An Efficient Low-Resolution NIR Classification Scheme for M, L, and T dwarfs and Its Application to Young BDs

Bibcode
2003IAUS..211..359T
Testi, L.; Natta, A.; Baffa, C.; Comoretto, G.; Gennari, S.; Ghinassi, F.; Licandro, J.; Magazzù, A.; Oliva, E.; D'Antona, F.
Bibliographical reference

Brown Dwarfs, Proceedings of IAU Symposium #211, held 20-24 May 2002 at University of Hawaii, Honolulu, Hawaii. Edited by Eduardo Martín. San Francisco: Astronomical Society of the Pacific, 2003, p. 359

Advertised on:
6
2003
Number of authors
10
IAC number of authors
0
Citations
0
Refereed citations
0
Description
We present the preliminary results of a programme aimed at defining a low-resolution near-infrared spectral classification scheme for faint M, L, and T-dwarfs. The method is based on the global shape of R˜100 complete near-infrared spectra from 0.8 to 2.4μm as obtained through a high-throughput prism-based optical element, the Amici device, mounted inside the NICS instrument at the TNG 3.5m telescope (Baffa et al. 2001; Oliva 2000). The aim of our project is to provide an efficient classification scheme based on very low-resolution near infrared spectroscopy, which can be carried on at a 4m-class telescope.
Type
Non-refereed

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