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A 3D Dust Map Based on Gaia, Pan-STARRS 1, and 2MASS

  • Authors: Gregory M. Green, Edward Schlafly, Catherine Zucker, Joshua S. Speagle, and Douglas Finkbeiner

2019 The Astrophysical Journal 887 93.

  • Provider: AAS Journals

Caption: Figure 10.

Histogram of the residuals of our new map with Bayestar17, as a function of the SFD reddening. Both maps are integrated to infinite distance. The left panel compares our uncorrelated map (initial iteration) with Bayestar17, while the right panel compares our correlated map (final iteration) with Bayestar17. All reddenings are in magnitudes of ﹩E\left(g-r\right)﹩.

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