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A Redshift-based Red Selection of Dusty Star-forming Galaxies

  • Authors: A. J. Barger, L. L. Cowie, S. J. McKay, F. E. Bauer

A. J. Barger et al 2026 The Astrophysical Journal 1004 .

  • Provider: AAS Journals

Caption: Figure 11.

SFR vs. redshift for our JWST sample with z = 1.5−5.5 and M* = 108–1010 M (top), z = 1.5−5.5 and M* > 1010 M (middle), and z > 4 without any mass restriction (bottom). Along the top of each panel is the age in Gyr. The red line shows SFR = 30 M yr−1. The symbols are for ALMA detections (purple squares; filled for sources with >4.5σ detections, open for >3σ), published LRDs (red circles), quiescent galaxies satisfying the strict R. J. Williams et al. (2009) selection (blue diamonds), bright X-ray sources (green triangles), and the remaining sources (plus signs). Note that none of the LRDs or quiescent galaxies are detected in the ALMA data.

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