Using an Ellipsoid Model to Track and Predict the Evolution and Propagation of Coronal Mass Ejections

Using HINODE/EIS to Confirm a Seismologically Inferred Coronal Temperature

Using Limb-Darkening to Measure the Masses of Red Giants

Using open clusters to study mixing in low- and intermediate-mass stars

Using the Sun to estimate Earth-like planets detection capabilities. III. Impact of spots and plages on astrometric detection

Using X-Ray Observations to Explore the Binary Interaction in Eta Carinae

UV Emission line shifts of symbiotic binaries

UV Spectral Synthesis of Vega

UV Spectroscopy of the Central Star of the Planetary Nebula A43

UV, optical and near-IR diagnostics of massive stars

UV-Bright Stellar Populations and Their Evolutionary Implications in the Collapsed-Core Cluster M15

uvby-$β$ photometry of solar twins: the solar colors, model atmospheres, and the Teff and metallicity scales

uvby-beta photoelectric photometry of Cepheid stars

uvbybeta photometry of early type open cluster and field stars

UX Mon as a W Ser binary

V1162 Orion: Updated Amplitude and Period Variation

V1647 Orionis: Optical Photometric and Spectroscopic Monitoring Through the 2003-2006 Outburst

V1647 Orionis: Reinvigorated Accretion and the Re-Appearance of McNeil's Nebula

V1898 Cygni: An interacting eclipsing binary in the vicinity of North America nebula

V2368 Oph: An eclipsing and double-lined spectroscopic binary used as a photometric comparison star for U Oph