PASSAGE releases 2183 spectroscopic redshifts (0.08<z<4.7) from JWST NIRISS observations in COSMOS, with strong agreement to photometric redshifts for multi-line sources and a quantified ~18% misidentification rate for single-line emitters.
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3 Pith papers cite this work. Polarity classification is still indexing.
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Spectroscopic confirmation of one luminous z=7.96 Lyman break galaxy in a 4.8 arcmin² COSMOS field implies a surface density of 0.21 arcmin⁻², about 10 times higher than wide-area surveys and hinting at a z~8 overdensity.
Hα luminosity functions at z~1.3 and z~2.0 yield faint-end slopes of -1.50 and -1.60, with integrated SFR densities of 0.097 and 0.129 M⊙ yr⁻¹ Mpc⁻³ from a sample of 99 emitters.
citing papers explorer
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The NIRISS PASSAGE Spectroscopic Redshift Catalog in COSMOS
PASSAGE releases 2183 spectroscopic redshifts (0.08<z<4.7) from JWST NIRISS observations in COSMOS, with strong agreement to photometric redshifts for multi-line sources and a quantified ~18% misidentification rate for single-line emitters.
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Validating z > 7.5 Lyman Break Galaxy candidates in the COSMOS field with JWST/PASSAGE
Spectroscopic confirmation of one luminous z=7.96 Lyman break galaxy in a 4.8 arcmin² COSMOS field implies a surface density of 0.21 arcmin⁻², about 10 times higher than wide-area surveys and hinting at a z~8 overdensity.
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The GLASS-JWST Early Release Science Program. V. H$\alpha$ luminosity functions at $z\sim1.3$ and $z\sim2.0$
Hα luminosity functions at z~1.3 and z~2.0 yield faint-end slopes of -1.50 and -1.60, with integrated SFR densities of 0.097 and 0.129 M⊙ yr⁻¹ Mpc⁻³ from a sample of 99 emitters.