398 citations · 823 across the 13 of their papers we have counts for
13 papers
STIPS: The Nancy Grace Roman Space Telescope Imaging Product Simulator
STIPS Development Team, Sebastian Gomez, Andrea Bellini +9
The Space Telescope Imaging Product Simulator (STIPS) is a Python-based package that can be used to simulate scenes from the upcoming \textit{Nancy Grace Roman Space Telescope} (\n…
The IGRINS YSO Survey III: Stellar parameters of pre-main sequence stars in Ophiuchus and Upper Scorpius
Ricardo López-Valdivia, Gregory N. Mace, Eunkyu Han +9
We used the Immersion GRating Infrared Spectrometer (IGRINS) to determine fundamental parameters for 61 K- and M-type young stellar objects (YSOs) located in the Ophiuchus and Uppe…
A 2+1+1 quadruple star system containing the most eccentric, low-mass, short-period, eclipsing binary known
E. Han, S. A. Rappaport, A. Vanderburg +12
We present an analysis of a newly discovered 2+1+1 quadruple system with TESS containing an unresolved eclipsing binary (EB) as part of TIC 121088960 and a close neighbor TIC 12108…
Magnetic Inflation and Stellar Mass IV. Four Low-mass Kepler Eclipsing Binaries Consistent with Non-magnetic Stellar Evolutionary Models
Eunkyu Han, Philip S. Muirhead, Jonathan J. Swift
Low-mass eclipsing binaries show systematically larger radii than model predictions for their mass, metallicity and age. Prominent explanations for the inflation involve enhanced m…
Magnetic Inflation and Stellar Mass III: Revised Parameters for the Component Stars of NSVS 07394765
Brian F. Healy, Eunkyu Han, Philip S. Muirhead +4
We perform a new analysis of the M dwarf-M dwarf eclipsing binary system NSVS 07394765 in order to investigate the reported hyper-inflated radius of one of the component stars. Our…
LHS 1610A: A Nearby Mid-M Dwarf with a Companion That is Likely A Brown Dwarf
Jennifer G. Winters, Jonathan Irwin, Elisabeth R. Newton +7
We present the spectroscopic orbit of LHS 1610A, a newly discovered single-lined spectroscopic binary with a trigonometric distance placing it at 9.9 pm 0.2 pc. We obtained spectra…