Image Details
Caption: Figure 13.
Spitzer light curves for the variable brown dwarf SIMP 1629+0335. The top panel displays the data taken in Channel 1 (3.6 μm) in 2012. The middle and bottom panels display the data from Channel 2 (4.5 μm) and Channel 1 (3.6 μm), respectively, taken in 2015. The corrected light curves are shown in red, with 50 random draws from our MCMC fit shown in black. The measured rotation period is significantly different in all three epochs.
© 2022. The Author(s). Published by the American Astronomical Society.