Results 171 to 180 of about 6,851 (202)

Cognitive Priming and Cognitive Training: Immediate and Far Transfer to Academic Skills in Children. [PDF]

Sci Rep, 2016
Wexler BE, Iseli M, Leon S, Zaggle W, Rush C, Goodman A, Esat Imal A, Bo E.   +7 more
europepmc   +1 more source

Stratified wind from a super-Eddington X-ray binary is slower than expected. [PDF]

Nature
XRISM collaboration.
europepmc   +1 more source

A COMPARISON OF SIMULATED JWST OBSERVATIONS DERIVED FROM EQUILIBRIUM AND NON-EQUILIBRIUM CHEMISTRY MODELS OF GIANT EXOPLANETS. [PDF]

Astrophys J, 2018
Blumenthal SD, Mandell AM, Hébrard E, Batalha NE, Cubillos PE, Rugheimer S, Wakeford HR.   +6 more
europepmc   +1 more source

An X-ray and Radio Study of the Varying Expansion Velocities in Tycho's Supernova Remnant. [PDF]

Astrophys J Lett, 2016
Williams BJ, Chomiuk L, Hewitt JW, Blondin JM, Borkowski KJ, Ghavamian P, Petre R, Reynolds SP.   +7 more
europepmc   +1 more source

Multiple Probe Measurements at Uranus Motivated by Spatial Variability. [PDF]

Space Sci Rev
Wong MH, Rowe-Gurney N, Markham S, Sayanagi KM.   +3 more
europepmc   +1 more source

A case for a binary black hole system revealed via quasi-periodic outflows. [PDF]

Sci Adv
Pasham DR, Tombesi F, Suková P, Zajaček M, Rakshit S, Coughlin E, Kosec P, Karas V, Masterson M, Mummery A, Holoien TW, Guolo M, Hinkle J, Ripperda B, Witzany V, Shappee B, Kara E, Horesh A, van Velzen S, Sfaradi I, Kaplan D, Burger N, Murphy T, Remillard R, Steiner JF, Wevers T, Arcodia R, Buchner J, Merloni A, Malyali A, Fabian A, Fausnaugh M, Daylan T, Altamirano D, Payne A, Ferraraa EC.   +35 more
europepmc   +1 more source

Long-Term Evolution of the Saturnian System. [PDF]

Space Sci Rev
Ćuk M, El Moutamid M, Lari G, Neveu M, Nimmo F, Noyelles B, Rhoden A, Saillenfest M.   +7 more
europepmc   +1 more source

The CRESST dark matter search [PDF]

Astroparticle Physics, 1999
We present first competitive results on WIMP dark matter using the phonon-light-detection technique. A particularly strong limit for WIMPs with coherent scattering results from selecting a region of the phonon-light plane corresponding to tungsten recoils.
Urmas Nagel, María Luisa Sarsa, Monica Sisti   +2 more
exaly   +14 more sources

Light dark matter in the light of CRESST-II

Journal of Cosmology and Astroparticle Physics, 2012
Recently the CRESST collaboration has published the long anticipated results of their direct Dark Matter (DM) detection experiment with a CaWO_4 target. The number of observed events exceeds known backgrounds at more than 4 sigma significance, and this excess could potentially be due to DM scattering.
Joachim Kopp, Thomas Schwetz, Jure Zupan
exaly   +5 more sources

CRESST cryogenic dark matter search

New Astronomy Reviews, 2005
Abstract The CRESST Phase II experiment at Gran Sasso is using 300 g scintillating CaWO 4 crystals as absorbers for direct WIMP (weakly interactive massive particles) detection. The phonon signal in the CaWO 4 crystal is registered in coincidence with the light signal, which is measured with a separate cryogenic light detector. The absorber crystal
Sergey Uchaikin
exaly   +3 more sources