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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 9.

Confusion matrices for all eight model configurations, normalized to the number of objects tested in each “True Label” category (see Table 3 for the number of objects in each class). The numbers below the percentages are the average and standard deviation of the model agreement in each quadrant. Left: confusion matrices for models that include F150W and Paα data in training. Right: confusion matrices for models which exclude F150W and Paα data in training.

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