JADES Data Release 3 -- NIRSpec/MSA spectroscopy for 4,000 galaxies in the GOODS fields
JADES Data Release 3 -- NIRSpec/MSA spectroscopy for 4,000 galaxies in the GOODS fields
Apr 9, 2024·,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,
Francesco D'Eugenio
Alex J. Cameron
Jan Scholtz
Stefano Carniani
Chris J. Willott
Emma Curtis-Lake
Andrew J. Bunker
Eleonora Parlanti
Roberto Maiolino
Christopher N. A. Willmer
Peter Jakobsen
Brant E. Robertson
Benjamin D. Johnson
Sandro Tacchella
Phillip A. Cargile
Tim Rawle
Santiago Arribas
Jacopo Chevallard
Mirko Curti
Eiichi Egami
Daniel J. Eisenstein
Nimisha Kumari
Tobias J. Looser
Marcia J. Rieke
Bruno Rodrı́guez Del Pino
Aayush Saxena
Hannah Übler
Giacomo Venturi
Joris Witstok
William M. Baker
Rachana Bhatawdekar
Nina Bonaventura
Kristan Boyett
Stéphane Charlot
A. Lola Danhaive
Kevin N. Hainline
Ryan Hausen
Jakob M. Helton
Xihan Ji
Zhiyuan Ji
Gareth C. Jones
Ignas Joudžbalis
Michael v. Maseda
Pablo G. Pérez-González
Michele Perna
Dávid Puskás
Irene Shivaei
Maddie S. Silcock
Charlotte Simmonds
Renske Smit
Fengwu Sun
Natalia C. Villanueva
Christina C. Williams
Yongda Zhu
Abstract
We present the third data release of JADES, the JWST Advanced Deep Extragalactic Survey, providing both imaging and spectroscopy in the two GOODS fields. Spectroscopy consists of medium-depth and deep NIRSpec/MSA spectra of $4,000$
targets, covering the spectral range $0.6-5.3\ \mu\mathrm{m}$
and observed with both the low-dispersion prism ($R = 30-300$
) and all three medium-resolution gratings ($R = 500-1500$
). We describe the observations, data reduction, sample selection, and target allocation. We measured $2,375$
redshifts ($2,053$
from multiple emission lines); our targets span the range from $z = 0.5$
up to $z = 13$
, including $404$
at $z > 5$
. The data release includes two-dimensional and one-dimensional fully reduced spectra, with slit-loss corrections and background subtraction optimized for point sources. We also provide redshifts and $\mathrm{S/N} > 5$
emission-line flux catalogs for the prism and grating spectra, and concise guidelines on how to use these data products. Alongside spectroscopy, we are also publishing fully calibrated NIRCam imaging, which enables studying the JADES sample with the combined power of imaging and spectroscopy. Together, these data provide the largest statistical sample to date to characterize the properties of galaxy populations in the first billion years after the Big Bang.
Type
Publication
eprint arXiv:2404.06531
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