Zobrazeno 1 - 10
of 825 126
pro vyhledávání: '"Simone Andrews'
Winchester's identity as a royal centre became well established between the ninth and twelfth centuries, closely tied to the significance of the religious communities who lived within and without the city walls. The reach of power of Winchester was f
Autor:
Tribello, Gareth A., Bonomi, Massimiliano, Bussi, Giovanni, Camilloni, Carlo, Armstrong, Blake I., Arsiccio, Andrea, Aureli, Simone, Ballabio, Federico, Bernetti, Mattia, Bonati, Luigi, Brookes, Samuel G. H., Brotzakis, Z. Faidon, Capelli, Riccardo, Ceriotti, Michele, Chan, Kam-Tung, Cossio, Pilar, Dasetty, Siva, Donadio, Davide, Ensing, Bernd, Ferguson, Andrew L., Fraux, Guillaume, Gale, Julian D., Gervasio, Francesco Luigi, Giorgino, Toni, Herringer, Nicholas S. M., Hocky, Glen M., Hoff, Samuel E., Invernizzi, Michele, Languin-Cattöen, Olivier, Leone, Vanessa, Limongelli, Vittorio, Lopez-Acevedo, Olga, Marinelli, Fabrizio, Martinez, Pedro Febrer, Masetti, Matteo, Mehdi, Shams, Michaelides, Angelos, Murtada, Mhd Hussein, Parrinello, Michele, Piaggi, Pablo M., Pietropaolo, Adriana, Pietrucci, Fabio, Pipolo, Silvio, Pritchard, Claire, Raiteri, Paolo, Raniolo, Stefano, Rapetti, Daniele, Rizzi, Valerio, Rydzewski, Jakub, Salvalaglio, Matteo, Schran, Christoph, Seal, Aniruddha, Zadeh, Armin Shayesteh, Silva, Tomás F. D., Spiwok, Vojtěch, Stirnemann, Guillaume, Sucerquia, Daniel, Tiwary, Pratyush, Valsson, Omar, Vendruscolo, Michele, Voth, Gregory A., White, Andrew D., Wu, Jiangbo
In computational physics, chemistry, and biology, the implementation of new techniques in a shared and open source software lowers barriers to entry and promotes rapid scientific progress. However, effectively training new software users presents sev
Externí odkaz:
http://arxiv.org/abs/2412.03595
Autor:
Cecconello, Thomas, Riggi, Simone, Becciani, Ugo, Vitello, Fabio, Hopkins, Andrew M., Vizzari, Giuseppe, Spampinato, Concetto, Palazzo, Simone
The upcoming Square Kilometer Array (SKA) telescope marks a significant step forward in radio astronomy, presenting new opportunities and challenges for data analysis. Traditional visual models pretrained on optical photography images may not perform
Externí odkaz:
http://arxiv.org/abs/2411.14078
Autor:
Liotine, Camille, Kalogera, Vicky, Andrews, Jeff J., Bavera, Simone S., Briel, Max, Fragos, Tassos, Gossage, Seth, Kovlakas, Konstantinos, Kruckow, Matthias U., Rocha, Kyle A., Srivastava, Philipp M., Sun, Meng, Teng, Elizabeth, Xing, Zepei, Zapartas, Emmanouil
Binaries harboring a millisecond pulsar (MSP) and a black hole (BH) are a key observing target for current and upcoming pulsar surveys. We model the formation and evolution of such binaries in isolation at solar metallicity using the next-generation
Externí odkaz:
http://arxiv.org/abs/2412.15521
Autor:
Goswami, Dipam, Magistri, Simone, Wang, Kai, Twardowski, Bartłomiej, Bagdanov, Andrew D., van de Weijer, Joost
Using pre-trained models has been found to reduce the effect of data heterogeneity and speed up federated learning algorithms. Recent works have investigated the use of first-order statistics and second-order statistics to aggregate local client data
Externí odkaz:
http://arxiv.org/abs/2412.14326
Autor:
Williams, Gwenllian M., Thompson, Mark A., Mutale, Mubela, Rigby, Andrew J., Bordiu, Cristobal, Riggi, Simone, Bietenholz, Michael, Anderson, Loren D., Camilo, Fernando, Goedhart, Sharmila, Jaffa, Sarah E., Obonyo, Willice O., Trigilio, Corrado, Umana, Grazia
We present a catalogue of filamentary structures identified in the SARAO (South African Radio Astronomy Observatory) MeerKAT 1.3 GHz Galactic Plane Survey (SMGPS). We extract 933 filaments across the survey area, 803 of which (~86%) are associated wi
Externí odkaz:
http://arxiv.org/abs/2412.07852
Autor:
Rocha, Kyle Akira, Hur, Rachel, Kalogera, Vicky, Gossage, Seth, Sun, Meng, Doctor, Zoheyr, Andrews, Jeff J., Bavera, Simone S., Briel, Max, Fragos, Tassos, Kovlakas, Konstantinos, Kruckow, Matthias U., Misra, Devina, Xing, Zepei, Zapartas, Emmanouil
We investigate Roche lobe overflow mass transfer (MT) in eccentric binary systems between stars and compact objects (COs), modeling the coupled evolution of both the star and the orbit due to eccentric MT (eMT) in a self-consistent framework. We impl
Externí odkaz:
http://arxiv.org/abs/2411.11840
Autor:
Bazavov, Alexei, Clarke, David A., Davies, Christine, DeTar, Carleton, El-Khadra, Aida X., Gámiz, Elvira, Gottlieb, Steven, Grebe, Anthony V., Hostetler, Leon, Jay, William I., Jeong, Hwancheol, Kronfeld, Andreas S., Lahert, Shaun, Laiho, Jack, Lepage, G. Peter, Lynch, Michael, Lytle, Andrew T., McNeile, Craig, Neil, Ethan T., Peterson, Curtis T., Simone, James N., Sitison, Jacob W., Van de Water, Ruth S., Vaquero, Alejandro
We present complete results for the hadronic vacuum polarization (HVP) contribution to the muon anomalous magnetic moment $a_\mu$ in the short- and intermediate-distance window regions, which account for roughly 10% and 35% of the total HVP contribut
Externí odkaz:
http://arxiv.org/abs/2411.09656
Autor:
Srivastava, Philipp M., Demir, Ugur, Katsaggelos, Aggelos, Kalogera, Vicky, Teng, Elizabeth, Fragos, Tassos, Andrews, Jeff J., Bavera, Simone S., Briel, Max, Gossage, Seth, Kovlakas, Konstantinos, Kruckow, Matthias U., Liotine, Camille, Rocha, Kyle A., Sun, Meng, Xing, Zepei, Zapartas, Emmanouil
Modeling of large populations of binary stellar systems is an intergral part of a many areas of astrophysics, from radio pulsars and supernovae to X-ray binaries, gamma-ray bursts, and gravitational-wave mergers. Binary population synthesis codes tha
Externí odkaz:
http://arxiv.org/abs/2411.02586
Autor:
Andrews, Jeff J., Bavera, Simone S., Briel, Max, Chattaraj, Abhishek, Dotter, Aaron, Fragos, Tassos, Gallegos-Garcia, Monica, Gossage, Seth, Kalogera, Vicky, Kasdagli, Eirini, Katsaggelos, Aggelos, Kimball, Chase, Kovlakas, Konstantinos, Kruckow, Matthias U., Liotine, Camille, Misra, Devina, Rocha, Kyle A., Souropanis, Dimitris, Srivastava, Philipp M., Sun, Meng, Teng, Elizabeth, Xing, Zepei, Zapartas, Emmanouil, Zevin, Michael
Whether considering rare astrophysical events on cosmological scales or unresolved stellar populations, accurate models must account for the integrated contribution from the entire history of star formation upon which that population is built. Here,
Externí odkaz:
http://arxiv.org/abs/2411.02376