George H. Rieke

TL;DR: In this paper, the authors provide a short discussion of the principles of operation, design, and performance of individual MIRI detectors, in support of a description of their operation in arrays provided in an accompanying paper.

TL;DR: In this article, the authors presented Spitzer observations of the dwarf starburst galaxy NGC 1705 obtained as part of SINGS, showing that the galaxy morphology is very different shortward and longward of ~5 microns: short-wavelength imaging shows an underlying red stellar population, with the central super star cluster (SSC) dominating the luminosity; longer wavelength data reveals warm dust emission arising from two off-nuclear regions offset by ~250 pc from the SSC.

TL;DR: In this article, the authors compare the soft diffuse X-ray emission from Chandra images of 12 nearby intermediate inclination spiral galaxies to the morphology seen in Halpha, molecular gas, and mid-infrared emission.

TL;DR: In this article, physical dust models are presented for 65 galaxies in the SINGS survey that are strongly detected in the four IRAC bands and three MIPS bands, and the observed SEDs including galaxies with SCUBA photometry, can be reproduced by dust models that do not require "cold" (T < 10K) dust.