Zobrazeno 1 - 10
of 8 629
pro vyhledávání: '"Klingler A"'
The Aldous-Hoover Theorem concerns an infinite matrix of random variables whose distribution is invariant under finite permutations of rows and columns. It states that, up to equality in distribution, each random variable in the matrix can be express
Externí odkaz:
http://arxiv.org/abs/2411.12840
Autor:
Eyles-Ferris, R. A. J., Evans, P. A., Breeveld, A. A., Cenko, S. B., Dichiara, S., Kennea, J. A., Klingler, N. J., Kuin, N. P. M., Marshall, F. E., Oates, S. R., Page, M. J., Ronchini, S., Siegel, M. H., Tohuvavohu, A., Campana, S., D'Elia, V., Osborne, J. P., Page, K. L., De Pasquale, M., Troja, E.
The LIGO, Virgo and KAGRA gravitational wave observatories are currently undertaking their O4 observing run offering the opportunity to discover new electromagnetic counterparts to gravitational wave events. We examine the capability of the Neil Gehr
Externí odkaz:
http://arxiv.org/abs/2411.05072
Autor:
O'Connor, B., Pasham, D., Andreoni, I., Hare, J., Beniamini, P., Troja, E., Ricci, R., Dobie, D., Chakraborty, J., Ng, M., Klingler, N., Karambelkar, V., Rose, S., Schulze, S., Ryan, G., Dichiara, S., Monageng, I., Buckley, D., Hu, L., Srinivasaragavan, G., Bruni, G., Cabrera, T., Cenko, S. B., van Eerten, H., Freeburn, J., Hammerstein, E., Kasliwal, M., Kouveliotou, C., Kunnumkai, K., Leung, J. K., Lien, A., Palmese, A., Sakamoto, T.
We present the results of our multi-wavelength (X-ray to radio) follow-up campaign of the Einstein Probe transient EP240408a. The initial 10 s trigger displayed bright soft X-ray (0.5-4 keV) radiation with peak luminosity $L_\textrm{X} \gtrsim 10^{49
Externí odkaz:
http://arxiv.org/abs/2410.21622
Autor:
Gupta, Rahul, Ror, A. K., Pandey, S. B., Racusin, J., Moss, M., Aryan, A., Klingler, N., Castro-Tirado, A. J.
We have analyzed the prompt and afterglow characteristics of the intermediate luminosity burst ``GRB 210210A". Our prompt emission analysis indicates that GRB 210210A is among the softest long GRBs detected by the Swift-BAT. The time-integrated promp
Externí odkaz:
http://arxiv.org/abs/2409.04871
Is there an algorithm to determine attributes such as positivity or non-zeroness of linear recurrence sequences? This long-standing question is known as Skolem's problem. In this paper, we study the complexity of an equivalent problem, namely the (ge
Externí odkaz:
http://arxiv.org/abs/2404.15053
Autor:
Klingler, Andreas, Netzer, Tim
Convex optimization encompasses a wide range of optimization problems, containing many efficiently solvable subclasses. Interior point methods are currently the state-of-the-art approach for solving such problems, particularly effective for classes l
Externí odkaz:
http://arxiv.org/abs/2403.02095
We use Markov categories to develop generalizations of the theory of Markov chains and hidden Markov models in an abstract setting. This comprises characterizations of hidden Markov models in terms of local and global conditional independences as wel
Externí odkaz:
http://arxiv.org/abs/2401.14669
We study when the Picard group of smooth surfaces of degree $d\geq 5$ in $\mathbb{P}^3$ acquires extra classes. In particular we show that the so called exceptional components of the Noether-Lefschetz locus are not Zariski dense. This answers a 1991
Externí odkaz:
http://arxiv.org/abs/2312.11246
Autor:
Gagnon, Seth, Kargaltsev, Oleg, Klingler, Noel, Hare, Jeremy, Yang, Hui, Lange, Alexander, Eagle, Jordan
Publikováno v:
Volume 968, (2024) pg 67-80
We obtained a 108 ks Chandra X-ray Observatory (CXO) observation of PSR J1849-0001 and its pulsar wind nebula (PWN), coincident with the TeV source HESS J1849-000. By analyzing the new and archival CXO data, we resolved the pulsar from the PWN, explo
Externí odkaz:
http://arxiv.org/abs/2311.13677
Autor:
Safi-Harb, S., Burdge, K. B., Bodaghee, A., An, H., Guest, B., Hare, J., Hebbar, P., Ho, W. C. G., Kargaltsev, O., Kirmizibayrak, D., Klingler, N., Nynka, M., Reynolds, M. T., Sasaki, M., Sridhar, N., Vasilopoulos, G., Woods, T. E., Yang, H., Heinke, C., Kong, A., Li, J., MacMaster, A., Mallick, L., Treyturik, C., Tsuji, N., Binder, B., Braun, C., Chang, H. -K., Chatterjee, A., Ferrand, G., Holland-Ashford, T., Ng, C. -Y., Plotkin, R., Romani, R., Zhang, S.
Compact objects and supernova remnants provide nearby laboratories to probe the fate of stars after they die, and the way they impact, and are impacted by, their surrounding medium. The past five decades have significantly advanced our understanding
Externí odkaz:
http://arxiv.org/abs/2311.07673