Zobrazeno 1 - 10
of 50 233
pro vyhledávání: '"P, Rice"'
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
While astronomers often assume that exoplanets are perfect spheres when analyzing observations, the subset of these distant worlds that are subject to strong tidal forces and/or rapid rotations are expected to be distinctly ellipsoidal or even triaxi
Externí odkaz:
http://arxiv.org/abs/2409.00167
Autor:
Wang, Xian-Yu, Rice, Malena, Wang, Songhu, Kanodia, Shubham, Dai, Fei, Logsdon, Sarah E., Schweiker, Heidi, Teske, Johanna K., Butler, R. Paul, Crane, Jeffrey D., Shectman, Stephen A., Quinn, Samuel N., Kostov, Veselin B., Osborn, Hugh P., Goeke, Robert F., Eastman, Jason D., Shporer, Avi, Rapetti, David, Collins, Karen A., Watkins, Cristilyn, Relles, Howard M., Ricker, George R., Seager, Sara, Winn, Joshua N., Jenkins, Jon M.
The stellar obliquity distribution of warm-Jupiter systems is crucial for constraining the dynamical history of Jovian exoplanets, as the warm Jupiters' tidal detachment likely preserves their primordial obliquity. However, the sample size of warm-Ju
Externí odkaz:
http://arxiv.org/abs/2408.10038
Autor:
Li, Yanzeng, Valenton, Emmanuel, Nagasamudram, Spoorthi, Parker, John, Perez, Marcos, Manna, Uttam, Biswas, Mahua, Rice, Stuart A., Scherer, Norbert F.
Optical trapping is having ever-increasing impact in science $-$ particularly biophysics, photonics and most recently in quantum optomechanics $-$ owing to its superior capability for manipulating nanoscale structures and materials. However, essentia
Externí odkaz:
http://arxiv.org/abs/2408.09707
Brown dwarfs occupy a middle ground in mass space between gaseous giant planets and ultra-cool dwarf stars, and the characterisation of their orbital orientations may shed light on how these neighbouring objects form. We present an analysis of the Ro
Externí odkaz:
http://arxiv.org/abs/2408.00725