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First Results from the JWST Early Release Science Program Q3D: Benchmark Comparison of Optical and Mid-infrared Tracers of a Dusty, Ionized Red Quasar Wind at z = 0.435

  • Authors: David S. N. Rupke, Dominika Wylezalek, Nadia L. Zakamska, Sylvain Veilleux, Caroline Bertemes, Yuzo Ishikawa, Weizhe Liu, Swetha Sankar, Andrey Vayner, Hui Xian Grace Lim, Ryan McCrory, Grey Murphree, Lillian Whitesell, Lu Shen, Guilin Liu, Jorge K. Barrera-Ballesteros, Hsiao-Wen Chen, Nadiia Diachenko, Andy D. Goulding, Jenny E. Greene, Kevin N. Hainline, Fred Hamann, Timothy Heckman, Sean D. Johnson, Dieter Lutz, Nora Lützgendorf, Vincenzo Mainieri, Nicole P. H. Nesvadba, Patrick Ogle, Eckhard Sturm

David S. N. Rupke et al 2023 The Astrophysical Journal Letters 953 .

  • Provider: AAS Journals

Caption: Figure 7.

(a) MIRI Channel 3B point-spread function. White contours are spaced by factors of 2 in surface brightness from 0.512 times the peak flux to 0.002 of peak. The dashed red and purple lines mark two apertures used in the radial profile computation. (b) Radial surface brightness profiles of the MIRI and GMOS data, normalized to the 2D peak flux. The profiles are Gaussian within 3 pixels, with FWHM = 0.″62–0.″65. They have non-Gaussian wings carrying ∼10%–15% power. The 1σ error in the MIRI profile is represented by the shaded area. The apertures shown in (a) are delineated by the vertical dashed lines.

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