Imaging Data from Sub-Seasonal Variation in Neptune's Mid-Infrared Emission by Roman et al.

Images of Neptune as used in Imaging Data from Sub-Seasonal Variation in Neptune's Mid-Infrared Emission by Michael T. Roman, Leigh N. Fletcher, Glenn S. Orton, Thomas K. Greathouse, Julianne I. Moses, Naomi Rowe-Gurney, Patrick G. J. Irwin, Arrate Antunano, James Sinclair, Yasumasa Kasaba, Takuya Fujiyoshi, Imke de Pater, Heidi B. Hammel.

Data are from various observatories/telescope instruments, including:

The European Southern Observatory's Very Large Telescope, VISIR

Keck Observatory, LWS

Subaru Observatory, COMICS

Gemini North, Michelle and TEXES

Gemini South, T-ReCS

Data were acquired from observatory archives and flux calibrated, when possible, by comparison to standard stars, with spectral radiances expressed in units of W/m2/sr/micron.  North is up in the images.  The first extension (ext=0) is the image in native spatial resolution.  The second extension (ext=1) features the disk normalized in size to that of the finest data (i.e., to a disk with an equatorial width of 51.8 pixels, as imaged by VLT-VISIR on August 13, 2018).

Image file names and times correspond to approximate mid-time of combined image sequences, and will differ from original file headers.

Questions concerning these data should be directed towards Michael Roman, [e-mail] or [e-mail]