Zobrazeno 1 - 10
of 50 506
pro vyhledávání: '"P, Rice"'
Autor:
Leahy, Ian A., Rice, Anthony D., Nelson, Jocienne N., Ness, Herve, van Schilfgaarde, Mark, Pan, Wei, Alberi, Kirstin
Low carrier densities in topological semimetals (TSMs) enable the exploration of novel magnetotransport in the quantum limit (QL). Reports consistent with 3D quasi-quantum Hall effect (QQHE) have repositioned TSMs as promising platforms for exploring
Externí odkaz:
http://arxiv.org/abs/2412.05273
We present a pattern emerging from stellar obliquity measurements in single-star systems: planets with high planet-to-star mass ratios ($M_{\rm p}/M{_*}$$>$ $2\times10^{-3}$) -- such as super-Jupiters, brown dwarf companions, and M-dwarfs hosting Jup
Externí odkaz:
http://arxiv.org/abs/2412.04438
Autor:
Pinto, Marcelo Tala, Jordán, Andrés, Acuña, Lorena, Jones, Matías, Brahm, Rafael, Reinarz, Yared, Eberhardt, Jan, Espinoza, Néstor, Henning, Thomas, Hobson, Melissa, Rojas, Felipe, Schlecker, Martin, Trifonov, Trifon, Bakos, Gaspar, Boyle, Gavin, Csubry, Zoltan, Hartmann, Joel, Knepper, Benjamin, Kreidberg, Laura, Suc, Vincent, Teske, Johanna, Butler, R. Paul, Crane, Jeffrey, Schectman, Steve, Thompson, Ian, Osip, Dave, Ricker, George, Collins, Karen A., Watkins, Cristilyn N., Bieryla, Allyson, Stockdale, Chris, Wang, Gavin, Zambelli, Roberto, Seager, Sara, Winn, Joshua, Rose, Mark E., Rice, Malena, Essack, Zahra
We report the discovery and characterization of three new transiting giant planets orbiting TOI-6628, TOI-3837 and TOI-5027, and one new warm sub-Saturn orbiting TOI-2328, whose transits events were detected in the lightcurves of the Transiting Exopl
Externí odkaz:
http://arxiv.org/abs/2412.02069
Many of the world's languages have insufficient data to train high-performing general neural machine translation (NMT) models, let alone domain-specific models, and often the only available parallel data are small amounts of religious texts. Hence, d
Externí odkaz:
http://arxiv.org/abs/2412.00966
Autor:
Liang, Haoming, Chen, Li-Jen, Fuselier, Stephen A., Gomez, Roman G., Burkholder, Brandon, Bessho, Naoki, Gurram, Harsha, Rice, Rachel C., Shuster, Jason, Ardakani, Akhtar S.
We report Magnetospheric Multiscale observations of oxygen ions (O+) during a coronal mass ejection in April 2023 when the solar wind was sub-Alfv\'enic and Alfv\'en wings formed. For the first time, O+ characteristics are studied at the contact regi
Externí odkaz:
http://arxiv.org/abs/2410.21172
This paper introduces the Bayesian Confidence Estimator (BACON) for deep neural networks. Current practice of interpreting Softmax values in the output layer as probabilities of outcomes is prone to extreme predictions of class probability. In this w
Externí odkaz:
http://arxiv.org/abs/2410.12604
One of the most promising techniques for detecting ultra-high energy neutrinos involves the use of radio antennas to observe the 10-1000 MHz radiation generated by the showers that neutrinos induce in large volumes of ice. The expected neutrino detec
Externí odkaz:
http://arxiv.org/abs/2410.08615
Autor:
Michaux, Jonathan, Isaacson, Seth, Adu, Challen Enninful, Li, Adam, Swayampakula, Rahul Kashyap, Ewen, Parker, Rice, Sean, Skinner, Katherine A., Vasudevan, Ram
Neural Radiance Fields and Gaussian Splatting have transformed the field of computer vision by enabling photo-realistic representation of complex scenes. Despite this success, they have seen only limited use in real-world robotics tasks such as traje
Externí odkaz:
http://arxiv.org/abs/2409.16915
Autor:
Harada, Caleb K., Dressing, Courtney D., Kane, Stephen R., Blunt, Sarah, Dietrich, Jamie, Hinkel, Natalie R., Li, Zhexing, Mamajek, Eric, Rice, Malena, Tuchow, Noah W., Turtelboom, Emma V., Wittenmyer, Robert A.
Future large, space-based observatories with starlight suppression technology, e.g., the Habitable Worlds Observatory (HWO), will directly image and characterize nearby Earth-like exoplanets. Prior limits on planet masses and system architectures fro
Externí odkaz:
http://arxiv.org/abs/2409.10679
Autor:
Xiao, Guang-Yao, Feng, Fabo, Shectman, Stephen A., Tinney, C. G., Teske, Johanna K., Carter, B. D., Jones, H. R. A., Wittenmyer, Robert A., Díaz, Matías R., Crane, Jeffrey D., Wang, Sharon X., Bailey, J., O'Toole, S. J., Feinstein, Adina D., Rice, Malena, Essack, Zahra, Montet, Benjamin T., Shporer, Avi, Butler, R. Paul
Giant planets on long period orbits around the nearest stars are among the easiest to directly image. Unfortunately these planets are difficult to fully constrain by indirect methods, e.g., transit and radial velocity (RV). In this study, we present
Externí odkaz:
http://arxiv.org/abs/2409.08067