Optical Spectra of the Large Uranian Moons

Visible-wavelength (~0.4 - 0.9 micron) reflectance spectra of the large Uranian satellites Ariel, Umbriel, Titania, and Oberon. These spectra were collected between 2002-2010 (and in 2024) with the DBSP spectrograph on the 200-inch telescope at Palomar Observatory, and between 2018-2020 with the DeVeny spectrograph on the Lowell Discovery Telescope. The dataset also includes B,V,R filter photometry of Titania and Oberon, acquired in 2005 with the 24-inch telescope at Table Mountain Observatory. All data files are plain text ASCII files or .csv files. For more information, see the associated manuscript and the readme file in the download. Please also cite the associated manuscript for any use of this dataset.