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Mapping the Interstellar Medium with Near-infrared Diffuse Interstellar Bands

  • Authors: G. Zasowski, B. Ménard, D. Bizyaev, D. A. García-Hernández, A. E. García Pérez, M. R. Hayden, J. Holtzman, J. A. Johnson, K. Kinemuchi, S. R. Majewski, D. L. Nidever, M. Shetrone, and J. C. Wilson

Zasowski et al. 2015 The Astrophysical Journal 798 35.

  • Provider: AAS Journals

Caption: Figure 12.

WDIB completeness estimate over the A0 and σ0 ranges tested using mock DIB features. The blue shaded panel indicates the fraction of well-detected features in the input A0 − σ0 field (see the text). Bottom: completeness as a function of |A0|, averaged over the range of input σ0 (black) and for three sample σ0 values (blue: 0.9 Å, green: 3.6 Å, red: 7.5 Å). Right: completeness as a function of σ0, averaged over the range of input |A0| (black) and for three sample |A0| values (blue: 0.02, green: 0.05, red: 0.09).

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