A. Gopakumar, S. Gossan, M. Gosselin, R. Gouaty, B. Grace, A. Grado, M. Granata, V. Granata, A. Grant, S. Gras, P. Grassia, C. Gray, R. Gray, G. Greco, A. Green, R. Green, E. Gretarsson, H. L. Griggs, G. Grignani, A. Grimaldi, E. Grimes, S. Grimm, H. Grote, S. Grunewald, P. Gruning, J. G. Guerrero, G. Guidi, A. R. Guimaraes, G. Guixé, H. Gulati, Y. Guo +499 moresemanticscholar +1 more sourceComparing random dot motion in MATLAB vs. Inquisit Millisecond
Frontiers in Psychology, 2022 Random Dot Motion (RDM) displays refer to clouds of independently moving dots that can be parametrically manipulated to provide a perception of the overall cloud moving coherently in a specified direction of motion.Kimia C. Yaghoubi, Sarah Kabbara, Sara Arian, Hadi Kobaissi, Megan A. K. Peters, Megan A. K. Peters, Aaron R. Seitz +6 moredoaj +1 more sourceThe Galactic Millisecond Pulsar Population [PDF]
, 2012 Among the current sample of over 2000 radio pulsars known primarily in the
disk of our Galaxy, millisecond pulsars now number almost 200. Due to the
phenomenal success of blind surveys of the Galactic field, and targeted
searches of Fermi gamma-ray ...Lorimer, Duncan R.core +1 more sourceA NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437–4715 [PDF]
Astrophysical Journal LettersWe report Bayesian inference of the mass, radius, and hot X-ray emitting region properties—using data from the Neutron Star Interior Composition ExploreR (NICER)—for the brightest rotation-powered millisecond X-ray pulsar, PSR J0437−4715. Our modeling is Devarshi Choudhury, Tuomo Salmi, S. Vinciguerra, T. E. Riley, Yves Kini, A. Watts, Bas Dorsman, S. Bogdanov, S. Guillot, P. Ray, D. Reardon, R. Remillard, A. Bilous, D. Huppenkothen, J. Lattimer, Nathan Rutherford, Z. Arzoumanian, K. Gendreau, S. Morsink, W. C. Ho +19 moresemanticscholar +1 more sourceMillisecond Magnetars
, 2021 Two classes of X-ray/$γ$-ray sources, the Soft Gamma Repeaters and the Anomalous X-ray Pulsars have been identified with isolated, slowly spinning magnetars, neutron stars whose emission draws energy from their extremely strong magnetic field ($\sim 10^{15}-10^{16}$ G).Dall'Osso, Simone, Stella, Luigiopenaire +2 more sourcesMillisecond accuracy video display using OpenGL under Linux [PDF]
, 2006 To measure people’s reaction times to the nearest millisecond, it is necessary to know exactly when
a stimulus is displayed. This article describes how to display stimuli with millisecond accuracy on a
normal CRT monitor, using a PC running Linux.A. Nye, B. Myors, B. Myors, J.-L. Tsai, M. Woo, N. Stewart, Neil Stewart, R. [E.] Graves, R. E. Graves, R. P. Plant, S. A. Finney, W. J. MacInnes +11 morecore +2 more sourcesThe NANOGrav 11-year Data Set: High-precision Timing of 45 Millisecond Pulsars [PDF]
, 2017 We present high-precision timing data over time spans of up to 11 years for 45 millisecond pulsars observed as part of the North American Nanohertz Observatory for Gravitational Waves (NANOGrav) project, aimed at detecting and characterizing low ...Z. Arzoumanian, A. Brazier, S. Burke-Spolaor, S. Chamberlin, S. Chatterjee, B. Christy, J. Cordes, N. Cornish, F. Crawford, H. Cromartie, K. Crowter, M. DeCesar, P. Demorest, T. Dolch, Justin A. Ellis, R. Ferdman, E. Ferrara, E. Fonseca, N. Garver-Daniels, P. Gentile, Daniel Halmrast, Daniel Halmrast, E. Huerta, F. Jenet, Cody Jessup, Glenn Jones, Megan L. Jones, David L. Kaplan, M. Lam, T. Lazio, L. Levin, A. Lommen, D. Lorimer, J. Luo, R. Lynch, D. Madison, Allison M. Matthews, M. McLaughlin, S. McWilliams, C. Mingarelli, C. Ng, C. Ng, D. Nice, T. Pennucci, S. Ransom, P. Ray, X. Siemens, J. Simon, R. Spiewak, R. Spiewak, I. Stairs, D. Stinebring, K. Stovall, J. Swiggum, S. Taylor, M. Vallisneri, R. V. Haasteren, S. Vigeland, Weiwei Zhu, Weiwei Zhu +59 moresemanticscholar +1 more sourceDescription and Application of the Surfing Effect
Universe, 2022 The standard technique for very low-frequency gravitational wave detection is mainly based on searching for a specific spatial correlation in the variation of the times of arrival of the radio pulses emitted by millisecond pulsars with respect to a ...Michele Maiorano, Francesco De Paolis, Achille A. Nucita +2 moredoaj +1 more source
