LMI Gallery
Learn MoreThe all-purpose camera, principal imager, and workhorse instrument for the LDT.
Lowell astronomer Phil Massey is Principal Investigator for the instrument. Funded by a grant from the National Science Foundation, the LMI was commissioned in 2013 and 2014 and is now in full service. To maximize its field of view, the LMI is mounted at the straight-through position of the instrument cube.
The LMI features a 36 megapixel e2V charge-coupled device (CCD) with a field of view of 12.5 x 12.5 arc minutes. The philosophy behind the LMI is to enable imaging of a significant field of view in one exposure. Smaller CCDs have to be assembled in a mosaic to cover a large field of view, which reduces observing efficiency and creates complications in data reduction. The LMI, which uses the largest CCD that can be manufactured using current technology, sidesteps these problems and gives the LDT a highly effective and efficient imaging camera.
These images are copyrighted, and all rights are reserved. If you plan to use any of these images for anything other than your personal enjoyment or educational/research use, please contact Kevin Schindler (kevin@lowell.edu); in general, commercial use is not allowed.
NGC 891
The Moon
Stephan's Quintet
NGC 4631
NGC 2903
NGC 7538
NGC 7331 Group of Galaxies
NGC 6946
NGC 1275 and the Perseus Cluster of Galaxies
NGC 772
NGC 772 Stretched
NGC 772 B&W
NGC 210
NGC 206 in M31 - 1
NGC 206 in M31 - 2
The Sombrero Galaxy
M 95 (NGC 3351)
M 74 (NGC 628)
M 51 The Whirlpool Galaxy
M 15 (NGC 7078)
M 1: the Crab Nebula
Jupiter and the Galilean Satellites
IC 342
The Horsehead Nebula
The Helix Nebula (NGC 7293)
M 108
M108 Version 2
M 66
M 27 The Dumbbell Nebula
M33