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Absolute dimensions of the low-mass eclipsing binary system NSVS 10653195
Ramon Iglesias-Marzoa, Maria J. Arevalo, Mercedes Lopez-Morales +3
Low-mass stars in eclipsing binary systems show radii larger and effective temperatures lower than theoretical stellar models predict for isolated stars with the same masses. Eclip…
Photometric and Spectroscopic Properties of Type Ia Supernova 2018oh with Early Excess Emission from the 2 Observations
W. Li, X. Wang, J. Vinkó +160
Supernova (SN) 2018oh (ASASSN-18bt) is the first spectroscopically-confirmed type Ia supernova (SN Ia) observed in the field. The data revealed an excess emission…
A refined analysis of the low-mass eclipsing binary system T-Cyg1-12664
R. Ramón Iglesias-Marzoa, M. López-Morales, M. J. Arévalo +2
The observational mass-radius relation of main sequence stars with masses between ~0.3 and 1.0 Msun reveals deviations between the stellar radii predicted by models and the observe…
Structure in the Disk of epsilon Aurigae: Analysis of the ARCES and TripleSpec data obtained during the 2010 eclipse
Justus L. Gibson, Robert E. Stencel, William Ketzeback +4
Context: Worldwide interest in the recent eclipse of epsilon Aurigae resulted in the generation of several extensive data sets, including those related to high resolution spectrosc…
Kepler Eclipsing Binary Stars. VI. Identification of Eclipsing Binaries in the K2 Campaign 0 Data-set
Daryll M. LaCourse, Kian J. Jek, Thomas L. Jacobs +15
The original {\it Kepler} mission observed and characterized over 2400 eclipsing binaries in addition to its prolific exoplanet detections. Despite the mechanical malfunction and s…
Fundamental Parameters of Exoplanets and Their Host Stars
Jeffrey L. Coughlin
For much of human history we have wondered how our solar system formed, and whether there are any other planets like ours around other stars. Only in the last 20 years have we had…