Slide to compare HST and JWST
Use the handle to sweep between the legacy HST color image and our JWST color composite. Full-resolution FITS images are linked below.
Image Comparison
JWSTHST
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assets/hst_xlssc.png and assets/jwst_xlssc.png (case‑sensitive).Data Description
The images above show the galaxy cluster XLSSC 122 at a redshift of z=1.98.
A distant look into the past
JWST's deep imaging provides an exceptionally detailed look at this distant cluster, with a limiting magnitude of 30.9 in the deepest filter.
JWST's deep imaging provides an exceptionally detailed look at this distant cluster, with a limiting magnitude of 30.9 in the deepest filter.
Imaging & processing
The JWST mosaics are resampled with a pixel scale of 0.02 arcsec/pixel using the JWST Science Calibration Pipeline, with systematic effects corrected with the Yonsei Observable UNiverse Group JWST pipeline
The JWST mosaics are resampled with a pixel scale of 0.02 arcsec/pixel using the JWST Science Calibration Pipeline, with systematic effects corrected with the Yonsei Observable UNiverse Group JWST pipeline
Notable features
The JWST imaging reveals two remarkable features: asymmetric ICL suggesting ongoing merger activity, and strong lensing arcs that signal a highly concentrated cluster core.
The JWST imaging reveals two remarkable features: asymmetric ICL suggesting ongoing merger activity, and strong lensing arcs that signal a highly concentrated cluster core.
Data Access
Products
- NIRCam mosaics (F090W, F200W, F277W, F356W)
- Weight maps
How to Cite
Please cite the data DOI and our paper. Example BibTeX:
@dataset{Scofield2025JWSTRelease,
author = {Scofield, Zachary and Collaborators},
title = {JWST Cluster Field Data Release},
year = {2025},
publisher = {Zenodo},
doi = {10.5281/zenodo.16810356},
}
@ARTICLE{2025arXiv250808356F,
author = {{Finner}, Kyle and {Cha}, Sangjun and {Scofield}, Zachary P. and {Jee}, M. James and {Lin}, Yu-heng and {Joo}, Hyungjin and {Park}, Hyosun and {Morishita}, Takahiro and {Faisst}, Andreas and {Lee}, Bomee and {Wang}, Wuji and {Chary}, Ranga-Ram},
title = "{JWST Discovery of Strong Lensing from a Galaxy Cluster at Cosmic Noon: Giant Arcs and a Highly Concentrated Core of XLSSC 122}",
journal = {arXiv e-prints},
keywords = {Astrophysics of Galaxies, Cosmology and Nongalactic Astrophysics},
year = 2025,
month = aug,
eid = {arXiv:2508.08356},
pages = {arXiv:2508.08356},
doi = {10.48550/arXiv.2508.08356},
archivePrefix = {arXiv},
eprint = {2508.08356},
primaryClass = {astro-ph.GA},
adsurl = {https://ui.adsabs.harvard.edu/abs/2025arXiv250808356F},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
About
This page is a lightweight, static site designed for GitHub Pages. Images are previews; for scientific work use the FITS files provided in the archive.