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| Format: | Preprint |
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2023
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| Online Access: | https://arxiv.org/abs/2306.02465 |
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| _version_ | 1866911323394146304 |
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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 |