Fig. 4
Flux calibrated NIR spectra of [CTF93]216-2: SofI spectrum (black), and NICS spectrum (red). For comparison, we show an AMES-DUSTY model spectrum for effective temperature of 3200 K and log g = 4.0 (Allard et al. 2001). The DUSTY spectrum has been shifted by –0.3 × 10-10 erg s-1 cm-2 μm-1 for clarity. The detected features are also labelled.
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