Synthetic Photometry
Model:
UVES/VLT
A high-resolution (R = 40000), flux calibrated, optical+NIR (6400-8900A) library of late type subdwarfs, from late K to M9.5, obtained with UVES at VLT. The library is described in Rajpurohit et al. (2014)
Model parameters
SpTy:(?)

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© CAB 2008