Overview of the JWST Advanced Deep Extragalactic Survey (JADES)
Overview of the JWST Advanced Deep Extragalactic Survey (JADES)
Jun 4, 2023·,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,,
Daniel J. Eisenstein
Chris Willott
Stacey Alberts
Santiago Arribas
Nina Bonaventura
Andrew J. Bunker
Alex J. Cameron
Stefano Carniani
Stephane Charlot
Emma Curtis-Lake
Francesco D'Eugenio
Ryan Endsley
Pierre Ferruit
Giovanna Giardino
Kevin Hainline
Ryan Hausen
Peter Jakobsen
Benjamin D. Johnson
Roberto Maiolino
Marcia Rieke
George Rieke
Hans-Walter Rix
Brant Robertson
Daniel P. Stark
Sandro Tacchella
Christina C. Williams
Christopher N. A. Willmer
William M. Baker
Stefi Baum
Rachana Bhatawdekar
Kristan Boyett
Zuyi Chen
Jacopo Chevallard
Chiara Circosta
Mirko Curti
A. Lola Danhaive
Christa DeCoursey
Anna De Graaff
Alan Dressler
Eiichi Egami
Jakob M. Helton
Raphael E. Hviding
Zhiyuan Ji
Gareth C. Jones
Nimisha Kumari
Nora Lützgendorf
Isaac Laseter
Tobias J. Looser
Jianwei Lyu
Michael v. Maseda
Erica Nelson
Eleonora Parlanti
Michele Perna
Dávid Puskás
Tim Rawle
Bruno Rodrı́guez Del Pino
Lester Sandles
Aayush Saxena
Jan Scholtz
Katherine Sharpe
Irene Shivaei
Maddie S. Silcock
Charlotte Simmonds
Maya Skarbinski
Renske Smit
Meredith Stone
Katherine A. Suess
Fengwu Sun
Mengtao Tang
Michael W. Topping
Hannah Übler
Natalia C. Villanueva
Imaan E. B. Wallace
Lily Whitler
Joris Witstok
Charity Woodrum
Abstract
We present an overview of the James Webb Space Telescope (JWST) Advanced Deep Extragalactic Survey (JADES), an ambitious program of infrared imaging and spectroscopy in the GOODS-S and GOODS-N deep fields, designed to study galaxy evolution from high redshift to cosmic noon. JADES uses about $770$
hours of Cycle $1$
guaranteed time largely from the Near-Infrared Camera (NIRCam) and Near-Infrared Spectrograph (NIRSpec) instrument teams. In GOODS-S, in and around the Hubble Ultra Deep Field and Chandra Deep Field South, JADES produces a deep imaging region of $\sim 45\ \mathrm{arcmin}^{2}$
with an average of $\sim 130\ \mathrm{hours}$
of exposure time spread over $9$
NIRCam filters. This is extended at medium depth in GOODS-S and GOODS-N with NIRCam imaging of $\sim 175\ \mathrm{arcmin}^{2}$
with an average exposure time of $\sim 20\ \mathrm{hours}$
spread over $8-10$
filters. In both fields, we conduct extensive NIRSpec multi-object spectroscopy, including $2$
deep pointings of $\sim 55\ \mathrm{hours}$
exposure time, $14$
medium pointings of $\sim 12\ \mathrm{hours}$
, and $15$
shallower pointings of $\sim 4\ \mathrm{hours}$
, targeting over $5000$
HST and JWST-detected faint sources with $5$
low, medium, and high-resolution dispersers covering $0.6-5.3\ \mathrm{microns}$
. Finally, JADES extends redward via coordinated parallels with the JWST Mid-Infrared Instrument (MIRI), featuring $\sim 9\ \mathrm{arcmin}^{2}$
with $\sim 43\ \mathrm{hours}$
hours of exposure at $7.7\ \mathrm{microns}$
and twice that area with $2.0-6.5\ \mathrm{hours}$
hours of exposure at $12.8\ \mathrm{microns}$
. For nearly $30$
years, the GOODS-S and GOODS-N fields have been developed as the premier deep fields on the sky; JADES is now providing a compelling start on the JWST legacy in these fields.
Type
Publication
eprint arXiv:2306.02465
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