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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 13.

Example ideal cluster candidates as seen in the Zooniverse interface (left), a three-color NIRCam image (center), and a three-color HST image (right). From top to bottom, we show one candidate from NGC 1097, NGC 1559, NGC 2775, and NGC 2997. The four cutouts in the left panel are 2﹩\mathop{.}\limits^{^{\prime\prime} }﹩0 cutouts centered on the source using the same images as Figure 2, with the cyan circle denoting the final F335M source center. The three-color images also display a 2﹩\mathop{.}\limits^{^{\prime\prime} }﹩0 cutout centered on the source. The individual bands are shown in the small boxes above the composite image.

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