Image Details
Caption: Figure 5.
The color–magnitude diagrams for field sources, low-gravity brown dwarfs and directly imaged planetary mass companions color coded by spectral subtype. Top: MJ (2MASS) vs. (J−W2). Middle: MJ (MKO) vs. (J–K) (MKO). Bottom: MH (MKO) vs. (H–L) (MKO). In the absence of L-band photometry for brown dwarfs we used the relation in Faherty et al. (2016) to convert WISE W1 photometry to L (MKO).
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