Difference between 'Optical Spectral Type' and 'IR Spectral Type'?

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The discussion highlights the distinction between 'Optical Spectral Type' and 'IR Spectral Type' in L and T dwarfs, noting that these classifications arise from different measurement instruments. It emphasizes that spectral types reflect surface temperatures, yet optical and infrared measurements can yield varying results due to the faintness of visual spectra. The infrared spectral type is suggested to be more accurate, as most celestial objects, particularly those with low V-band emissions, are brighter in the infrared spectrum. The optical band, limited to the V-band spectrum, provides a narrower view compared to the broader infrared spectrum. Overall, the choice of spectral type depends on the specific characteristics of the observed objects.
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In the list of L and T dwarfs at 'dwarfarchives.org' (http://ldwarf.ipac.caltech.edu/archive/version5/viewlist.php?table=ltdwarf&format=html") there are two columns named 'spectral_type_opt' and 'spectral_type_ir'. I guess this comes from the type of instrument used in the measurements?

If I'm correct, the Spectral Type indicates the surface temperature of stars. If so why would the optical and infrared spectra give two different measurements? Which one is more accurate? Since the visual spectra of L and T dwarfs are very faint, would the 'infrared spectral type' be more accurate?
 
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