Author ORCID Identifier
Nicholas Foo: 0000-0002-7460-8460
Kevin C. Harrington: 0000-0001-5429-5762
Brenda Frye: 0000-0003-1625-8009
Patrick S. Kamieneski: 0000-0001-9394-6732
Min S. Yun: 0000-0001-7095-7543
Massimo Pascale: 0000-0002-2282-8795
Ilsang Yoon: 0000-0001-9163-0064
Allison Noble: 0000-0003-1832-4137
Rogier Windhorst: 0000-0001-8156-6281
Seth H. Cohen: 0000-0003-3329-1337
James D. Lowenthal: 0000-0001-9969-3115
Melanie Kaasinen: 0000-0002-1173-2579
Belén Alcalde Pampliega: 0000-0002-4140-0428
Daizhong Liu: 0000-0001-9773-7479
Olivia Cooper: 0000-0003-3881-1397
Carlos Garcia Diaz: 0000-0002-4223-2016
Anastasio Diaz-Sanchez: 0000-0003-0748-4768
Jose Diego: 0000-0001-9065-3926
Nikhil Garuda: 0000-0003-3418-2482
Eric F. Jiménez-Andrade: 0000-0002-2640-5917
Reagen Leimbach: 0009-0001-7446-2350
Amit Vishwas: 0000-0002-4444-8929
Q. Daniel Wang: 0000-0002-9279-4041
Dazhi Zhou: 0000-0002-6922-469X
Adi Zitrin: 0000-0002-0350-4488
Document Type
Article
Publication Date
12-19-2025
Publication Title
The Astrophysical Journal
Abstract
Investigating the processes by which galaxies rapidly build up their stellar mass during the peak of their star formation (z = 2–3) is crucial to advancing our understanding of the assembly of large-scale structures. We report the discovery of one of the most gas- and dust-rich protocluster core candidates, PJ0846+15 (J0846), from the Planck All-Sky Survey to Analyze Gravitationally lensed Extreme Starbursts (PASSAGES) sample. The exceedingly high total star formation rate (SFR) uncorrected for lensing magnification ( μ) of μSFR yr−1 is the result of a foreground cluster lensing at least 11 dusty star-forming galaxies between z = 2.660 and 2.669, where the intrinsic value is estimated to be SFR yr−1. Atacama Large Millimeter/submillimeter Array observations uncovered 18 CO(3–2) emission-line detections, some of which are multiply imaged systems, lensed by a foreground cluster at z = 0.77. We present the first multiwavelength characterization of this field, constructing a lens model that predicts that these 11 galaxies (μ ≃ 1.5–25) are contained within a projected physical extent of 280 × 150 kpc, with a velocity dispersion of σv = 246 ± 72 km s−1. J0846 exhibits the rare case of a protocluster candidate whose core is strongly lensed, offering a magnified view of the rapid stellar buildup within an overdense environment at Cosmic Noon.
Keywords
Protoclusters (1297), Strong gravitational lensing (1643), Starburst galaxies (1570), Galaxy evolution (594), Interstellar medium (847)
Volume
995
Issue
2
Creative Commons License

This work is licensed under a Creative Commons Attribution 4.0 International License.
Rights
© 2025. The Author(s). Published by the American Astronomical Society.
Version
Version of Record
Recommended Citation
Foo, Nicholas; Harrington, Kevin C.; Frye, Brenda L.; Kamieneski, Patrick S.; Yun, Min S.; Pascale, Massimo; Yoon, Ilsang; Noble, Allison; Windhorst, Rogier A.; Cohen, Seth H.; Lowenthal, James; Kaasinen, Melanie; Pampliega, Belén Alcalde; Liu, Daizhong; Cooper, Olivia; Garcia Diaz, Carlos; Diaz-Sanchez, Anastasio; Diego, Jose; Garuda, Nikhil; Jiménez-Andrade, Eric F.; Leimbach, Reagen; Vishwas, Amit; Wang, Q. Daniel; Zhou, Dazhi; and Zitrin, Adi, "PASSAGES: The Discovery of a Strongly Lensed Protocluster Core Candidate at Cosmic Noon" (2025). Astronomy: Faculty Publications, Smith College, Northampton, MA.
https://scholarworks.smith.edu/ast_facpubs/154
