SMASS ASTEROID SURVEY V1.0

Description

The Small Main-belt Asteroid Spectrographic Survey (SMASS) was initiated in 1990 with the goal of obtaining spectra over the visual wavelength region for a substantial number of small (D < 20 km) main-belt asteroids. Observations were primarily made using the 2.4 m Hiltner telescope, located at the Michigan-Dartmouth-MIT (MDM) Observatory on the southwest ridge of Kitt Peak in Arizona.

Resources

Name Format Description Link
21 Search results for publications that cite this dataset by its DOI. https://scholar.google.com/scholar?q=10.7927%2FH4JW8BX5
22 Sample browse graphic of the data set. https://sedac.ciesin.columbia.edu/downloads/maps/gpw-v4/gpw-v4-population-count-rev11/gpw-v4-population-count-rev11-global-2015-thumbnail.jpg
21 Data Download Page https://sedac.ciesin.columbia.edu/data/set/gpw-v4-population-count-rev10/data-download
21 Maps Download Page https://sedac.ciesin.columbia.edu/data/set/gpw-v4-population-count-rev11/maps
21 Web Map Service Page https://sedac.ciesin.columbia.edu/data/set/gpw-v4-population-count-rev11/maps/services
21 Data Set Overview Page https://sedac.ciesin.columbia.edu/data/set/gpw-v4-population-count-rev11

Tags

  • support-archives
  • asteroid

Topics

Categories