MIRACLES: atmospheric characterization of directly imaged planets and substellar companions at 4-5 micron. I. Photometric analysis of $β$ Pic b, HIP 65426 b, PZ Tel B and HD 206893 B

31 Dec 2019Tomas StolkerSascha P. QuanzKamen O. TodorovJonas KühnPaul MollièreMichael R. MeyerThayne CurrieSebastian DaemgenBaptiste Lavie

Directly imaged planets and substellar companions are key targets for the characterization of self-luminous atmospheres. Their photometric appearance at 4-5 $\mu$m is sensitive to the chemical composition and cloud content of their atmosphere... (read more)

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