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JWST Early Release Science Program TEMPLATES: Targeting Extremely Magnified Panchromatic Lensed Arcs and Their Extended Star Formation

  • Authors: Jane R. Rigby, Joaquin D. Vieira, Kedar A. Phadke, Taylor A. Hutchison, Brian Welch, Jared Cathey, Justin S. Spilker, Anthony H. Gonzalez, Prasanna Adhikari, M. Aravena, Matthew B. Bayliss, Jack E. Birkin, Emmy Bursk, Scott C. Chapman, Håkon Dahle, Lauren A. Elicker, Travis C. Fischer, Michael K. Florian, Michael D. Gladders, Christopher C. Hayward, Rose Hewald, Lily A. Kettler, Gourav Khullar, Seonwoo Kim, David R. Law, Guillaume Mahler, Sangeeta Malhotra, Eric J. Murphy, Desika Narayanan, Grace M. Olivier, James E. Rhoads, Keren Sharon, Manuel Solimano, Athish Thiruvengadam, David Vizgan, Nikolas Younker

Jane R. Rigby et al 2025 The Astrophysical Journal 978 .

  • Provider: AAS Journals

Caption: Figure 1.

The TEMPLATES sample. The HST filters used were F390W, F775W, and F110W for SGAS1723+34; F606W, F814W, and F110W for SGAS1226+21; and F140W for the two SMGs. The ALMA band is the rest-frame 160 μm continuum. A 3″ scale bar is shown to illustrate the approximate size of the NIRSpec integral field unit (IFU) field of view (FOV). The TEMPLATES galaxies are all highly magnified, with sizes that fit in the FOVs of the JWST IFUs. The sources are all aligned with north up and east left.

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