Results 111 to 120 of about 7,111 (156)

The deep atmosphere of Jupiter. [PDF]

Nat Commun
Duer-Milner K.
europepmc   +1 more source

Quantum sensing for NASA science missions. [PDF]

EPJ Quantum Technol
Mercer CR, Montbach EN, Christe SD, Connerton RM, Podolski DA, Robinson MP, Perez MR.   +6 more
europepmc   +1 more source

An X-ray-emitting protocluster at z ≈ 5.7 reveals rapid structure growth. [PDF]

Nature
Bogdán Á, Schellenberger G, Li Q, Conselice CJ.   +3 more
europepmc   +1 more source

Generalizing the similitude approach for laboratory astrophysics through equivalence symmetries for the example of radiative waves. [PDF]

Sci Rep
Tranchant V, Charpentier N, Van Box Som L, Ciardi A, Falize É.   +4 more
europepmc   +1 more source

Dynamical dark energy in light of the DESI DR2 baryonic acoustic oscillations measurements. [PDF]

Nat Astron
Gu G, Wang X, Wang Y, Zhao GB, Pogosian L, Koyama K, Peacock JA, Cai Z, Cervantes-Cota JL, Ishak M, Shafieloo A, Zhao R, Ahlen S, Bianchi D, Brooks D, Claybaugh T, Cole S, de la Macorra A, de Mattia A, Doel P, Ferraro S, Forero-Romero JE, Gaztañaga E, Gontcho A Gontcho S, Gutierrez G, Hahn C, Howlett C, Kehoe R, Kirkby D, Kneib JP, Kremin A, Lahav O, Landriau M, Le Guillou L, Leauthaud A, Levi M, Manera M, Meisner A, Miquel R, Moustakas J, Muñoz-Gutiérrez A, Nadathur S, Newman JA, Palanque-Delabrouille N, Percival W, Prada F, Pérez-Ràfol I, Rossi G, Samushia L, Sanchez E, Schlegel D, Seo HJ, Sprayberry D, Tarlé G, Walther M, Weaver BA, Zarrouk P, Zhao C, Zhou R, Zou H.   +59 more
europepmc   +1 more source

Cryogenic Infrared Action Spectroscopy of [H₂NCO]⁺ and [H₂NCS]⁺, Protonated Forms of Interstellar HNCO and HNCS. [PDF]

J Phys Chem A
Gerlach M, Schneider NR, Petrić S, Kaur H, Changala PB, Redlich B, Brünken S.   +6 more
europepmc   +1 more source

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High-energy neutrino astrophysics

Nature Physics, 2016
The chargeless, weakly interacting neutrinos are ideal astronomical messengers as they travel through space without scattering, absorption or deflection. But this weak interaction also makes them notoriously difficult to detect, leading to neutrino observatories requiring large-scale detectors.
Francis Halzen, Halzen Francis
exaly   +2 more sources

High-Energy Astrophysics

Undergraduate Lecture Notes in Physics, 2022
Jorge Ernesto Horvath
exaly   +2 more sources

High-Energy Astrophysics

Science, 1994
Gamma ray line radiation, R. Ramaty and R. Lingenfelter gamma ray bursters, D. Hartmann gamma ray astronomy above 0.1TeV, D.J.Fegan cosmic ray observations at extreme energies, P. Sokolsky astrophysical neutrinos, T. Stanev AGN and galactic sites of cosmic ray origin, P.L. Biermann.
  +5 more sources

High Energy Astrophysics with INTEGRAL

Astrophysics and Space Science, 2001
INTEGRAL is an ESA mission scheduled to be launched in 2001. Its four coaligned instruments will allow observations of cosmic sources from a fraction of a keV to several MeV plus source monitoring in the optical band. INTEGRAL will be operated as a space observatory and an Announcement of Opportunity to the astronomical community at large will be ...
openaire   +1 more source