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The JADES Origins Field: A New JWST Deep Field in the JADES Second NIRCam Data Release

Abstract:
We summarize the properties and initial data release of the JADES Origins Field (JOF), the longest single pointing yet imaged with the James Webb Space Telescope (JWST). This field falls within the GOODS-S region about 8′ southwest of the Hubble Ultra Deep Field (HUDF), where it was formed initially in Cycle 1 as a parallel field of HUDF spectroscopic observations within the JWST Advanced Deep Extragalactic Survey (JADES). This imaging was greatly extended in Cycle 2 program 3215, which observed the JOF for 5 days in six medium-band filters, seeking robust candidates for z > 15 galaxies. This program also includes ultradeep parallel NIRSpec spectroscopy (up to 91 hr on source, summing over the dispersion modes) on the HUDF. Cycle 3 observations from program 4540 added 20 hr of NIRCam slitless spectroscopy and F070W imaging to the JOF. With these three campaigns, the JOF was observed for 380 open-shutter hours with NIRCam using 15 imaging filters and two grism bandpasses. Further, parts of the JOF have deep 43 hr MIRI observations in F770W. Taken together, the JOF is one of the most compelling deep fields available with JWST and a powerful window into the early Universe. This paper presents the second data release from JADES, featuring the imaging and catalogs from the year 1 JOF observations.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.3847/1538-4365/ae1137

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Author
ORCID:
0000-0002-2929-3121
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Author
ORCID:
0000-0002-9280-7594
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ORCID:
0000-0002-4271-0364
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ORCID:
0000-0002-8224-4505
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ORCID:
0000-0003-4565-8239


Publisher:
American Astronomical Society
Journal:
The Astrophysical Journal: Supplement Series More from this journal
Volume:
281
Issue:
2
Article number:
50
Publication date:
2025-12-01
Acceptance date:
2025-10-07
DOI:
EISSN:
1538-4365
ISSN:
0067-0049


Language:
English
Keywords:
Pubs id:
2347507
Local pid:
pubs:2347507
Source identifiers:
3523688
Deposit date:
2025-12-01
ARK identifier:
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