Spectroscopic survey of IC 1396 identifies 25 new brown dwarfs and measures a star-to-brown-dwarf ratio of 5.0±0.4 that is consistent with other young clusters.
Color Transformations for the 2MASS Second Incremental Data Release
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abstract
Transformation equations are presented to convert colors and magnitudes measured in the AAO, ARNICA, CIT, DENIS, ESO, LCO (Persson standards), MSSSO, SAAO, and UKIRT photometric systems to the photometric system inherent to the 2MASS Second Incremental Data Release. The transformations have been derived by comparing 2MASS photometry with published magnitudes and colors for stars observed in these systems. Transformation equations have also been derived indirectly for the Bessell & Brett (1988) and Koornneef (1983) homogenized photometric systems.
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Revealing the substellar population of IC 1396: A spectroscopic survey of brown dwarfs in the region
Spectroscopic survey of IC 1396 identifies 25 new brown dwarfs and measures a star-to-brown-dwarf ratio of 5.0±0.4 that is consistent with other young clusters.