Theoretical models of evaporating lava atmospheres for 55 Cnce from Zilinskas et al. (2022). Two models are for bulk-silicate composition (in yellow) and for evolved bulk-silicate composition (in purple). Also overplotted are photometric occultation depths from 2.1 μm channel (in blue) and white-light occultation depths for 4.5 μm channel (in maroon). The blue and maroon points are slightly spread in wavelength near their bandpasses to avoid overlap. We show the two bandpasses corresponding to both of these channels. The black points show the predicted occultation depths for both NIRCam bandpasses with different shapes representing bulk-silicate (stars) and evolved bulk- silicate (squares) compositions.