Zobrazeno 1 - 10
of 26 963
pro vyhledávání: '"Pittman AS"'
Autor:
Pittman, Jason M.
Machine learning systems increasingly drive innovation across scientific fields and industry, yet challenges in compute overhead, specifically during inference, limit their scalability and sustainability. Responsible AI guardrails, essential for ensu
Externí odkaz:
http://arxiv.org/abs/2412.19241
Patients at a comprehensive cancer center who do not achieve cure or remission following standard treatments often become candidates for clinical trials. Patients who participate in a clinical trial may be suitable for other studies. A key factor inf
Externí odkaz:
http://arxiv.org/abs/2411.01394
Autor:
Thanathibodee, Thanawuth, Robinson, Connor, Calvet, Nuria, Espaillat, Catherine, Pittman, Caeley, Arulanantham, Nicole, France, Kevin, Günther, Hans Moritz, Chang, Seok-Jun, Schneider, P. Christian
The C IV doublet in the UV has long been associated with accretion in T Tauri stars. However, it is still unclear where and how the lines are formed. Here, we present a new C IV line model based on the currently available accretion shock and accretio
Externí odkaz:
http://arxiv.org/abs/2409.10361
Autor:
Espaillat, C. C., Thanathibodee, T., Zhu, Z., Rabago, I., Wendeborn, J., Calvet, N., Zamudio-Ruvalcaba, L., Volz, M., Pittman, C., McClure, M., Babb, J. F., Franco-Hernandez, R., Macias, E., Reynolds, M., Yan, P. -G.
Here we report the detection of dust depletion in a misaligned inner disk around UX Tau A using JWST MIRI spectra. Mid-infrared (MIR) continuum "seesaw" variability was detected in this disk by Spitzer and attributed to variable shadows cast on the o
Externí odkaz:
http://arxiv.org/abs/2409.03702
Autor:
Wendeborn, John, Espaillat, Catherine C., Thanathibodee, Thanawuth, Robinson, Connor E., Pittman, Caeley V., Calvet, Nuria, Muzerolle, James, Walter, Fredrick M., Eisloffel, Jochen, Fiorellino, Eleonora, Manara, Carlo F., Kospal, Agnes, Abraham, Peter, Claes, Rik, Rigliaco, Elisabetta, Venuti, Laura, Campbell-White, Justyn, McGinnis, Pauline, Gangi, Manuele, Mauco, Karina, Gameiro, Filipe, Frasca, Antonio, Guo, Zhen
Classical T Tauri Stars (CTTSs) are highly variable stars that possess gas- and dust-rich disks from which planets form. Much of their variability is driven by mass accretion from the surrounding disk, a process that is still not entirely understood.
Externí odkaz:
http://arxiv.org/abs/2408.04465
Autor:
Pittman, Jason M.
Contemporary artificial intelligence systems are pivotal in enhancing human efficiency and safety across various domains. One such domain is autonomous systems, especially in automotive and defense use cases. Artificial intelligence brings learning a
Externí odkaz:
http://arxiv.org/abs/2407.14975
Autor:
Ajmani, Leah Hope, Foriest, Jasmine C, Taylor, Jordan, Pittman, Kyle, Gilbert, Sarah, Devito, Michael Ann
Social computing scholars have long known that people do not interact with knowledge in straightforward ways, especially in digital environments. While policies around knowledge are essential for targeting misinformation, they are value-laden; in cho
Externí odkaz:
http://arxiv.org/abs/2407.03477
Autor:
Wendeborn, John, Espaillat, Catherine C., Thanathibodee, Thanawuth, Robinson, Connor E., Pittman, Caeley V., Calvet, Nuria, Kóspál, Ágnes, Grankin, Konstantin N., Walter, Fredrick M., Guo, Zhen, Eislöffel, Jochen
Classical T Tauri Stars (CTTSs) are young, low-mass stars which accrete material from their surrounding protoplanetary disk. To better understand accretion variability, we conducted a multi-epoch, multi-wavelength photometric monitoring campaign of f
Externí odkaz:
http://arxiv.org/abs/2405.21071
Autor:
Wendeborn, John, Espaillat, Catherine C., Lopez, Sophia, Thanathibodee, Thanawuth, Robinson, Connor E., Pittman, Caeley V., Calvet, Nuria, Flors, Nicole, Walter, Fredrick M., Kóspál, Ágnes, Grankin, Konstantin N., Mendigutía, Ignacio, Günther, Hans Moritz, Eislöffel, Jochen, Guo, Zhen, France, Kevin, Fiorellino, Eleonora, Fischer, William J., Ábrahám, Péter, Herczeg, Gregory J.
The Classical T Tauri Star (CTTS) stage is a critical phase of the star and planet formation process. In an effort to better understand the mass accretion process, which can dictate further stellar evolution and planet formation, a multi-epoch, multi
Externí odkaz:
http://arxiv.org/abs/2405.21038
Recent work by Mi\v{c}uda et al. (arXiv:1206.2852v1) suggests that pairing noiseless amplification with noiseless attenuation can conditionally suppress loss terms in the direct transmission of quantum states. Here we extend this work to entangled st
Externí odkaz:
http://arxiv.org/abs/2405.00510