Showing 21–40 of 46 results
/ Date/ Name
Oct 12, 2014Magnetism in a family of $S = 1$ square lattice antiferromagnets Ni$X_2$(pyz)$_2$ ($X = $ Cl, Br, I, NCS; pyz = pyrazine)Mar 6, 2020The binary evolution of SAX J1808.4-3658: Implications of an evolved donor starFeb 24, 2013He II recombination lines as a test of the nature of SN Ia progenitors in elliptical galaxiesApr 17, 2014Next generation population synthesis of accreting white dwarfs: I. Hybrid calculations using BSE + MESANov 7, 2013Emission line diagnostics to constrain high temperature populations in early-type galaxiesAug 13, 2015Population synthesis of accreting white dwarfs: II. X-ray and UV emissionJul 29, 2003Analysis of Point-contact Andreev Reflection Spectra in Spin Polarization MeasurementsFeb 22, 2012The Origin of the EUV Late Phase: A Case Study of the C8.8 Flare on 2010 May 5Aug 4, 2010Measurement of 37Ar to support technology for On-site Inspection under the Comprehensive Nuclear-Test-Ban TreatySep 17, 2019Comprehensive models of novae at metallicity $Z = 0.02$ and $Z = 10^{-4}$Feb 12, 2014Upper limits on the luminosity of the progenitor of type Ia supernova SN2014JMar 28, 2001Soft x-ray spectroscopy measurements of the p-like density of states of B in MgB2 and evidence for surface boron oxides on exposed surfacesSep 7, 2002Measurements of Spin Polarization of Epitaxial SrRuO3 Thin FilmsMay 4, 2016Soft X-ray irradiance measured by the Solar Aspect Monitor on the Solar Dynamic Observatory Extreme ultraviolet Variability ExperimentFeb 25, 2016Modelling nova populations in galaxiesJan 28, 2026Euclid: Early Release Observations -- The star-formation history of massive early-type galaxies in the Perseus clusterJun 10, 2025ADAM: Autonomous Discovery and Annotation Model using LLMs for Context-Aware AnnotationsSep 20, 2020Discovery of a ~30-Year-Duration Post-Nova Pulsating Supersoft Source in the Large Magellanic CloudNov 20, 2019The GOES-R EUVS Model for EUV Irradiance VariabilityDec 20, 2018Excluding super-soft X-ray sources as progenitors for four Type Ia supernovae in the Large Magellanic Cloud