Zobrazeno 1 - 10
of 8 217
pro vyhledávání: '"Chakrabarty P"'
Autor:
Rathi, R., Sivakandan, M., Chakrabarty, D., Krishna, M. V. Sunil, Upadhayaya, A. K., Sarkhel, S.
Electrified Medium Scale Traveling Ionospheric Disturbances (EMSTIDs) is one of the prominent plasma structures that affect the propagation of high frequency radio waves. Overall, seasonal variation and propagation characteristics of the EMSTIDs are
Externí odkaz:
http://arxiv.org/abs/2410.08550
Autor:
Ray, Paul S., Roming, Peter W. A., Argan, Andrea, Arzoumanian, Zaven, Ballantyne, David R., Bogdanov, Slavko, Bonvicini, Valter, Brandt, Terri J., Bursa, Michal, Cackett, Edward M., Chakrabarty, Deepto, Christophersen, Marc, Coderre, Kathleen M., De Geronimo, Gianluigi, Del Monte, Ettore, DeRosa, Alessandra, Dietz, Harley R., Evangelista, Yuri, Feroci, Marco, Ford, Jeremy J., Froning, Cynthia, Fryer, Christopher L., Gendreau, Keith C., Goldstein, Adam, Gonzalez, Anthony H., Hartmann, Dieter, Hernanz, Margarita, Hutcheson, Anthony, Zand, Jean in `t, Jenke, Peter, Kennea, Jamie, Lloyd-Ronning, Nicole M., Maccarone, Thomas J., Maes, Dominic, Markwardt, Craig B., Michalska, Malgorzata, Okajima, Takashi, Patruno, Alessandro, Persyn, Steven C., Phillips, Mark L., Prescod-Weinstein, Chanda, Redfern, Jillian A., Remillard, Ronald A., Santangelo, Andrea, Schwendeman, Carl L., Sleator, Clio, Steiner, James, Strohmayer, Tod E., Svoboda, Jiri, Tenzer, Christoph, Thompson, Steven P., Warwick, Richard W., Watts, Anna L., Wilson-Hodge, Colleen A., Wu, Xin, Wulf, Eric A., Zampa, Gianluigi
We give an overview of the science objectives and mission design of the Spectroscopic Time-Resolving Observatory for Broadband Energy X-rays (STROBE-X) observatory, which has been proposed as a NASA probe-class (~$1.5B) mission in response to the Ast
Externí odkaz:
http://arxiv.org/abs/2410.08342
Autor:
Yogesh, Gopalswamy, N., Chakrabarty, D., Mostafavi, Parisa, Yashiro, Seiji, Srivastava, Nandita, Ofman, Leon
The abundance of helium ($A_{He}$) in the solar wind exhibits variations typically in the range from 2-5% with respect to solar cycle activity and solar wind velocity. However, there are instances where the observed $A_{He}$ is exceptionally low ($<$
Externí odkaz:
http://arxiv.org/abs/2410.04713
Autor:
Lu, Haotian, Yin, Ziang, Bhoumik, Partho, Banerjee, Sanmitra, Chakrabarty, Krishnendu, Gu, Jiaqi
Electronic-photonic computing systems have emerged as a promising platform for accelerating deep neural network (DNN) workloads. Major efforts have been focused on countering hardware non-idealities and boosting efficiency with various hardware/algor
Externí odkaz:
http://arxiv.org/abs/2410.01289
Autor:
Mylavarapu, Ganesh, Ghosh, Subrata, Hens, Chittaranjan, Chakrabarty, Indranil, Mitra, Subhadip
We show that the average of the maximum teleportation fidelities between all pairs of nodes in a large quantum repeater network is a measure of the resourcefulness of the network as a whole. We use simple Werner state-based models to characterise som
Externí odkaz:
http://arxiv.org/abs/2409.20304
The geo-effectiveness of Coronal Mass Ejections (CMEs) is a critical area of study in space weather, particularly in the lesser-explored domain of CME-CME interactions and their geomagnetic consequences. This study leverages the SWASTi framework to p
Externí odkaz:
http://arxiv.org/abs/2409.19943
Autor:
Maity, Dibyendu, Chakrabarty, Suman
The identification and classification of different phases of ice within molecular simulations is a challenging task due to the complex and varied phase space of ice, which includes numerous crystalline and amorphous forms. Traditional order parameter
Externí odkaz:
http://arxiv.org/abs/2409.19123
LLM-based applications are helping people write, and LLM-generated text is making its way into social media, journalism, and our classrooms. However, the differences between LLM-generated and human-written text remain unclear. To explore this, we hir
Externí odkaz:
http://arxiv.org/abs/2409.14509
Autor:
Chakrabarty, Deeparnab, Liao, Hang
We consider the problem of learning an unknown partition of an $n$ element universe using rank queries. Such queries take as input a subset of the universe and return the number of parts of the partition it intersects. We give a simple $O(n)$-query,
Externí odkaz:
http://arxiv.org/abs/2409.13092
Autor:
Dorsman, Bas, Salmi, Tuomo, Watts, Anna L., Ng, Mason, Kamath, Satish, Bobrikova, Anna, Poutanen, Juri, Loktev, Vladislav, Kini, Yves, Choudhury, Devarshi, Vinciguerra, Serena, Bogdanov, Slavko, Chakrabarty, Deepto
Pulse profile modelling (PPM) is a technique for inferring mass, radius and hotspot properties of millisecond pulsars. PPM is now regularly used for analysis of rotation-powered millisecond pulsars (RMPs) with data from the Neutron Star Interior Comp
Externí odkaz:
http://arxiv.org/abs/2409.07908