Zobrazeno 1 - 10
of 8 508
pro vyhledávání: '"Murphy, Michael A"'
Autor:
Milaković, Dinko, Webb, John K., Molaro, Paolo, Lee, Chung-Chi, Jethwa, Prashin, Cupani, Guido, Murphy, Michael T., Welsh, Louise, D'Odorico, Valentina, Cristiani, Stefano, Santos, Ricardo Génova, Martins, Carlos J. A. P., Nunes, Nelson J., Schmidt, Tobias M., Pepe, Francesco A., Osorio, Maria Rosa Zapatero, Alibert, Yann, Hernández, J. I. González, Di Marcantonio, Paolo, Palle, Enric, Santos, Nuno C., Rebolo, Rafael
Chemical evolution models predict a gradual build-up of $^{13}$C in the universe, based on empirical nuclear reaction rates and assumptions on the properties of stellar populations. However, old metal-poor stars within the Galaxy contain more $^{13}$
Externí odkaz:
http://arxiv.org/abs/2407.17953
Autor:
Halak, Basel, Csete, Cristian Sebastian, Joyce, Edward, Papaioannou, Jack, Pires, Alexandre, Soma, Jin, Gokkaya, Betul, Murphy, Michael
The rapid advancement of quantum computing poses a significant threat to many current security algorithms used for secure communication, digital authentication, and information encryption. A sufficiently powerful quantum computer could potentially ex
Externí odkaz:
http://arxiv.org/abs/2407.13523
Autor:
Murphy, Michael A.
Machine learning is becoming a pivotal tool in the analysis of datasets generated from high-throughput biological omics experiments. However, omics data introduces distinctive algorithmic challenges that set it apart from other domains where machine
Autor:
Liu, Fan, Ting, Yuan-Sen, Yong, David, Bitsch, Bertram, Karakas, Amanda, Murphy, Michael T., Joyce, Meridith, Dotter, Aaron, Dai, Fei
Stellar chemical compositions can be altered by ingestion of planetary material and/or planet formation which removes refractory material from the proto-stellar disc. These "planet signatures" appear as correlations between elemental abundance differ
Externí odkaz:
http://arxiv.org/abs/2403.13209
Autor:
Guarneri, Francesco, Pasquini, Luca, D'Odorico, Valentina, Cristiani, Stefano, Cupani, Guido, Di Marcantonio, Paolo, Hernández, J. I. González, Martins, C. J. A. P., Mascareño, Alejandro Suárez, Milaković, Dinko, Molaro, Paolo, Murphy, Michael T., Nunes, Nelson J., Palle, Enric, Pepe, Francesco, Rebolo, Rafael, Santos, Nuno C., Santos, Ricardo Génova, Schmidt, Tobias M., Sousa, Sérgio G., Sozzetti, Alessandro, Trost, Andrea
Primordial abundances of light elements are sensitive to the physics of the early Universe and can directly constrain cosmological quantities, such as the baryon-to-photon ratio $\eta_{10}$, the baryon density and the number of neutrino families. Deu
Externí odkaz:
http://arxiv.org/abs/2402.05586
Autor:
Cristiani, Stefano, Cupani, Guido, Trost, Andrea, D'Odorico, Valentina, Guarneri, Francesco, Curto, Gaspare Lo, Meneghetti, Massimo, Di Marcantonio, Paolo, Faria, João P., Hernández, Jonay I. González, Lovis, Christophe, Martins, Carlos J. A. P., Milaković, Dinko, Molaro, Paolo, Murphy, Michael T., Nunes, Nelson J., Pepe, Francesco, Rebolo, Rafael, Santos, Nuno C., Schmidt, Tobias M., Sousa, Sérgio G., Sozzetti, Alessandro, Osorio, María Rosa Zapatero
The gravitationally lensed quasar J014516.6-094517 at z=2.719 has been observed with the ESPRESSO instrument at the ESO VLT to obtain high-fidelity spectra of the two images A and B with a resolving power R=70000. At the redshifts under investigation
Externí odkaz:
http://arxiv.org/abs/2402.05896
Autor:
Magrini, Laura, Bensby, Thomas, Brucalassi, Anna, Randich, Sofia, Jeffries, Robin, de Silva, Gayandhi, Skuladottir, Asa, Smiljanic, Rodolfo, Gonzalez, Oscar, Hill, Vanessa, Lagarde, Nadege, Tolstoy, Eline, Arroyo-Polonio, Jose' Maria, Baratella, Martina, Barnes, John R., Battaglia, Giuseppina, Baumgardt, Holger, Bellazzini, Michele, Biazzo, Katia, Bragaglia, Angela, Carter, Bradley, Casali, Giada, Cescutti, Gabriele, Danielski, Camilla, Mena, Elisa Delgado, Drazdauskas, Arnas, Gieles, Mark, Giribaldi, Riano, Hawkins, Keith, Hoeijmakers, H. Jens, Jablonka, Pascale, Kamath, Devika, Louth, Tom, Marino, Anna Fabiola, Martell, Sarah, Merle, Thibault, Montet, Benjamin, Murphy, Michael T., Nisini, Brunella, Nordlander, Thomas, D'Orazi, Valentina, Pino, Lorenzo, Romano, Donatella, Sacco, Germano, Sandford, Nathan R., Sollima, Antonio, Spina, Lorenzo, Tautvaivsiene, Grazina, Ting, Yuan-Sen, Tozzi, Andrea, Van der Swaelmen, Mathieu, Van Eck, Sophie, Watson, Stephen, Worley, C. Clare, Zocchi, Alice
The High-Resolution Multi-Object Spectrograph (HRMOS) is a facility instrument that we plan to propose for the Very Large Telescope (VLT) of the European Southern Observatory (ESO), following the initial presentation at the VLT 2030 workshop held at
Externí odkaz:
http://arxiv.org/abs/2312.08270
Autor:
Nateghi, Hasti, Kacprzak, Glenn G., Nielsen, Nikole M., Murphy, Michael T., Churchill, Christopher W., Muzahid, Sowgat, Sameer, Charlton, Jane C.
The CGM hosts many physical processes with different kinematic signatures that affect galaxy evolution. We address the CGM-galaxy kinematic connection by quantifying the fraction of HI that is aligned with galaxy rotation with the equivalent width co
Externí odkaz:
http://arxiv.org/abs/2311.05164
Autor:
Nateghi, Hasti, Kacprzak, Glenn G., Nielsen, Nikole M., Sameer, Murphy, Michael T., Churchill, Christopher W., Charlton, Jane C.
The multiphase CGM hosts critical processes that affect galaxy evolution such as accretion and outflows. We searched for evidence of these phenomena by using the EW co-rotation fraction ($f_{\rm EWcorot}$) to study the kinematic connection between th
Externí odkaz:
http://arxiv.org/abs/2311.05165
Autor:
Chambers, Theodore, Vierhauser, Michael, Agrawal, Ankit, Murphy, Michael, Brauer, Jason Matthew, Purandare, Salil, Cohen, Myra B., Cleland-Huang, Jane
Small Unmanned Aerial Systems (sUAS) must meet rigorous safety standards when deployed in high-stress emergency response scenarios; however many reported accidents have involved humans in the loop. In this paper, we, therefore, present the HiFuzz tes
Externí odkaz:
http://arxiv.org/abs/2310.12058