Emma McGinness

ORCID: 0000-0003-1457-2213
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About
Contact & Profiles
Research Areas
  • Neutrino Physics Research
  • Dark Matter and Cosmic Phenomena
  • Gamma-ray bursts and supernovae
  • Ionosphere and magnetosphere dynamics
  • Solar and Space Plasma Dynamics
  • Scientific Research and Discoveries
  • Particle physics theoretical and experimental studies
  • Earthquake Detection and Analysis
  • Pulsars and Gravitational Waves Research
  • Galaxies: Formation, Evolution, Phenomena
  • Stellar, planetary, and galactic studies
  • Geomagnetism and Paleomagnetism Studies
  • Atomic and Subatomic Physics Research
  • Astrophysics and Cosmic Phenomena

University of California, Berkeley
2021-2023

Netherlands Institute for Radio Astronomy
2021

Abstract Isolated geomagnetic storms during solar minimum offer the opportunity to observe effects of wind on Earth's atmosphere without interference from other background changes in ionosphere‐thermosphere system. Here, we a minor storm ionosphere at middle and low latitudes, where disturbances thermospheric winds composition can produce storm‐time ionospheric densities. Using data NASA Ionospheric Connection Explorer (ICON), investigate competing neutral modifying 25 January 2021 storm....

10.1029/2022ja031207 article EN cc-by-nc Journal of Geophysical Research Space Physics 2023-06-25

We present BVRI and unfiltered Clear light curves of 70 stripped-envelope supernovae (SESNe), observed between 2003 2020, from the Lick Observatory Supernova Search (LOSS) follow-up program. Our SESN sample consists 19 spectroscopically normal SNe~Ib, two peculiar SNe Ib, six SN Ibn, 14 Ic, one ten Ic-BL, 15 IIb, ambiguous IIb/Ib/c, superluminous SNe. photometry has (on a per-SN basis) mean coverage 81 photometric points (median 58 points) cadence 3.6d 1.2d). From our full sample, subset 38...

10.1093/mnras/stac723 article EN Monthly Notices of the Royal Astronomical Society 2022-03-15

The DARWIN collaboration recently argued that (dark matter wimp search with liquid xenon) can collect, via neutrino-electron scattering, a large, useful sample of solar $pp$-neutrinos, and measure their survival probability subpercent precision. We explore the physics potential such in more detail. estimate that, 300 ton-years data, also measure, help current neutrino value ${\mathrm{sin}}^{2}{\ensuremath{\theta}}_{13}$, to exclude ${\mathrm{sin}}^{2}{\ensuremath{\theta}}_{13}=0$ close...

10.1103/physrevd.106.096017 article EN cc-by Physical review. D/Physical review. D. 2022-11-17

A string of recent studies has debated the exact form and physical origin an evolutionary trend between peak luminosity Type Ia supernovae (SNe Ia) properties galaxies that host them. We shed new light on discussion by presenting analysis ~200 low-redshift SNe in which we measure separation Hubble residuals (HR; as probes luminosity) two host-galaxy morphological types. show this can test predictions made recently proposed models, using independently empirically determined distribution each...

10.1093/mnrasl/slab034 article EN Monthly Notices of the Royal Astronomical Society Letters 2021-03-31

The DARWIN collaboration recently argued that (DARk matter WImp search with liquid xenoN) can collect, via neutrino--electron scattering, a large, useful sample of solar $pp$-neutrinos, and measure their survival probability sub-percent precision. We explore the physics potential such in more detail. estimate that, 300 ton-years data, also measure, help current neutrino value $\sin^2θ_{13}$, to exclude $\sin^2θ_{13}=0$ close three-sigma level. some detail how well constrain existence new...

10.48550/arxiv.2111.02421 preprint EN cc-by arXiv (Cornell University) 2021-01-01
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