IRTF observations of Io from 1983 to 1993
These images show Jupiter's moon Io obtained at different infrared wavelengths with the W. M. Keck Observatory's 10-meter Keck II telescope on Aug. 15, 2013 (a and c), and the Gemini North telescope on Aug. 29, 2013 (d).Image Credit: NSF/NASA/JPL-Caltech//UC Berkeley/Gemini Observatory/W. M. Keck Observatory
NASA's Infrared Telescope Facility (IRTF) data were collected at 4.8 μ (M band), 8.7 μ,10 μ (N band),and 20 μ (Q band).These data were published in 1994 by Veeder, G. J., et al. Io's heat flow from infrared radiometry: 1983-1993, J. Geophys. Research, 99, 17095-17162. An electronically accessible form is provided here.
Data (Tables 2, 3, 4 and 5 are 4.8, 8.7, 10 and 20 µ, respectively)
Tables 1, A1 an A2 are ancillary data
A. G. Davies, G.J. Veeder (2020), Io IRTF Photometry 1983-1993, NASA Planetary Data System, https://doi.org/10.17189/1518953.