IRTF NEAR-IR SPECTROSCOPY OF ASTEROIDS V1.0

This data set contains low-resolution, near-infrared (0.8 - 2.5 micron) spectra of asteroids obtained with SpeX at the NASA Infrared Telescope Facility (IRTF) on Mauna Kea. Since it was commissioned in June 2000, SpeX has been the premier instrument for producing high quality near-IR spectra of asteroids. These spectra have been used for both taxonomic studies of asteroids, and for more detailed mineralogical and compositional investigations. This data set archives the reduced, calibrated spectra that have been published in the peer-reviewed literature, and will be regularly updated as more data become publicly available.

本数据集收录了使用位于莫纳克亚山的美国宇航局红外望远镜设施（IRTF）中的 SpeX 仪器获取的低分辨率近红外（0.8 - 2.5 微米）小行星光谱。自 2000 年 6 月投入使用以来，SpeX 一直是最主要的用于生成高质量近红外小行星光谱的仪器。这些光谱不仅被用于对小行星进行分类研究，亦被用于更深入的矿物学和成分分析。本数据集存储了已发表在同行评审文献中的经过还原和校准的光谱，并将随着更多数据的公开而定期更新。