Results 51 to 60 of about 375 (170)

The CRESST dark matter search

open access: yesJournal of Physics: Conference Series, 2008
CRESST is a WIMP dark matter search using scintillating CaWO4 cryogenic detectors with active background suppression. First results obtained in the commissioning run are presented.
W Seidel   +40 more
openaire   +1 more source

A likelihood framework for cryogenic scintillating calorimeters used in the CRESST dark matter search

open access: yesEuropean Physical Journal C: Particles and Fields
Cryogenic scintillating calorimeters are ultra- sensitive particle detectors for rare event searches, particularly for the search for dark matter and the measurement of neutrino properties.
CRESST Collaboration   +59 more
doaj   +1 more source

Results on MeV-scale dark matter from a gram-scale cryogenic calorimeter operated above ground

open access: yesEuropean Physical Journal C: Particles and Fields, 2017
Models for light dark matter particles with masses below 1 GeV/c $$^2$$ 2 are a natural and well-motivated alternative to so-far unobserved weakly interacting massive particles.
G. Angloher   +47 more
doaj   +1 more source

The Complex X-Ray Obscuration Environment in the Radio-loud Type 2 Quasar 3C 223

open access: yesThe Astrophysical Journal, 2023
3C 223 is a radio-loud, Type 2 quasar at z = 0.1365 with an intriguing X-ray Multi-mirror Mission (XMM)-Newton spectrum that implicated it as a rare, Compton-thick ( N _H ≳ 1.25 × 10 ^24 cm ^−2 ) active galactic nucleus (AGN). We obtained contemporaneous
Stephanie M. LaMassa   +6 more
doaj   +1 more source

Discrimination, Harassment, and Bias in Higher Education: Disaggregating the Experiences of LGBTQ+ Students

open access: yesNew Directions for Higher Education, Volume 2025, Issue 210, Page 37-46, Summer 2025.
ABSTRACT Queer and transgender students in higher education experience elevated rates of discrimination, bias, and harassment, which affect their well‐being and academic outcomes. These experiences differ across various identities within these communities, necessitating a nuanced approach to understanding their distinct challenges.
John Yang, Ellen Bara Stolzenberg
wiley   +1 more source

Erratum to: Geant4-based electromagnetic background model for the CRESST dark matter experiment

open access: yesEuropean Physical Journal C: Particles and Fields, 2019
The original version of this article unfortunately contains mistakes.
A. H. Abdelhameed   +52 more
doaj   +1 more source

Recurrent Novae — A Review

open access: yesActa Polytechnica CTU Proceedings, 2015
In recent years, recurrent nova eruptions are often observed very intensely in wide range of wavelengths from radio to optical to X-rays. Here I present selected highlights from recent multi-wavelength observations. The enigma of T Pyx is at the heart of
K. Mukai
doaj   +1 more source

Rapid growth of a carbonate island over the last millennium

open access: yesSedimentology, Volume 71, Issue 7, Page 2119-2143, December 2024.
Abstract Low‐lying islands in tropical regions are vulnerable to near‐term sea‐level rise and hurricane‐induced flooding, with substantial human impact. These risks motivate researchers to elucidate the processes and timescales involved in the formation, growth and stabilization of coastlines through the study of Holocene shoreline dynamics.
Marjorie Cantine   +12 more
wiley   +1 more source

Fracture processes studied in CRESST

open access: yesNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 2006
In the early stages of running of the CRESST dark matter search with sapphire crystals as detectors, an unexpectedly high rate of signal pulses appeared. Their origin was finally traced to fracture events in the sapphire due to the very tight clamping of the detectors.
Astrom, J   +17 more
openaire   +1 more source

A Low‐Viscosity Lower Lunar Mantle Implied by Measured Monthly and Yearly Tides

open access: yesAGU Advances, Volume 5, Issue 5, October 2024.
Abstract The Moon's frequency‐dependent tidal response, expressed as temporal variations in its gravity field through the Love number k2 ${k}_{2}$ and as dissipation through the quality factor Q $Q$, provides information about its interior structure. Lunar laser ranging has provided measurements for Q $Q$, but so far no frequency‐dependent values for ...
Sander Goossens   +3 more
wiley   +1 more source

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