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Main Authors: Eisenstein, Daniel J., Willott, Chris, Alberts, Stacey, Arribas, Santiago, Bonaventura, Nina, Bunker, Andrew J., Cameron, Alex J., Carniani, Stefano, Charlot, Stephane, Curtis-Lake, Emma, D'Eugenio, Francesco, Ferruit, Pierre, Giardino, Giovanna, Hainline, Kevin, Hausen, Ryan, Jakobsen, Peter, Johnson, Benjamin D., Maiolino, Roberto, Rauscher, Bernard J., Rieke, Marcia, Rieke, George, Rix, Hans-Walter, Robertson, Brant, Stark, Daniel P., Tacchella, Sandro, Williams, Christina C., Willmer, Christopher N. A., Baker, William M., Baum, Stefi, Bhatawdekar, Rachana, Boyett, Kristan, Chen, Zuyi, Chevallard, Jacopo, Circosta, Chiara, Curti, Mirko, Danhaive, A. Lola, DeCoursey, Christa, Endsley, Ryan, de Graaff, Anna, Dressler, Alan, Egami, Eiichi, Helton, Jakob M., Hviding, Raphael E., Ji, Zhiyuan, Jones, Gareth C., Kumari, Nimisha, Lützgendorf, Nora, Laseter, Isaac, Looser, Tobias J., Lyu, Jianwei, Maseda, Michael V., Nelson, Erica, Parlanti, Eleonora, Perna, Michele, Puskás, Dávid, Rawle, Tim, Del Pino, Bruno Rodríguez, Rujopakarn, Wiphu, Sandles, Lester, Saxena, Aayush, Scholtz, Jan, Sharpe, Katherine, Shivaei, Irene, Silcock, Maddie S., Simmonds, Charlotte, Skarbinski, Maya, Smit, Renske, Stone, Meredith, Suess, Katherine A., Sun, Fengwu, Tang, Mengtao, Topping, Michael W., Übler, Hannah, Villanueva, Natalia C., Wallace, Imaan E. B., Whitler, Lily, Witstok, Joris, Woodrum, Charity
Format: Preprint
Published: 2023
Subjects:
Online Access:https://arxiv.org/abs/2306.02465
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author Eisenstein, Daniel J.
Willott, Chris
Alberts, Stacey
Arribas, Santiago
Bonaventura, Nina
Bunker, Andrew J.
Cameron, Alex J.
Carniani, Stefano
Charlot, Stephane
Curtis-Lake, Emma
D'Eugenio, Francesco
Ferruit, Pierre
Giardino, Giovanna
Hainline, Kevin
Hausen, Ryan
Jakobsen, Peter
Johnson, Benjamin D.
Maiolino, Roberto
Rauscher, Bernard J.
Rieke, Marcia
Rieke, George
Rix, Hans-Walter
Robertson, Brant
Stark, Daniel P.
Tacchella, Sandro
Williams, Christina C.
Willmer, Christopher N. A.
Baker, William M.
Baum, Stefi
Bhatawdekar, Rachana
Boyett, Kristan
Chen, Zuyi
Chevallard, Jacopo
Circosta, Chiara
Curti, Mirko
Danhaive, A. Lola
DeCoursey, Christa
Endsley, Ryan
de Graaff, Anna
Dressler, Alan
Egami, Eiichi
Helton, Jakob M.
Hviding, Raphael E.
Ji, Zhiyuan
Jones, Gareth C.
Kumari, Nimisha
Lützgendorf, Nora
Laseter, Isaac
Looser, Tobias J.
Lyu, Jianwei
Maseda, Michael V.
Nelson, Erica
Parlanti, Eleonora
Perna, Michele
Puskás, Dávid
Rawle, Tim
Del Pino, Bruno Rodríguez
Rujopakarn, Wiphu
Sandles, Lester
Saxena, Aayush
Scholtz, Jan
Sharpe, Katherine
Shivaei, Irene
Silcock, Maddie S.
Simmonds, Charlotte
Skarbinski, Maya
Smit, Renske
Stone, Meredith
Suess, Katherine A.
Sun, Fengwu
Tang, Mengtao
Topping, Michael W.
Übler, Hannah
Villanueva, Natalia C.
Wallace, Imaan E. B.
Whitler, Lily
Witstok, Joris
Woodrum, Charity
author_facet Eisenstein, Daniel J.
Willott, Chris
Alberts, Stacey
Arribas, Santiago
Bonaventura, Nina
Bunker, Andrew J.
Cameron, Alex J.
Carniani, Stefano
Charlot, Stephane
Curtis-Lake, Emma
D'Eugenio, Francesco
Ferruit, Pierre
Giardino, Giovanna
Hainline, Kevin
Hausen, Ryan
Jakobsen, Peter
Johnson, Benjamin D.
Maiolino, Roberto
Rauscher, Bernard J.
Rieke, Marcia
Rieke, George
Rix, Hans-Walter
Robertson, Brant
Stark, Daniel P.
Tacchella, Sandro
Williams, Christina C.
Willmer, Christopher N. A.
Baker, William M.
Baum, Stefi
Bhatawdekar, Rachana
Boyett, Kristan
Chen, Zuyi
Chevallard, Jacopo
Circosta, Chiara
Curti, Mirko
Danhaive, A. Lola
DeCoursey, Christa
Endsley, Ryan
de Graaff, Anna
Dressler, Alan
Egami, Eiichi
Helton, Jakob M.
Hviding, Raphael E.
Ji, Zhiyuan
Jones, Gareth C.
Kumari, Nimisha
Lützgendorf, Nora
Laseter, Isaac
Looser, Tobias J.
Lyu, Jianwei
Maseda, Michael V.
Nelson, Erica
Parlanti, Eleonora
Perna, Michele
Puskás, Dávid
Rawle, Tim
Del Pino, Bruno Rodríguez
Rujopakarn, Wiphu
Sandles, Lester
Saxena, Aayush
Scholtz, Jan
Sharpe, Katherine
Shivaei, Irene
Silcock, Maddie S.
Simmonds, Charlotte
Skarbinski, Maya
Smit, Renske
Stone, Meredith
Suess, Katherine A.
Sun, Fengwu
Tang, Mengtao
Topping, Michael W.
Übler, Hannah
Villanueva, Natalia C.
Wallace, Imaan E. B.
Whitler, Lily
Witstok, Joris
Woodrum, Charity
contents 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 ~42 arcmin^2 with over 100 hrs of exposure time spread over 9 NIRCam filters, including two medium-band filters. This is extended at medium depth in GOODS-S and GOODS-N with NIRCam imaging of ~167 arcmin^2, averaging 25 hrs of exposure over 8-10 filters. In both fields, we conduct extensive NIRSpec multi-object spectroscopy, including 2 deep pointings of 55 hrs exposure time, 14 medium pointings of ~12 hrs, and 15 shallower pointings of ~4 hrs, targeting over 5000 HST and JWST-detected faint sources with 5 low, medium, and high-resolution dispersers covering 0.6-5.3 um. Finally, JADES extends redward via coordinated parallels with the JWST Mid-Infrared Instrument (MIRI), featuring ~10 arcmin^2 with 43 hours of exposure at 7.7 um and thrice that area with 1.4-6.8 hours of exposure at 12.8 um and 15 um. 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.
format Preprint
id arxiv_https___arxiv_org_abs_2306_02465
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Overview of the JWST Advanced Deep Extragalactic Survey (JADES)
Eisenstein, Daniel J.
Willott, Chris
Alberts, Stacey
Arribas, Santiago
Bonaventura, Nina
Bunker, Andrew J.
Cameron, Alex J.
Carniani, Stefano
Charlot, Stephane
Curtis-Lake, Emma
D'Eugenio, Francesco
Ferruit, Pierre
Giardino, Giovanna
Hainline, Kevin
Hausen, Ryan
Jakobsen, Peter
Johnson, Benjamin D.
Maiolino, Roberto
Rauscher, Bernard J.
Rieke, Marcia
Rieke, George
Rix, Hans-Walter
Robertson, Brant
Stark, Daniel P.
Tacchella, Sandro
Williams, Christina C.
Willmer, Christopher N. A.
Baker, William M.
Baum, Stefi
Bhatawdekar, Rachana
Boyett, Kristan
Chen, Zuyi
Chevallard, Jacopo
Circosta, Chiara
Curti, Mirko
Danhaive, A. Lola
DeCoursey, Christa
Endsley, Ryan
de Graaff, Anna
Dressler, Alan
Egami, Eiichi
Helton, Jakob M.
Hviding, Raphael E.
Ji, Zhiyuan
Jones, Gareth C.
Kumari, Nimisha
Lützgendorf, Nora
Laseter, Isaac
Looser, Tobias J.
Lyu, Jianwei
Maseda, Michael V.
Nelson, Erica
Parlanti, Eleonora
Perna, Michele
Puskás, Dávid
Rawle, Tim
Del Pino, Bruno Rodríguez
Rujopakarn, Wiphu
Sandles, Lester
Saxena, Aayush
Scholtz, Jan
Sharpe, Katherine
Shivaei, Irene
Silcock, Maddie S.
Simmonds, Charlotte
Skarbinski, Maya
Smit, Renske
Stone, Meredith
Suess, Katherine A.
Sun, Fengwu
Tang, Mengtao
Topping, Michael W.
Übler, Hannah
Villanueva, Natalia C.
Wallace, Imaan E. B.
Whitler, Lily
Witstok, Joris
Woodrum, Charity
Astrophysics of Galaxies
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 ~42 arcmin^2 with over 100 hrs of exposure time spread over 9 NIRCam filters, including two medium-band filters. This is extended at medium depth in GOODS-S and GOODS-N with NIRCam imaging of ~167 arcmin^2, averaging 25 hrs of exposure over 8-10 filters. In both fields, we conduct extensive NIRSpec multi-object spectroscopy, including 2 deep pointings of 55 hrs exposure time, 14 medium pointings of ~12 hrs, and 15 shallower pointings of ~4 hrs, targeting over 5000 HST and JWST-detected faint sources with 5 low, medium, and high-resolution dispersers covering 0.6-5.3 um. Finally, JADES extends redward via coordinated parallels with the JWST Mid-Infrared Instrument (MIRI), featuring ~10 arcmin^2 with 43 hours of exposure at 7.7 um and thrice that area with 1.4-6.8 hours of exposure at 12.8 um and 15 um. 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.
title Overview of the JWST Advanced Deep Extragalactic Survey (JADES)
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2306.02465