Published August 2, 2021
| Version 1.0
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The Outer Stellar Mass of Massive Galaxies: A Simple Tracer of Halo Mass with Scatter Comparable to Richness and Reduced Projection Effects
Description
These are the data for reproducing the results of the publication titled "The Outer Stellar Mass of Massive Galaxies: A Simple Tracer of Halo Mass with Scatter Comparable to Richness and Reduced Projection Effects" by Song Huang et al.
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The record is publicly accessible, but files are restricted to users with access.
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Funding
- Collaborative Research: Connecting the Smallest and the Largest Galaxies to their Dark Matter Halos 1714610
- U.S. National Science Foundation
- Kavli Institute for Theoretical Physics 1748958
- U.S. National Science Foundation
- Kavli Institute for Theoretical Physics 1125915
- U.S. National Science Foundation