The PANORAMIC Survey: Pure Parallel Wide Area Legacy Imaging with JWST/NIRCam
Abstract We present the PANORAMIC survey, a pure parallel extragalactic imaging program with JWST/NIRCam observed during Cycle 1. The survey obtained ∼530 square arcmin of NIRCam imaging from 1–5 μ m, totaling ∼192 hr of science integration time. This represents the largest on-sky time investment of any Cycle 1 GO extragalactic NIRCam imaging program by nearly a factor of 2. The survey includes ∼432 square arcmin of novel sky area not yet observed with JWST using at least six NIRCam broadband filters, increasing the existing area covered by similar Cycle 1 data by ∼60%. Additionally, 70 square arcmin was also covered by a seventh filter (F410M). A fraction of PANORAMIC data (∼200 square arcmin) was obtained in or around extragalactic deep fields, enhancing their legacy value. Pure parallel observing naturally creates a “wedding cake” survey with both wide and ultra-deep tiers, with 5 σ point-source depths at F444W ranging from 27.8–29.4 (ABmag), and with minimized cosmic variance. The ≳6-filter strategy yields remarkably good photometric redshift performance, achieving similar median scatter and outlier fraction as CANDELS ( σ NMAD ∼ 0.07; η ∼ 0.2), enabling a wealth of science across redshift without need for follow-up or ancillary data. We overview the proposed survey, the data obtained as part of this program, and document the science-ready data products in the data release. PANORAMIC has delivered wide-area and deep imaging with excellent photometric performance, demonstrating that pure parallel observations with JWST are a highly efficient observing mode that is key to acquiring a complete picture of galaxy evolution from rare bright galaxies to fainter, more abundant sources across redshifts.
Authors
- Pratika Dayal (ORCID: https://orcid.org/0000-0001-8460-1564)
- Zhiyuan Ji (ORCID: https://orcid.org/0000-0001-7673-2257)
- Marijn Franx (ORCID: https://orcid.org/0000-0002-8871-3026)
- Laia Barrufet (ORCID: https://orcid.org/0000-0003-1641-6185)
- Rachel Bezanson (ORCID: https://orcid.org/0000-0001-5063-8254)
- Jenny E. Greene (ORCID: https://orcid.org/0000-0002-5612-3427)
- Ivo Labbé (ORCID: https://orcid.org/0000-0002-2057-5376)
- Christina C. Williams (ORCID: https://orcid.org/0000-0003-2919-7495)
- Aidan P. Cloonan (ORCID: https://orcid.org/0000-0001-9978-2601)
- R. A. A. Bowler (ORCID: https://orcid.org/0000-0003-3917-1678)
- Pascal A. Oesch (ORCID: https://orcid.org/0000-0001-5851-6649)
- Gabriel Brammer (ORCID: https://orcid.org/0000-0003-2680-005X)
- Michael V. Maseda (ORCID: https://orcid.org/0000-0003-0695-4414)
- Anne Hutter (ORCID: https://orcid.org/0000-0003-3760-461X)
- Katherine E. Whitaker (ORCID: https://orcid.org/0000-0001-7160-3632)
- Mengyuan Xiao (ORCID: https://orcid.org/0000-0003-1207-5344)
- Sinclaire M. Manning (ORCID: https://orcid.org/0000-0003-0415-0121)
- Andrea Weibel (ORCID: https://orcid.org/0000-0001-8928-4465)
Publication Details
- Journal
- The Astrophysical Journal
- Published
- 2025-01-22
- DOI
- https://doi.org/10.3847/1538-4357/ad97bc
- Citations
- 13
- Primary Topic
- Gamma-ray bursts and supernovae
- Type
- article
- Field-Weighted Citation Impact
- 15.01
Funders
- National Science Foundation
- U.S. Department of Energy
- National Aeronautics and Space Administration
- Aspen Center for Physics
- Villum Fonden
- Space Telescope Science Institute
- European Commission
- National Research Foundation
- Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung
- Rijksuniversiteit Groningen
- Danmarks Grundforskningsfond
- Chinese Academy of Sciences
- Nederlandse Organisatie voor Wetenschappelijk Onderzoek
- Office of Science
- Science and Technology Facilities Council
- Staatssekretariat für Bildung, Forschung und Innovation
- Division of Astronomical Sciences
- High Energy Physics