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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 8.

Relation between the Gaia spectral index IB and the B V color. The upper x-axis relates spectral types of main-sequence stars to BV (M. J. Pecaut & E. E. Mamajek 2013). Gray points: all 2527 stars with Gaia spectra, BV colors, and no saturation issues; black, yellow, and gold points: 1195 stars with d ≤ 80 pc. The cyan curve is the best-fitting polynomial to the 80 pc data (Equations (4)–(5)). The clear correlation between IB and BV enables spectral classification with an accuracy of ±0.5–0.75 subclass.

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