Pharmacokinetics of organic cation transporter 1 (OCT1) substrates in Oct1/2 knockout mice and species difference in hepatic OCT1-mediated uptake
BL Morse, A Kolur, LR Hudson, AT Hogan… - Drug Metabolism and …, 2020 - ASPET
Organic cation transporter 1 (OCT1) plays a role in hepatic uptake of drugs, affecting in vivo
exposure, distinguished primarily through pharmacogenetics of the SLC22A1 gene. The role …
exposure, distinguished primarily through pharmacogenetics of the SLC22A1 gene. The role …
The MUSCLES treasury survey. V. FUV Flares on active and inactive M Dwarfs
… For the COS and STIS UV data, we created light curves over a given bandpass using the
process described in Loyd & France (2014). In brief, this involves binning detector events within …
process described in Loyd & France (2014). In brief, this involves binning detector events within …
Constraining the physical properties of stellar coronal mass ejections with coronal dimming: application to far-ultraviolet data of ϵ Eridani
Coronal mass ejections (CMEs) are a prominent contributor to solar system space weather
and might have impacted the Sun's early angular momentum evolution. A signal diagnostic of …
and might have impacted the Sun's early angular momentum evolution. A signal diagnostic of …
Stellar flares from blended and neighbouring stars in Kepler short cadence observations
…, E Shkolnik, ROP Loyd - Monthly Notices of the …, 2021 - academic.oup.com
We present the results of a search for stellar flares from stars neighbouring the target sources
in the Kepler short cadence data. These flares have been discarded as contaminants in …
in the Kepler short cadence data. These flares have been discarded as contaminants in …
Extending optical flare models to the UV: results from comparing of TESS and GALEX flare observations for M Dwarfs
…, S Fleming, T Richey-Yowell, ROP Loyd - Monthly Notices of …, 2023 - academic.oup.com
… To detect white-light flares in the TESS observations, we first detrended the light curves
following a method similar to that used in Jackman, Shkolnik & Loyd (2021a). This method is …
following a method similar to that used in Jackman, Shkolnik & Loyd (2021a). This method is …
Fluctuations and flares in the ultraviolet line emission of cool stars: Implications for exoplanet transit observations
Variations in stellar flux can potentially overwhelm the photometric signal of a transiting planet.
Such variability has not previously been well-characterized in the ultraviolet lines used to …
Such variability has not previously been well-characterized in the ultraviolet lines used to …
Flares, Rotation, Activity Cycles, and a Magnetic Star–Planet Interaction Hypothesis for the Far-ultraviolet Emission of GJ 436
ROP Loyd, PC Schneider, JAG Jackman… - The Astronomical …, 2023 - iopscience.iop.org
… instead of the 1 minute bins used by Loyd & France (2014), to offset the faintness of GJ 436,
which was the fifth faintest star among the 42 analyzed in Loyd & France (2014). We allowed …
which was the fifth faintest star among the 42 analyzed in Loyd & France (2014). We allowed …
Discovery of an extremely short duration flare from Proxima Centauri using millimeter through far-ultraviolet observations
…, AJ Weinberger, ROP Loyd… - The Astrophysical …, 2021 - iopscience.iop.org
We present the discovery of an extreme flaring event from Proxima Cen by the Australian
Square Kilometre Array Pathfinder (ASKAP), Atacama Large Millimeter/submillimeter Array (…
Square Kilometre Array Pathfinder (ASKAP), Atacama Large Millimeter/submillimeter Array (…
The Mouse that Squeaked: A small flare from Proxima Cen observed in the millimeter, optical, and soft X-ray with Chandra and ALMA
We present millimeter, optical, and soft X-ray observations of a stellar flare with an energy
squarely in the regime of typical X1 solar flares. The flare was observed from Proxima Cen on …
squarely in the regime of typical X1 solar flares. The flare was observed from Proxima Cen on …
The Volatility of Far-Ultraviolet Radiation from Low-Mass Stars and Planetary Implications
ROP Loyd - 2017 - search.proquest.com
A low-mass star emits only 0.001-0.01% of its electromagnetic energy in the ultraviolet (100–1700
Å), yet the implications for planets are profound. Radiation at the short-wavelength …
Å), yet the implications for planets are profound. Radiation at the short-wavelength …