JADES NIRSpec initial data release for the  Hubble  Ultra Deep Field

Bunker, Andrew J.; Cameron, Alex J.; Curtis-Lake, Emma; Jakobsen, P.; Carniani, Stefano; Curti, Mirko; Witstok, Joris; Maiolino, R.; D’Eugenio, Francesco; Looser, Tobias J.; Willott, Chris J.; Bonaventura, Nina; Hainline, Kevin; Übler, Hannah; Willmer, Christopher N. A.; Saxena, Aayush; Smit, Renske; Alberts, Stacey; Arribas, Santiago; Baker, William; Baum, Stefi A.; Bhatawdekar, Rachana; Bowler, R. A. A.; Boyett, Kristan; Charlot, S.; Chen, Zuyi; Chevallard, Jacopo; Circosta, Chiara; DeCoursey, Christa; Graaff, Anna de; Egami, Eiichi; Eisenstein, Daniel J.; Endsley, Ryan; Ferruit, Pierre; Giardino, Giovanna; Hausen, Ryan; Helton, Jakob M.; Hviding, Raphael E.; Ji, Zhiyuan; Johnson, Benjamin D.; Jones, Gareth C.; Kumari, Nimisha; Laseter, Isaac; Lützgendorf, Nora; Maseda, Michael V.; Nelson, Erica J.; Parlanti, Eleonora; Perna, Michele; Rauscher, Bernard J.; Rawle, Tim; Rix, Hans‐Walter; Rieke, Marcia; Robertson, Brant; Pino, Bruno Rodríguez Del; Sandles, Lester; Scholtz, Jan; Sharpe, Katherine; Skarbinski, Maya; Stark, Daniel P.; Sun, Fengwu; Tacchella, Sandro; Topping, Michael W.; Villanueva, Natalia C.; Wallace, Imaan E. B.; Williams, Christina C.; Woodrum, Charity

doi:10.1051/0004-6361/202347094

articleAstronomy and AstrophysicsSep 9, 2024DIAMOND OA

JADES NIRSpec initial data release for the Hubble Ultra Deep Field

AJAndrew J. Bunker AJAlex J. Cameron ECEmma Curtis-Lake PJP. Jakobsen SCStefano Carniani

University of Oxford · University of Hertfordshire · +31 more institutions

Indexed incrossrefdoaj

Abstract

We describe the NIRSpec component of the JWST Deep Extragalactic Survey (JADES), and provide deep spectroscopy of 253 sources targeted with the NIRSpec micro-shutter assembly in the Hubble Ultra Deep Field and surrounding GOODS-South. The multi-object spectra presented here are the deepest so far obtained with JWST, amounting to up to 28 hours in the low-dispersion ( R ~30–300) prism, and up to 7 hours in each of the three medium-resolution R ≈ 1000 gratings and one high-dispersion grating, G395H ( R ≈ 2700). Our low-dispersion and medium-dispersion spectra cover the wavelength range 0.6–5.3 μm. We describe the selection of the spectroscopic targets, the strategy for the allocation of targets to…

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Keywords

Physics
Astrophysics
Redshift
Galaxy
Astronomy
Line (geometry)
Spectroscopy
Hubble Deep Field

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