Zobrazeno 71 - 80
of 980
pro vyhledávání: '"Chatterjee, Sourav"'
Autor:
Azadkia, Mona, Chatterjee, Sourav
We propose a coefficient of conditional dependence between two random variables $Y$ and $Z$ given a set of other variables $X_1,\ldots,X_p$, based on an i.i.d. sample. The coefficient has a long list of desirable properties, the most important of whi
Externí odkaz:
http://arxiv.org/abs/1910.12327
Autor:
Ye, Claire S., Fong, Wen-fai, Kremer, Kyle, Rodriguez, Carl L., Chatterjee, Sourav, Fragione, Giacomo, Rasio, Frederic A.
Publikováno v:
The Astrophysical Journal Letters, Volume 888, Issue 1, article id. L10, 13 pp. (2020)
The first detection of gravitational waves from a neutron star - neutron star (NS-NS) merger, GW170817, and the increasing number of observations of short gamma-ray bursts (SGRBs) have greatly motivated studies of the origins of NS-NS and neutron sta
Externí odkaz:
http://arxiv.org/abs/1910.10740
Autor:
Chatterjee, Sourav
The problem of completing a large low rank matrix using a subset of revealed entries has received much attention in the last ten years. The main result of this paper gives a necessary and sufficient condition, stated in the language of graph limit th
Externí odkaz:
http://arxiv.org/abs/1910.01079
Autor:
Chatterjee, Sourav
Is it possible to define a coefficient of correlation which is (a) as simple as the classical coefficients like Pearson's correlation or Spearman's correlation, and yet (b) consistently estimates some simple and interpretable measure of the degree of
Externí odkaz:
http://arxiv.org/abs/1909.10140
In astrometric binaries, the presence of a dark, unseen star can be inferred from the gravitational pull it induces on its luminous binary companion. While the orbit of such binaries can be characterized with precise astrometric measurements, constra
Externí odkaz:
http://arxiv.org/abs/1909.05606
Publikováno v:
In Journal of Energy Storage 15 November 2023 72 Part A
Publikováno v:
In Atmospheric Research November 2023 295
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Among the growing list of confirmed exoplanets, the number of planets identified in dense star clusters remains sparse. Previous analyses have suggested this may be due in part to dynamical interactions that unbind large fractions of planets from the
Externí odkaz:
http://arxiv.org/abs/1908.06978
As self-gravitating systems, dense star clusters exhibit a natural diffusion of energy from their innermost to outermost regions, which leads to a slow and steady contraction of the core until it ultimately collapses under gravity. However, in spite
Externí odkaz:
http://arxiv.org/abs/1907.12564