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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 1.

(a) Total [S IV] 10.51 μm model surface brightness in each 0.″2 spaxel, in erg s−1 cm−2 arcsec−2. A black, filled circle locates the quasar. The inset shows the spectrum of, and fit to, two spaxels. Surface brightness contours begin at 1 × 10−15 erg s−1 cm−2 arcsec−2 and descend by factors of 2. (b) Model flux reprojected to 2.″3 spaxels, to illustrate the 10× improved resolution of MIRI/MRS compared to the sampling of the Short–High module of the InfraRed Spectrograph on board Spitzer.

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