JADES Data Release 4 Paper I : Sample Selection, Observing Strategy and Redshifts of the complete spectroscopic sample

Curtis-Lake, Emma, Cameron, Alex J., Bunker, Andrew J., Scholtz, Jan, Carniani, Stefano, Parlanti, Eleonora, D'Eugenio, Francesco, Jakobsen, Peter, Willmer, Christopher N. A., Arribas, Santiago, Baker, William M., Charlot, Stéphane, Chevallard, Jacopo, Circosta, Chiara, Curti, Mirko, Eisenstein, Daniel J., Hainline, Kevin, Ji, Zhiyuan, Johnson, Benjamin D., Jones, Gareth C., Maiolino, Roberto, Maseda, Michael V., Pérez-González, Pablo G., Rawle, Tim, Rieke, Marcia, Rinaldi, Pierluigi, Robertson, Brant, Pino, Bruno Rodrígez Del, Saxena, Aayush, Shivaei, Irene, Smit, Renske, Tacchella, Sandro, Übler, Hannah, Venturi, Giacomo, Willott, Chris and Duan, Qiao (2026) JADES Data Release 4 Paper I : Sample Selection, Observing Strategy and Redshifts of the complete spectroscopic sample. Monthly Notices of the Royal Astronomical Society (MNRAS), 549 (4). ISSN 0035-8711
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This paper accompanies Data Release 4 of the JWST Deep Extragalactic Survey (JADES), which presents the full NIRSpec spectroscopy of the survey. We provide spectra of 5190 targets across GOODS-North and GOODS-South (including the Hubble Ultra Deep Field), observed with the low-dispersion (R $\sim$ 30-300) prism and three medium-resolution (R $\sim$ 1000) gratings spanning 0.8 $< λ$ 4400 galaxies in the Medium tiers. Targets were selected from photometric redshifts or colours, with priority given to rest-UV-selected galaxies at $z > 5.7$ and F444W-selected galaxies at $1.5 < z < 5.7$. We describe the full target selection and present spectroscopic redshifts and success rates. In total we obtain robust redshifts for 3297 galaxies, including 396 at $z > 5.7$ and 2545 at $1.5 < z < 5.7$. To facilitate uniform analyses, we define 'gold' sub-samples based on UV- and F444W-selection. Using the parent samples and redshift success rates, we construct rest-UV luminosity functions at $6 \lesssim z \lesssim 9$ from the Medium- and Deep-JWST tiers. Our number densities agree well with previous determinations from both photometric and spectroscopic samples, with modest interloper fractions confirming the reliability of photometric UV-bright galaxy selections at these redshifts.


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