Zobrazeno 1 - 10
of 2 231
pro vyhledávání: '"Levine, Benjamin"'
Autor:
Cloonan, Aidan P., Khullar, Gourav, Napier, Kate A., Gladders, Michael D., Dahle, Håkon, Rosener, Riley, Sullivan Jr., Jamar, Bayliss, Matthew B., Chicoine, Nathalie, Escapa, Isaiah, Garza, Diego, Garza, Josh, Glusman, Rowen, Gozman, Katya, Horwath, Gabriela, Kisare, Andi, Levine, Benjamin C., Liang, Olina, Malagon, Natalie, Martinez, Michael N., Masegian, Alexandra, Acuña, Owen S. Matthews, Mork, Simon D., Niu, Kunwanhui, Owens, M. Riley, Pan, Yue, Rigby, Jane R., Sharon, Keren, Sierra, Isaac, Stark, Antony A., Sukay, Ezra, Tamargo-Arizmendi, Marcos, Tavangar, Kiyan, Teixeira, Raul, Tsiane, Kabelo, Wagner, Grace, Zaborowski, Erik A., Zhang, Yunchong, Zhao, Megan
Wide-separation lensed quasars (WSLQs) are a rare class of strongly lensed quasars, magnified by foreground massive galaxy clusters, with typically large magnifications of the multiple quasar images. They are a relatively unexplored opportunity for d
Externí odkaz:
http://arxiv.org/abs/2408.03379
The exponential scaling of complete active space (CAS) and full configuration interaction (CI) calculations limits the ability of quantum chemists to simulate the electronic structures of strongly correlated systems. Herein, we present corner hierarc
Externí odkaz:
http://arxiv.org/abs/2407.21134
Autor:
Liang, Fangchun, Levine, Benjamin G.
The Ehrenfest with collapse-to-a-block (TAB) molecular dynamics approach was recently introduced to allow accurate simulation of nonadiabatic dynamics on many electronic states. Previous benchmarking work has demonstrated it to be highly accurate for
Externí odkaz:
http://arxiv.org/abs/2407.17652
Autor:
Mehmood, Arshad, Silfies, Myles C., Durden, Andrew S., Allison, Thomas K., Levine, Benjamin G.
Transient absorption spectroscopy (TAS) is among the most common ultrafast photochemical experiments, but its interpretation remains challenging. In this work, we present an efficient and robust method for simulating TAS signals from first principles
Externí odkaz:
http://arxiv.org/abs/2404.16568
Autor:
Sowa, Jakub K., Cadena, Danielle M., Mehmood, Arshad, Levine, Benjamin G., Roberts, Sean T., Rossky, Peter J.
Publikováno v:
J. Phys. Chem. C 2024, 128, 21, 8724-8731
Surfaces of colloidal nanocrystals are frequently passivated with carboxylate ligands which exert significant effects on their optoelectronic properties and chemical stability. Experimentally, binding geometries of such ligands are typically investig
Externí odkaz:
http://arxiv.org/abs/2403.18779
Autor:
Mork, Simon D., Gladders, Michael D., Khullar, Gourav, Sharon, Keren, Chicoine, Nathalie, Cloonan, Aidan P., Dahle, Håkon, Garza, Diego, Glusman, Rowen, Gozman, Katya, Horwath, Gabriela, Levine, Benjamin C., Liang, Olina, Mahronic, Daniel, Manwadkar, Viraj, Martinez, Michael N., Masegian, Alexandra, Acuña, Owen S. Matthews, Merz, Kaiya, Pan, Yue, Sanchez, Jorge A., Sierra, Isaac, Stein, Daniel J. Kavin, Sukay, Ezra, Tamargo-Arizmendi, Marcos, Tavangar, Kiyan, Tu, Ruoyang, Wagner, Grace, Zaborowski, Erik A., Zhang, Yunchong
We compute parametric measurements of the Einstein-radius-enclosed total mass for 177 cluster-scale strong gravitational lenses identified by the ChicagO Optically-selected Lenses Located At the Margins of Public Surveys (COOL-LAMPS) collaboration wi
Externí odkaz:
http://arxiv.org/abs/2401.08575
Computer simulation has long been an essential partner of ultrafast experiments, allowing the assignment of microscopic mechanistic detail to low-dimensional spectroscopic data. However, the ability of theory to make a priori predictions of ultrafast
Externí odkaz:
http://arxiv.org/abs/2401.08069
Autor:
Silfies, Myles C., Mehmood, Arshad, Kowzan, Grzegorz, Hohenstein, Edward G., Levine, Benjamin G., Allison, Thomas K.
Publikováno v:
J. Chem. Phys. 159, 104304 (2023)
Salicylidenaniline (SA) is an archetypal system for excited-state intramolecular proton transfer (ESIPT) in non-planar systems. Multiple channels for relaxation involving both the keto and enol forms have been proposed after excitation to S$_1$ with
Externí odkaz:
http://arxiv.org/abs/2306.05645
Autor:
Rojas, Karina, Collett, Thomas E., Ballard, Daniel, Magee, Mark R., Birrer, Simon, Buckley-Geer., Elizabeth, Chan, James H. H., Clément, Benjamin, Diego, José M., Gentile, Fabrizio, González, Jimena, Joseph, Rémy, Mastache, Jorge, Schuldt, Stefan, Tortora, Crescenzo, Verdugo, Tomás, Verma, Aprajita, Daylan, Tansu, Millon, Martin, Jackson, Neal, Dye, Simon, Melo, Alejandra, Mahler, Guillaume, Ogando, Ricardo L. C., Courbin, Frédéric, Fritz, Alexander, Herle, Aniruddh, Barroso, Javier A. Acevedo, Cañameras, Raoul, Cornen, Claude, Dhanasingham, Birendra, Glazebrook, Karl, Martinez, Michael N., Ryczanowski, Dan, Savary, Elodie, Góis-Silva, Filipe, Ureña-López, L. Arturo, Wiesner, Matthew P., Wilde, Joshua, Calçada, Gabriel Valim, Cabanac, Rémi, Pan, Yue, Sierra, Isaac, Despali, Giulia, Cavalcante-Gomes, Micaele V., Macmillan, Christine, Maresca, Jacob, Grudskaia, Aleksandra, O'Donnell, Jackson H., Paic, Eric, Niemiec, Anna, de la Bella, Lucia F., Bromley, Jane, Williams, Devon M., More, Anupreeta, Levine, Benjamin C.
We investigate the ability of human 'expert' classifiers to identify strong gravitational lens candidates in Dark Energy Survey like imaging. We recruited a total of 55 people that completed more than 25$\%$ of the project. During the classification
Externí odkaz:
http://arxiv.org/abs/2301.03670
Autor:
Zhang, Yunchong, Manwadkar, Viraj, Gladders, Michael D., Khullar, Gourav, Dahle, Håkon, Napier, Kate A., Mahler, Guillaume, Sharon, Keren, Acuña, Owen S. Matthews, Ashmead, Finian, Cerny, William, Gonzàlez, Juan Remolina, Gozman, Katya, Levine, Benjamin C., Marohnic, Daniel, Martinez, Michael N., Merz, Kaiya, Pan, Yue, Sanchez, Jorge A., Sierra, Isaac, Sisco, Emily E., Sukay, Ezra, Tavangar, Kiyan, Zaborowski, Erik
Publikováno v:
ApJ, 950, 58 (2023)
We report the discovery of five bright strong gravitationally lensed galaxies at $3 < z < 4$: COOLJ0101$+$2055 ($z = 3.459$), COOLJ0104$-$0757 ($z = 3.480$), COOLJ0145$+$1018 ($z = 3.310$), COOLJ0516$-$2208 ($z = 3.549$), and COOLJ1356$+$0339 ($z = 3
Externí odkaz:
http://arxiv.org/abs/2212.06902