Fornasier Spectra of M Asteroids
This data set contains reduced composite
visual and near-infrared spectra of thirty M-type asteroids, observed
over the years 2004-2008 and presented in Fornasier et al. (2010).
The spectra were taken with the Dolores and NICS instruments at the
Telescopio Nationale Galileo (TNG) in La Palma, with the EMMI and SOFI
instruments at the ESO New Technology Telescope (NTT) in Chile, and
with the SPeX instrument at the Infrared Telescope Facility (IRTF) in
Hawaii. The individual spectra from the various instruments used to
produce the composite spectra are also included.
Release Date: 2020-06-24
Data Set Info
|PDS4 version||urn:nasa:pds:gbo.ast-m-type.fornasier.spectra::1.0||Browse||Download (1.9 Mb)|
|PDS3 version||EAR-A-I1092-2-MSPECTRA-V1.0||Browse||Download (1.8 Mb)|
The PDS4 bundle was migrated from the PDS3 data set in June 2020. The data content is unchanged.
Use the following citation to reference this data set:
"Fornasier, S., Clark, B.E., Migliorini,
A., and Ockert-Bell, M. (2020). Fornasier Spectra of M Asteroids V1.0.
urn:nasa:pds:gbo.ast-m-type.fornasier.spectra::1.0. NASA Planetary Data System; https://doi.org/10.26033/2mpm-j141."