Planet WASP-103 b

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• Stellar obliquity measurements of six gas giants. Orbital misalignment of WASP-101b and WASP-131b

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• Thermal Emission from the Hot Jupiter WASP-103b in J and Ks Bands

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• Planet-star interactions with precise transit timing. III. Entering the regime of dynamical tides

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• On spectroscopic phase-curve retrievals: H2 dissociation and thermal inversion in the atmosphere of the ultra-hot Jupiter WASP-103 b

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• Geometric Albedos at Short Optical Wavelengths for the Hot Jupiters WASP-43b, WASP-103b, and TrES-3b

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• Detection of the tidal deformation of WASP-103b at 3 sigma with CHEOPS

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• ACCESS & LRG-BEASTS: a precise new optical transmission spectrum of the ultrahot Jupiter WASP-103b

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• Ground-Based Transmission Spectroscopy with FORS2: A featureless optical transmission spectrum and detection of H2O for the ultra-hot Jupiter WASP-103b

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• Ground-Based Transmission Spectroscopy with FORS2: A featureless optical transmission spectrum and detection of H2O for the ultra-hot Jupiter WASP-103b

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• Global Climate and Atmospheric Composition of the Ultra-Hot Jupiter WASP-103b from HST and Spitzer Phase Curve Observations

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• Planet-star interactions with precise transit timing. I. The refined orbital decay rate for WASP-12 b and initial constraints for HAT-P-23 b, KELT-1 b, KELT-16 b, WASP-33 b, and WASP-103 b

  2018 MACIEJEWSKI G., FERNANDEZ M., ACEITUNO F., MARTIN-RUIZ S., OHLERT J. et al.
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• Investigating the physical properties of transiting hot Jupiters with the 1.5-m Kuiper Telescope

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• High-precision multi-wavelength eclipse photometry of the ultra-hot gas giant exoplanet WASP-103 b

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  arxiv  

• Signs of strong Na and K absorption in the transmission spectrum of WASP-103b

  2017 LENDL M., CUBILLOS P., HAGELBERG J., MULLER A., JUVAN I. & FOSSATI L.
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• Spin-orbit alignments for Three Transiting Hot Jupiters: WASP-103b, WASP-87b, & WASP-66b

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• Near-IR Emission Spectrum of WASP-103b using Hubble Space Telescope/Wide Field Camera 3

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• SALT observations of the Chromospheric Activity of Transiting Planet Hosts: Mass Loss and Star Planet Interactions

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• Contamination from a nearby star cannot explain the anomalous transmission spectrum of the ultra-short period giant planet WASP-103b

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• Eight years of accurate photometric follow-up of transiting giant exoplanets

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• WASP-103b: a new planet at the edge of tidal disruption

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  Astron. & Astrophys. , accepted
  arxiv