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The PHANGS–JWST Treasury Survey: Star Formation, Feedback, and Dust Physics at High Angular Resolution in Nearby GalaxieS


Abstract The PHANGS collaboration has been building a reference data set for the multiscale, multiphase study of star formation and the interstellar medium (ISM) in nearby galaxies. With the successful launch and commissioning of JWST, we can now obtain high-resolution infrared imaging to probe the youngest stellar populations and dust emission on the scales of star clusters and molecular clouds (∼5–50 pc). In Cycle 1, PHANGS is conducting an eight-band imaging survey from 2 to 21 μ m of 19 nearby spiral galaxies. Optical integral field spectroscopy, CO(2–1) mapping, and UV-optical imaging for all 19 galaxies have been obtained through large programs with ALMA, VLT-MUSE, and Hubble. PHANGS–JWST enables a full inventory of star formation, accurate measurement of the mass and age of star clusters, identification of the youngest embedded stellar populations, and characterization of the physical state of small dust grains. When combined with Hubble catalogs of ∼10,000 star clusters, MUSE spectroscopic mapping of ∼20,000 H ii regions, and ∼12,000 ALMA-identified molecular clouds, it becomes possible to measure the timescales and efficiencies of the earliest phases of star formation and feedback, build an empirical model of the dependence of small dust grain properties on local ISM conditions, and test our understanding of how dust-reprocessed starlight traces star formation activity, all across a diversity of galactic environments. Here we describe the PHANGS–JWST Treasury survey, present the remarkable imaging obtained in the first few months of science operations, and provide context for the initial results presented in the first series of PHANGS–JWST publications.
Authors Janice Lee ORCID , Karin Sandström ORCID , Adam K. Leroy ORCID , David A. Thilker ORCID , E. Schinnerer ORCID , Erik Rosolowsky ORCID , Kirsten L. Larson ORCID , Oleg V. Egorov ORCID , Thomas G. Williams ORCID , J. Schmidt ORCID , Éric Emsellem ORCID , Gagandeep S. Anand ORCID , Ashley T. Barnes ORCID , Francesco Belfiore ORCID , Ivana Bešlić ORCID , Frank Bigiel ORCID , Guillermo A. Blanc ORCID , Alberto D. Bolatto ORCID , M. Boquien ORCID , Jakob S. den Brok ORCID , Yixian Cao ORCID , Rupali Chandar ORCID , Jérémy Chastenet ORCID , Mélanie Chevance ORCID , I-Da Chiang ORCID , Enrico Congiu ORCID , Daniel A. Dale University of WyomingORCID , Sinan Deger ORCID , Cosima Eibensteiner ORCID , Christopher M. Faesi ORCID , Simon C. O. Glover ORCID , Kathryn Grasha ORCID , Brent Groves ORCID , Hamid Hassani ORCID , Kiana F. Henny University of WyomingORCID , Jonathan D. Henshaw ORCID , Nils Hoyer ORCID , Annie Hughes ORCID , Sarah Jeffreson ORCID , María J. Jiménez-Donaire ORCID , Jaeyeon Kim ORCID , Hwi Kim ORCID , Ralf S. Klessen ORCID , Eric W. Koch ORCID , Kathryn Kreckel ORCID , J. M. Diederik Kruijssen ORCID , Jing Li ORCID , Daizhong Liu ORCID , Laura A. Lopez ORCID , Daniel Maschmann ORCID , Ness Mayker Chen ORCID , Sharon E. Meidt ORCID , E. J. Murphy ORCID , Justus Neumann ORCID , Nadine Neumayer ORCID , Hsi-An Pan ORCID , Ismael Pessa ORCID , J. Pety ORCID , Miguel Querejeta ORCID , Francesca Pinna ORCID , M.M. Rodríguez ORCID , Tomoka Tosaki ORCID , P. Sánchez-Blázquez ORCID , Francesco Santoro ORCID , Amy Sardone ORCID , Rowan J. Smith ORCID , Mattia C. Sormani ORCID , Fabian Scheuermann ORCID , Sophia K. Stuber ORCID , Jessica Sutter ORCID , Jiayi Sun ORCID , Yu-Hsuan Teng ORCID , Robin G. Treß ORCID , A. Usero ORCID , Elizabeth J. Watkins ORCID , Bradley C. Whitmore ORCID , Alessandro Razza ORCID
Journal Info IOP Publishing | The Astrophysical Journal Letters , vol: 944 , iss: 2 , pages: L17 - L17
Publication Date 2/1/2023
ISSN 2041-8205
TypeKeyword Image article
Open Access gold Gold Access
DOI https://doi.org/10.3847/2041-8213/acaaae
KeywordsKeyword Image High-Temperature Molecular Spectroscopy (Score: 0.506396)