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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 11.

Comparison of the input and best-fit parameters of the mock DIB profiles: (a) amplitude |A0|, (b) central wavelength λ0, and (c) profile width σ0. The top panels show the direct comparison and the 1:1 relation (dashed line), and the bottom panels show the difference (Δ = input-fit) as a function of input parameter. The contours enclose 50%, 75%, and 90% of the sample. Also shown are median fractional differences for A0 and σ0, the median absolute difference for λ0, and the dispersion in each case.

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