Image Details
Caption: Figure 4.
JWST NIRCam (top row) and MIRI (bottom row) imaging for the TEMPLATES program. NIRCam short-wavelength (SW) filters F200W, F150W, and F115W were used for the two LBG sources, whereas long-wavelength (LW) filters F444W, F356W, and F277W were used for the two SMGs as the red, green, and blue (RGB) channels. For MIRI imaging, F1000W, F770W, and F560W were selected as the filters for RGB for all sources but one. The exception, SGAS1226+21, is only detected in F560W, so only that filter image is shown using the color map “bone.” All images have been aligned with north up and east left, with a common scale bar of 0.″5 shown.
© 2024. The Author(s). Published by the American Astronomical Society.