Zobrazeno 1 - 10
of 7 032
pro vyhledávání: '"Ben, W."'
Autor:
French, Jenni R., Casewell, Sarah L., Amaro, Rachael C., Lothringer, Joshua D., Mayorga, L. C., Littlefair, Stuart P., Lew, Ben W. P., Zhou, Yifan, Apai, Daniel, Marley, Mark S., Parmentier, Vivien, Tan, Xianyu
Due to their short orbital periods and relatively high flux ratios, irradiated brown dwarfs in binaries with white dwarfs offer better opportunities to study irradiated atmospheres than hot Jupiters, which have lower planet-to-star flux ratios. WD103
Externí odkaz:
http://arxiv.org/abs/2409.06874
Autor:
Reichardt, Ben W., Aasen, David, Chao, Rui, Chernoguzov, Alex, van Dam, Wim, Gaebler, John P., Gresh, Dan, Lucchetti, Dominic, Mills, Michael, Moses, Steven A., Neyenhuis, Brian, Paetznick, Adam, Paz, Andres, Siegfried, Peter E., da Silva, Marcus P., Svore, Krysta M., Wang, Zhenghan, Zanner, Matt
A critical milestone for quantum computers is to demonstrate fault-tolerant computation that outperforms computation on physical qubits. The tesseract subsystem color code protects four logical qubits in 16 physical qubits, to distance four. Using th
Externí odkaz:
http://arxiv.org/abs/2409.04628
Autor:
Carter, Aarynn L., Bowens-Rubin, Rachel, Calissendorff, Per, Kammerer, Jens, Li, Yiting, Meyer, Michael R., Booth, Mark, Factor, Samuel M., Franson, Kyle, Gaidos, Eric, Leisenring, Jarron M., Lew, Ben W. P., Martinez, Raquel A., Rebollido, Isabel, Rickman, Emily, Sutlieff, Ben J., Ward-Duong, Kimberly, Zhang, Zhoujian
We advocate for a large scale imaging survey of nearby young moving groups and star-forming regions to directly detect exoplanets over an unexplored range of masses, ages and orbits. Discovered objects will be identified early enough in JWST's lifeti
Externí odkaz:
http://arxiv.org/abs/2408.07722
Autor:
Hainline, Kevin N., D'Eugenio, Francesco, Sun, Fengwu, Helton, Jakob M., Miles, Brittany E., Marley, Mark S., Lew, Ben W. P., Leisenring, Jarron M., Bunker, Andrew J., Cargile, Phillip A., Carniani, Stefano, Eisenstein, Daniel J., Juodzbalis, Ignas, Johnson, Benjamin D., Robertson, Brant, Tacchella, Sandro, Williams, Christina C., Willmer, Christopher N. A.
Large area observations of extragalactic deep fields with the James Webb Space Telescope (JWST) have provided a wealth of candidate low-mass L- and T-class brown dwarfs. The existence of these sources, which are at derived distances of hundreds of pa
Externí odkaz:
http://arxiv.org/abs/2407.08781
Autor:
Amaro, Rachael C., Apai, Daniel, Lew, Ben W. P., Zhou, Yifan, Lothringer, Joshua D., Casewell, Sarah L., Tan, Xianyu, Barman, Travis, Marley, Mark S., Mayorga, L. C., Parmentier, Vivien
Brown dwarfs in ultra-short period orbits around white dwarfs offer a unique opportunity to study the properties of tidally-locked, fast rotating (1-3 hr), and highly-irradiated atmospheres. Here, we present phase-resolved spectrophotometry of the wh
Externí odkaz:
http://arxiv.org/abs/2404.08087
Autor:
Lew, Ben W. P., Roellig, Thomas, Batalha, Natasha E., Line, Michael, Greene, Thomas, Murkherjee, Sagnick, Freedman, Richard, Meyer, Michael, Beichman, Charles, De Oliveira, Catarina Alves, De Furio, Matthew, Johnstone, Doug, Greenbaum, Alexandra Z., Marley, Mark, Fortney, Jonathan J., Young, Erick T., Leisenring, Jarron, Boyer, Martha, Hodapp, Klaus, Misselt, Karl, Stansberry, John, Rieke, Marcia
The launch of the James Webb Space Telescope (JWST) marks a pivotal moment for precise atmospheric characterization of Y dwarfs, the coldest brown dwarf spectral type. In this study, we leverage moderate spectral resolution observations (R $\sim$ 270
Externí odkaz:
http://arxiv.org/abs/2402.05900
Autor:
Petrus, Simon, Whiteford, Niall, Patapis, Polychronis, Biller, Beth A., Skemer, Andrew, Hinkley, Sasha, Suárez, Genaro, Lueber, Anna, Palma-Bifani, Paulina, Stone, Jordan M., Vos, Johanna M., Morley, Caroline V., Tremblin, Pascal, Charnay, Benjamin, Helling, Christiane, Miles, Brittany E., Carter, Aarynn L., Wang, Jason J., Janson, Markus, Gonzales, Eileen C., Sutlieff, Ben, Hoch, Kielan K. W., Bonnefoy, Mickaël, Chauvin, Gaël, Absil, Olivier, Balmer, William O., Boccaletti, Anthony, Bonavita, Mariangela, Booth, Mark, Bowler, Brendan P., Briesemeister, Zackery W., Bryan, Marta L., Calissendorff, Per, Cantalloube, Faustine, Chen, Christine H., Choquet, Elodie, Christiaens, Valentin, Cugno, Gabriele, Currie, Thayne, Danielski, Camilla, De Furio, Matthew, Dupuy, Trent J., Factor, Samuel M., Faherty, Jacqueline K., Fitzgerald, Michael P., Fortney, Jonathan J., Franson, Kyle, Girard, Julien H., Grady, Carol A., Henning, Thomas, Hines, Dean C., Hood, Callie E., Howe, Alex R., Kalas, Paul, Kammerer, Jens, Kennedy, Grant M., Kenworthy, Matthew A., Kervella, Pierre, Kim, Minjae, Kitzmann, Daniel, Kraus, Adam L., Kuzuhara, Masayuki, Lagage, Pierre-Olivier, Lagrange, Anne-Marie, Lawson, Kellen, Lazzoni, Cecilia, Leisenring, Jarron M., Lew, Ben W. P., Liu, Michael C., Liu, Pengyu, Llop-Sayson, Jorge, Lloyd, James P., Macintosh, Bruce, Mâlin, Mathilde, Manjavacas, Elena, Marino, Sebastián, Marley, Mark S., Marois, Christian, Martinez, Raquel A., Matthews, Elisabeth C., Matthews, Brenda C., Mawet, Dimitri, Mazoyer, Johan, McElwain, Michael W., Metchev, Stanimir, Meyer, Michael R., Millar-Blanchaer, Maxwell A., Mollière, Paul, Moran, Sarah E., Mukherjee, Sagnick, Pantin, Eric, Perrin, Marshall D., Pueyo, Laurent, Quanz, Sascha P., Quirrenbach, Andreas, Ray, Shrishmoy, Rebollido, Isabel, Redai, Jea Adams, Ren, Bin B., Rickman, Emily, Sallum, Steph, Samland, Matthias, Sargent, Benjamin, Schlieder, Joshua E., Stapelfeldt, Karl R., Tamura, Motohide, Tan, Xianyu, Theissen, Christopher A., Uyama, Taichi, Vasist, Malavika, Vigan, Arthur, Wagner, Kevin, Ward-Duong, Kimberly, Wolff, Schuyler G., Worthen, Kadin, Wyatt, Mark C., Ygouf, Marie, Zurlo, Alice, Zhang, Xi, Zhang, Keming, Zhan, Zhoujian, Zhou, Yifan
The unprecedented medium-resolution (R~1500-3500) near- and mid-infrared (1-18um) spectrum provided by JWST for the young (140+/-20Myr) low-mass (12-20MJup) L-T transition (L7) companion VHS1256b gives access to a catalogue of molecular absorptions.
Externí odkaz:
http://arxiv.org/abs/2312.03852
Magnetars are highly-magnetised rotating neutron stars that are predominantly observed as high-energy sources. Six of this class of neutron star are known to also emit radio emission, and magnetars are, thus, a favoured model for the origin for at le
Externí odkaz:
http://arxiv.org/abs/2311.13762
Autor:
Kundu, Sourav, Reichardt, Ben W.
The tetron architecture is a promising candidate for topological quantum computation. Each tetron Majorana island has four Majorana zero modes, and possible measurements are constrained to span zero or two Majoranas per tetron. Such measurements are
Externí odkaz:
http://arxiv.org/abs/2311.01779