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PAH Marks the Spot: Digging for Buried Clusters in Nearby Star-forming Galaxies

  • Authors: Gabrielle B. Graham, Daniel A. Dale, Chase L. Smith, Elisabeth Brann, Kaycee D. Conder, Samuel Crowe, Sumitra Dhileepkumar, Nicole A. Imming, Emilio Mendez, Zachary Pleska, Kelsey Sako, Amirnezam Amiri, Ashley T. Barnes, Médéric Boquien, Rupali Chandar, Ryan Chown, Oleg Y. Gnedin, Kathryn Grasha, Stephen Hannon, Hamid Hassani, Rémy Indebetouw, Hwihyun Kim, Jaeyeon Kim, Hannah Koziol, Kirsten L. Larson, Janice C. Lee, Adam K. Leroy, Elias K. Oakes, M. Jimena Rodríguez, Erik Rosolowsky, Karin Sandstrom, Eva Schinnerer, Jessica Sutter, David A. Thilker, Leonardo Ubeda, Bradley C. Whitmore, Tony D. Weinbeck, Thomas G. Williams, Aida Wofford, J. Eduardo Méndez-Delgado, Qiushi Chris Tian

Gabrielle B. Graham et al 2025 The Astronomical Journal 170 .

  • Provider: AAS Journals

Caption: Figure 8.

A histogram of the distribution of masses for the subset of 186 embedded cluster candidates with an F150W peak pixel S/N > 5. There are two sources with mass estimates below 102 M not shown. The maroon error bars show the 1σ standard deviations from Monte Carlo simulations for each bin with at least one embedded cluster candidate.

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