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The Cold Debris Disk Surveys. I. Host Star Properties

  • Authors: Scott J. Kenyon, Benjamin C. Bromley, Joan R. Najita

Scott J. Kenyon et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 2.

The same as in Figure 1 for data from WISE (purple), Spitzer IRAC and MIPS (light blue), IRAS (dark green), Herschel PACS and SPIRE (gold), and submillimeter to millimeter (red). The light-blue symbols with a dark-blue center indicate the fraction of CDDS stars with high-quality synthetic photometry at 8–25 μm from Spitzer IRS. The fraction of observed sources ranges from ∼1% to 2% at the longest wavelengths to ∼10%–20% for Spitzer IRAC, Spitzer IRS, and IRAS 25 μm to ≳ 50% for W3, W4, and MIPS 24 μm measurements. With a fraction observed of zero for 500 μm SPIRE data with SNR ≥ 3, this point is not shown.

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