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The NIRISS PASSAGE Spectroscopic Redshift Catalog in COSMOS

Abstract:
We present the Parallel Application of Slitless Spectroscopy to Analyze Galaxy Evolution (PASSAGE) spectroscopic redshift catalog in the COSMOS field. PASSAGE is a JWST Cycle 1 Near Infrared Imager and Slitless Spectrograph (or NIRISS) wide-field slitless spectroscopy pure-parallel survey, obtaining near-infrared spectra of thousands of extragalactic sources. Fifteen out of 63 PASSAGE fields fall within the Hubble Space Telescope COSMOS footprint, of which 11 overlap with COSMOS-Web, a JWST treasury survey providing additional space-based photometry. We present our custom line-finding algorithm and visual inspection effort used to identify emission lines and derive the spectroscopic redshifts for line-emitting sources in PASSAGE. The line-finding algorithm identifies between ∼200 and 950 line-emitting candidates per field, of which typically 47% were identified as true emission lines post visual inspection. We identify 2183 emission-line sources at 0.08 ≲ z ≲ 4.7, 1896 of which have available COSMOS photometric redshifts. We find excellent redshift agreement between the COSMOS photometric redshifts and the PASSAGE spectroscopic redshifts for strong (signal-to-noise ratio > 5), multi-line-emitting sources. This agreement weakens for PASSAGE single-line emitters with ambiguous identities. These single-line emitters are likely misidentified around 18% of the time based on comparisons to photometric redshifts. We derive stellar masses using PASSAGE photometry and spectroscopic redshifts, in broad agreement with existing COSMOS-Web stellar masses, but with some discrepancy driven by redshift disagreements. We publicly release this spectroscopic redshift catalog, which will enable community-led science in prime extragalactic fields and serve as a crucial dataset for validating Euclid and Roman spectroscopy.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.3847/1538-4365/ae6777

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Author
ORCID:
0009-0002-9932-4461
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Author
ORCID:
0000-0001-5294-8002
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ORCID:
0000-0002-0364-1159
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ORCID:
0000-0001-7166-6035
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Author
ORCID:
0000-0002-9136-8876


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Funder identifier:
10.13039/100000104
Grant:
JWST-GO-1571


Publisher:
American Astronomical Society
Journal:
The Astrophysical Journal: Supplement Series More from this journal
Volume:
284
Issue:
2
Pages:
64
Article number:
64
Publication date:
2026-06-02
Acceptance date:
2026-04-28
DOI:
EISSN:
1538-4365
ISSN:
0067-0049


Language:
English
Keywords:
Source identifiers:
4104675
Deposit date:
2026-06-02
ARK identifier:
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