Observations of debris disks provide a valuable window to investigate the formation and evolution of planetary systems. We present high-contrast JWST/NIRCam observations of CPD-72 2713, a 24 Myr-old star that belongs to the $\beta$ Pic moving group. We obtained the first scattered-light images of the disk in both F210M...
Jing-Wen Zhang, Maxwell A. Millar-Blanchaer, K. Lawson et al.· 0 citations
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
Kinematic perturbations observed with the Atacama Large Millimeter/submillimeter Array in CO line emission provide evidence for a population of embedded giant protoplanets shaping the structure of protoplanetary disks. We present JWST/MIRI F1140C (λ = 11.3 μm) coronagraphic observations of five protoplanetary disks—HD...
G. Cugno, M. Benisty, R. Teague et al.· Astronomical Journal· 0 citations
Subaru/SCExAO/CHARIS enables near-infrared integral field spectropolarimetry. Quantitative polarimetry is useful for a variety of science cases, particularly measurements related to dust grain properties in circumstellar disks. This capability requires correcting for polarization effects from the optical path via a Mue...
Thomas McIntosh, Man-Xuan Zhang, Briley L. Lewis et al.· Astronomical Telescopes + In...· 2 citations
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