0000000000460810

AUTHOR

Long Wang

showing 2 related works from this author

Photometric and Spectroscopic Properties of Type Ia Supernova 2018oh with Early Excess Emission from the $Kepler$ 2 Observations

2019

Supernova (SN) 2018oh (ASASSN-18bt) is the first spectroscopically-confirmed type Ia supernova (SN Ia) observed in the $Kepler$ field. The $Kepler$ data revealed an excess emission in its early light curve, allowing to place interesting constraints on its progenitor system (Dimitriadis et al. 2018, Shappee et al. 2018b). Here, we present extensive optical, ultraviolet, and near-infrared photometry, as well as dense sampling of optical spectra, for this object. SN 2018oh is relatively normal in its photometric evolution, with a rise time of 18.3$\pm$0.3 days and $\Delta$m$_{15}(B)=0.96\pm$0.03 mag, but it seems to have bluer $B - V$ colors. We construct the "uvoir" bolometric light curve hav…

DATA RELEASEULTRAVIOLETFACTORY OBSERVATIONSFOS: Physical sciencesAstrophysicsType (model theory)medicine.disease_causeSN 2011FE01 natural sciencesLuminosityPhotometry (optics)individual (SN 2018oh) [supernovae]supernovae: generalCIRCUMSTELLAR MATERIAL0103 physical sciencesmedicineSPECTRAAbsorption (logic)Ejecta010303 astronomy & astrophysicssupernovae: individualQCSolar and Stellar Astrophysics (astro-ph.SR)QBLIGHT CURVESHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsHIGH-VELOCITY FEATURES010308 nuclear & particles physicsAstronomy and AstrophysicsLight curveSupernovaAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceIMPROVED DISTANCESWHITE-DWARF MODELSAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]general [supernovae]Ultraviolet
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Measurement of the muon charge asymmetry from W boson decays

2008

We present a measurement of the muon charge asymmetry from W boson decays using 0.3 fb^{-1} of data collected at \sqrt{s}=1.96 GeV between 2002 and 2004 with the D0 detector at the Fermilab Tevatron ppbar Collider. We compare our findings with expectations from next-to-leading-order calculations performed using the CTEQ6.1M and MRST04 NLO parton distribution functions. Our findings can be used to constrain future parton distribution function fits.

PhysicsNuclear and High Energy PhysicsParticle physicsMuon010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyTevatronFOS: Physical sciencesCharge (physics)Parton01 natural sciencesHigh Energy Physics - Experimentlaw.inventionHigh Energy Physics - Experiment (hep-ex)Distribution functionlaw0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]High Energy Physics::ExperimentFermilab010306 general physicsColliderNuclear ExperimentBoson
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