We present the discovery of RX J0534.0-0221 b, a giant planet orbiting an M dwarf star in the β Pictoris moving group. RX J0534 was originally observed with JWST/NIRCam in the F444W and F200W filters. Observations in F444W reveal a point source at signal-to-noise ratio ∼17.5 at ∼0.″41 (∼14 au) from the host star, with...
Rodrigo Ferrer-Chávez, Jason J. Wang, K. Wagner et al.· Astrophysical Journal Letter...· 0 citations
The SAXO+ system is a planned second-stage Adaptive Optics (AO) upgrade to the VLT/SPHERE eXtreme Adaptive Optics (SAXO) system. This consists of adding a second adaptive optics stage using a near-infrared pyramid wavefront sensor to record images of fainter exoplanets around redder stars. In this work, we compare the...
M. Langlois, C. B'echet, L. Schreiber et al.· Astronomical Telescopes + In...· 2 citations
The Mid-infrared Extremely Large Telescope (ELT) Imager and Spectrograph (METIS) instrument, expected to see first light in early 2030, aims to detect and characterise exoplanets and circumstellar disks through high contrast imaging (HCI) and spectroscopy. The High-contrast End-to-End Performance Simulator (HEEPS), ini...
Gilles Orban de Xivry, O. Absil, I. Hammond et al.· Astronomical Telescopes + In...· 1 citation
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