2.9k citations
- Centre National de la Recherche ScientifiqueFR339 papers
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- European Southern ObservatoryCL252 papers
- University of CambridgeGB245 papers
- Max Planck Institute for AstronomyDE217 papers
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- Center for Astrophysics Harvard & SmithsonianUS204 papers
- Osservatorio Astronomico di PadovaIT192 papers
23 papers · 2 filters
OGLE-2013-BLG-0911Lb: A Secondary on the Brown-Dwarf Planet Boundary around an M-dwarf
Shota Miyazaki, Takahiro Sumi, David P. Bennett +92
We present the analysis of the binary-lens microlensing event OGLE-2013-BLG-0911. The best-fit solutions indicate the binary mass ratio of q~0.03 which differs from that reported i…
A Holistic and Probabilistic Approach to the Ground-based Data of HAT-P-19 System
Ozgur Basturk, Selcuk Yalcinkaya, Ekrem M. Esmer +2
We update the fundamental physical and orbital properties of the transiting hot-Saturn type exoplanet HAT-P-19b and its host star HAT-P-19 as a result of the global modeling of our…
Detection of Na, K and HO in the hazy atmosphere of WASP-6b
Aarynn L. Carter, Nikolay Nikolov, David K. Sing +13
We present new observations of the transmission spectrum of the hot Jupiter WASP-6b both from the ground with the Very Large Telescope (VLT) FOcal Reducer and Spectrograph (FORS2)…
WASP-127b transmission spectrum]{Abundance measurements of HO and carbon-bearing species in the atmosphere of WASP-127b confirm its super-solar metallicity
Jessica J. Spake, David K. Sing, Hannah R. Wakeford +14
The chemical abundances of exoplanet atmospheres may provide valuable information about the bulk compositions, formation pathways, and evolutionary histories of planets. Exoplanets…
WASP-South detection of HD219666b transits provides an accurate ephemeris
C. Hellier, D. R. Anderson, S. Gill +1
The hot-Neptune HD219666b (= TOI-118.01) was an early discovery from Sector 1 of the TESS transit survey. Being a rare "Neptune desert" planet, and transiting a bright, V = 9.9 sta…
The highly inflated giant planet WASP-174b
L. Mancini, P. Sarkis, Th. Henning +18
The transiting exoplanetary system WASP-174 was reported to be composed by a main-sequence F star (V=11.8 mag) and a giant planet, WASP-174b (orbital period 4.23 days). However onl…