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The Optical/Near-Infrared Extinction Law in Highly Reddened Regions

Authors: Matthew W. Hosek Jr; Jessica R. Lu; Jay Anderson; Tuan Do; Edward F. Schlafly; Andrea M. Ghez; William I. Clarkson; +3 Authors

The Optical/Near-Infrared Extinction Law in Highly Reddened Regions

Abstract

A python code to generate the extinction law between 0.8 -- 2.2 microns as described in ''The Optical/Near-Infrared Extinction Law in Highly Reddened Regions'' by Hosek et al. (2018). The law is derived using the Westerlund 1 (Wd1) main sequence (A_Ks ~ 0.6 mag) and Arches cluster field Red Clump at the Galactic Center (A_Ks ~ 2.7 mag). To derive the law a Wd1 cluster age of 5 Myr is assumed, though changing the cluster age between 4 Myr -- 7 Myr has no effect on the law. This extinction law can be applied to highly reddened stellar populations that have similar foreground material as Wd1 and the Arches RC, namely dust from the spiral arms of the Milky Way in the Galactic Plane.

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selected citations
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This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
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