Results 281 to 290 of about 401,472 (327)

Inverse-designed gyrotropic scatterers for non-reciprocal analog computing. [PDF]

Nanophotonics
Hadjiantoni N, Goh H, Hanham SM, Navarro-Cía M, Alù A.   +4 more
europepmc   +1 more source

Testing T2K's Bayesian constraints with priors in alternate parameterisations. [PDF]

Eur Phys J C Part Fields
T2K Collaboration.
europepmc   +1 more source

Performance evaluation of the ACTIVE 7 MAX benchtop preclinical PET scanner in accordance with the NEMA NU 4-2008 standard. [PDF]

EJNMMI Phys
Wang H, Wang K, Yuan Z, Li C, Liao R, Hou Y, Hua J, Tang Y, Ruan Q, Han D, Jiang J.   +10 more
europepmc   +1 more source

Textual interpretation of transient image classifications from large language models. [PDF]

Nat Astron
Stoppa F, Bulmus T, Bloemen S, Smartt SJ, Groot PJ, Vreeswijk P, Smith KW.   +6 more
europepmc   +1 more source

Discs no more: the morphology of low-mass simulated galaxies in FIREbox. [PDF]

Mon Not R Astron Soc
Benavides JA, Sales LV, Wetzel A, Moreno J, Feldmann R, Mercado FJ, Bullock JS, Hopkins PF, Faucher-Giguère CA, Stern J, Wheeler C, Kereš D.   +11 more
europepmc   +1 more source

Magnetic star-planet interaction in the young exoplanet system DS Tucanae Ab

Santos Ld, Owen J, Duvvuri G, Loyd ROP, Vidotto A, Presa A, Bourrier V, King G, Airapetian V, Ehrenreich D, France K, Lendl M, Lothringer J, Nielsen L.   +13 more
europepmc   +1 more source

High-energy astronomy from a lunar base.

, 1988
P. Gorenstein
openalex   +1 more source

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High energy neutrino astronomy

Nature, 1978
The possibility of doing point source neutrino astronomy is discussed. Probable sources include galactic nuclei, Seyferts, quasars, radio galaxies, pulsars and supernovae.
David Eichler, David N. Schramm
openaire   +1 more source

High-energy Gamma-ray Astronomy

Nature, 1970
Gamma-ray astronomy above 10 MeV is difficult from the experimental point of view, but promising data are beginning to appear, as this survey progress report shows.
openaire   +2 more sources

High energy neutrino astronomy

Nuclear Physics B - Proceedings Supplements, 2000
Abstract The sky survey with high energy neutrinos is complementary to the survey with photons. The method of the detection of ν μ is described and the expected sensitivity to high energy neutrino sources with a kilometer-scale detector is estimated. The status of the current under-water(ice) detector projects is reported.
openaire   +1 more source