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Stellar Populations and Molecular Gas Composition in the Low-metallicity Environment of WLM

  • Authors: Haylee N. Archer, Deidre A. Hunter, Bruce G. Elmegreen, Leslie K. Hunt, Rosalia O'Brien, Elias Brinks, Phil Cigan, Monica Rubio, Rogier A. Windhorst, Rolf A. Jansen, Elijah P. Mathews

Haylee N. Archer et al 2025 The Astronomical Journal 169 .

  • Provider: AAS Journals

Caption: Figure 3.

The difference between output and input magnitudes as a function of input magnitude for all artificial stars generated in the artificial star tests for each filter. The solid red horizontal line represents where the input and output magnitudes are identical, while the dashed red vertical line marks the faintest magnitude in that filter observed in the final matched catalog of stars.

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