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CANUCS/Technicolor data release 1: imaging, photometry, slit spectroscopy, and stellar population parameters
ID
Sarrouh, Ghassan T. E.
(
Author
),
ID
Martis, Nicholas S.
(
Author
),
ID
Rihtaršič, Gregor
(
Author
),
ID
Bradač, Maruša
(
Author
),
ID
Felicioni, Giordano
(
Author
),
ID
Harshan, Anishya
(
Author
),
ID
Judež, Jon
(
Author
),
ID
Markov, Vladan
(
Author
),
ID
Tripodi, Roberta
(
Author
), et al.
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URL - Source URL, Visit
https://iopscience.iop.org/article/10.3847/1538-4365/ae1611
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Abstract
We present the first data release of the Canadian NIRISS Unbiased Cluster Survey (CANUCS), a JWST Cycle 1 GTO program targeting five lensing clusters and flanking fields in parallel (A370, MACS0416, MACS0417, MACS1149, and MACS1423; survey area ∼100 arcmin$^2$), with NIRCam imaging, NIRISS slitless spectroscopy, and NIRSpec prism multiobject spectroscopy. Fields centered on cluster cores include imaging in eight bands from 0.9–4.4 μm, alongside continuous NIRISS coverage from 1.15–2 μm, while the NIRCam flanking fields provide five wide-band and nine medium-band filters for exceptional spectral sampling, all to ∼29 mag$_{AB}$. We also present JWST in Technicolor, a Cycle 2 follow-up GO program targeting three CANUCS clusters (A370, MACS0416, and MACS1149). The Technicolor program adds NIRISS slitless spectroscopy in F090W to the cluster fields while adding eight wide-, medium-, and narrowband filters to the flanking fields. This provides NIRCam imaging in all wide- and medium-band filters over ∼30 arcmin$^2$. This paper describes our data reduction and photometry methodology. We release NIRCam, NIRISS, and Hubble Space Telescope imaging, point-spread functions (PSFs), PSF-matched imaging, photometric catalogs, and photometric and spectroscopic redshifts. We provide lens models and stellar population parameters in up to 19 filters for ∼53,000 galaxies in the cluster fields, and ∼44,000 galaxies in up to 29 filters in the flanking fields. We further present 733 NIRSpec spectra and redshift measurements up to z = 10.8. Comparing against our photometric redshifts, we find catastrophic outlier rates of only 4%–7% and scatter of $\sigma_{\mathrm{NMAD}}$ of 0.01–0.03.
Language:
English
Keywords:
galaxy evolution
,
sky surveys
,
photometry
,
spectroscopy
,
galaxy clusters
Work type:
Article
Typology:
1.01 - Original Scientific Article
Organization:
FMF - Faculty of Mathematics and Physics
Publication status:
Published
Publication version:
Version of Record
Year:
2026
Number of pages:
45 str.
Numbering:
Vol. 282, no. 1, art. no. 3
PID:
20.500.12556/RUL-178333
UDC:
524.8
ISSN on article:
1538-4365
DOI:
10.3847/1538-4365/ae1611
COBISS.SI-ID:
265852419
Publication date in RUL:
23.01.2026
Views:
501
Downloads:
401
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Record is a part of a journal
Title:
The Astrophysical journal : supplement series
Shortened title:
Astrophys. j., suppl. ser.
Publisher:
University of Chicago Press for the American Astronomical Society
ISSN:
1538-4365
COBISS.SI-ID:
515080217
Licences
License:
CC BY 4.0, Creative Commons Attribution 4.0 International
Link:
http://creativecommons.org/licenses/by/4.0/
Description:
This is the standard Creative Commons license that gives others maximum freedom to do what they want with the work as long as they credit the author.
Secondary language
Language:
Slovenian
Keywords:
razvoj galaksij
,
pregledi neba
,
fotometrija
,
spektroskopija
,
jate galaksij
Projects
Funder:
EC - European Commission
Project number:
101053208
Name:
Exploring Cosmic Dawn with James Webb Space Telescope
Acronym:
FIRSTLIGHT
Funder:
ARIS - Slovenian Research and Innovation Agency
Project number:
N1-0238
Name:
Raziskave kozmične zore z James Webb vesoljskim teleskopom
Funder:
ARIS - Slovenian Research and Innovation Agency
Project number:
P1-0188
Name:
Astrofizika in fizika atmosfere
Funder:
Other - Other funder or multiple funders
Funding programme:
Space Telescope Science Institute
Project number:
HST-GO-16667
Name:
The Final Frontier: HST and JWST Exploration of Galaxies Across Cosmic Epochs
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