Results 141 to 150 of about 375 (170)

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

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

Nature
XRISM collaboration.
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.
M Bruckmayer, F Von Feilitzsch, R Keeling   +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   +2 more
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
C Cozzini, G Angloher, F Von Feilitzsch   +2 more
exaly   +3 more sources

Toward a consistent picture for CRESST, CoGeNT, and DAMA

Physical Review D, 2012
11 pages, 7 ...
Dan Hooper
exaly   +4 more sources

The CRESST dark matter experiment: status and perspectives

Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 2000
Abstract The CRESST experiment in its first phase is using sapphire detectors with tungsten phase transition thermometers to search for dark matter WIMPs. At present four 262 g detectors are performing first measurements under low background conditions. Detector performance as well as preliminary results from the background runs are presented.
M Sisti, F V Feilitzsch, R Keeling
exaly   +2 more sources