The JADES Origins Field: A New JWST Deep Field in the JADES Second NIRCam Data Release

We summarize the properties and initial data release of the JADES Origins Field (JOF), which will soon be the deepest imaging field yet observed with the James Webb Space Telescope (JWST). This field falls within the GOODS-S region about 8' south-west of the Hubble Ultra Deep Field (HUDF), wher...

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Veröffentlicht in:arXiv.org 2023-10
Hauptverfasser: Eisenstein, Daniel J, Johnson, Benjamin D, Robertson, Brant, Tacchella, Sandro, Hainline, Kevin, Jakobsen, Peter, Maiolino, Roberto, Bonaventura, Nina, Bunker, Andrew J, Cameron, Alex J, Cargile, Phillip A, Curtis-Lake, Emma, Hausen, Ryan, Puskás, Dávid, Rieke, Marcia, Sun, Fengwu, Willmer, Christopher N A, Willott, Chris, Alberts, Stacey, Arribas, Santiago, Baker, William M, Baum, Stefi, Bhatawdekar, Rachana, Carniani, Stefano, Charlot, Stephane, Chen, Zuyi, Chevallard, Jacopo, Curti, Mirko, DeCoursey, Christa, D'Eugenio, Francesco, de Graaff, Anna, Egami, Eiichi, Helton, Jakob M, Ji, Zhiyuan, Jones, Gareth C, Kumari, Nimisha, Lützgendorf, Nora, Laseter, Isaac, Looser, Tobias J, Lyu, Jianwei, Maseda, Michael V, Nelson, Erica, Parlanti, Eleonora, Rauscher, Bernard J, Rawle, Tim, Rieke, George, Hans-Walter Rix, Rujopakarn, Wiphu, Sandles, Lester, Saxena, Aayush, Scholtz, Jan, Sharpe, Katherine, Shivaei, Irene, Simmonds, Charlotte, Smit, Renske, Topping, Michael W, Übler, Hannah, Venturi, Giacomo, Williams, Christina C, Witstok, Joris, Woodrum, Charity
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creator Eisenstein, Daniel J
Johnson, Benjamin D
Robertson, Brant
Tacchella, Sandro
Hainline, Kevin
Jakobsen, Peter
Maiolino, Roberto
Bonaventura, Nina
Bunker, Andrew J
Cameron, Alex J
Cargile, Phillip A
Curtis-Lake, Emma
Hausen, Ryan
Puskás, Dávid
Rieke, Marcia
Sun, Fengwu
Willmer, Christopher N A
Willott, Chris
Alberts, Stacey
Arribas, Santiago
Baker, William M
Baum, Stefi
Bhatawdekar, Rachana
Carniani, Stefano
Charlot, Stephane
Chen, Zuyi
Chevallard, Jacopo
Curti, Mirko
DeCoursey, Christa
D'Eugenio, Francesco
de Graaff, Anna
Egami, Eiichi
Helton, Jakob M
Ji, Zhiyuan
Jones, Gareth C
Kumari, Nimisha
Lützgendorf, Nora
Laseter, Isaac
Looser, Tobias J
Lyu, Jianwei
Maseda, Michael V
Nelson, Erica
Parlanti, Eleonora
Rauscher, Bernard J
Rawle, Tim
Rieke, George
Hans-Walter Rix
Rujopakarn, Wiphu
Sandles, Lester
Saxena, Aayush
Scholtz, Jan
Sharpe, Katherine
Shivaei, Irene
Simmonds, Charlotte
Smit, Renske
Topping, Michael W
Übler, Hannah
Venturi, Giacomo
Williams, Christina C
Witstok, Joris
Woodrum, Charity
description We summarize the properties and initial data release of the JADES Origins Field (JOF), which will soon be the deepest imaging field yet observed with the James Webb Space Telescope (JWST). This field falls within the GOODS-S region about 8' south-west of the Hubble Ultra Deep Field (HUDF), where it was formed initially in Cycle 1 as a parallel field of HUDF spectroscopic observations within the JWST Advanced Deep Extragalactic Survey (JADES). This imaging will be greatly extended in Cycle 2 program 3215, which will observe the JOF for 5 days in six medium-band filters, seeking robust candidates for z>15 galaxies. This program will also include ultra-deep parallel NIRSpec spectroscopy (up to 104 hours on-source, summing over the dispersion modes) on the HUDF. Cycle 3 observations from program 4540 will add 20 hours of NIRCam slitless spectroscopy to the JOF. With these three campaigns, the JOF will be observed for 380 open-shutter hours with NIRCam using 15 imaging filters and 2 grism bandpasses. Further, parts of the JOF have deep 43 hr MIRI observations in F770W. Taken together, the JOF will soon be one of the most compelling deep fields available with JWST and a powerful window into the early Universe. This paper presents the second data release from JADES, featuring the imaging and catalogs from the year 1 JOF observations.
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Johnson, Benjamin D ; Robertson, Brant ; Tacchella, Sandro ; Hainline, Kevin ; Jakobsen, Peter ; Maiolino, Roberto ; Bonaventura, Nina ; Bunker, Andrew J ; Cameron, Alex J ; Cargile, Phillip A ; Curtis-Lake, Emma ; Hausen, Ryan ; Puskás, Dávid ; Rieke, Marcia ; Sun, Fengwu ; Willmer, Christopher N A ; Willott, Chris ; Alberts, Stacey ; Arribas, Santiago ; Baker, William M ; Baum, Stefi ; Bhatawdekar, Rachana ; Carniani, Stefano ; Charlot, Stephane ; Chen, Zuyi ; Chevallard, Jacopo ; Curti, Mirko ; DeCoursey, Christa ; D'Eugenio, Francesco ; de Graaff, Anna ; Egami, Eiichi ; Helton, Jakob M ; Ji, Zhiyuan ; Jones, Gareth C ; Kumari, Nimisha ; Lützgendorf, Nora ; Laseter, Isaac ; Looser, Tobias J ; Lyu, Jianwei ; Maseda, Michael V ; Nelson, Erica ; Parlanti, Eleonora ; Rauscher, Bernard J ; Rawle, Tim ; Rieke, George ; Hans-Walter Rix ; Rujopakarn, Wiphu ; Sandles, Lester ; Saxena, Aayush ; Scholtz, Jan ; Sharpe, Katherine ; Shivaei, Irene ; Simmonds, Charlotte ; Smit, Renske ; Topping, Michael W ; Übler, Hannah ; Venturi, Giacomo ; Williams, Christina C ; Witstok, Joris ; Woodrum, Charity</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-proquest_journals_28794415823</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2023</creationdate><topic>Galaxies</topic><topic>Hubble deep field</topic><topic>Hubble Space Telescope</topic><topic>Imaging</topic><topic>James Webb Space Telescope</topic><topic>Origins</topic><topic>Space telescopes</topic><topic>Spectroscopy</topic><topic>Spectrum analysis</topic><toplevel>online_resources</toplevel><creatorcontrib>Eisenstein, Daniel J</creatorcontrib><creatorcontrib>Johnson, Benjamin D</creatorcontrib><creatorcontrib>Robertson, Brant</creatorcontrib><creatorcontrib>Tacchella, Sandro</creatorcontrib><creatorcontrib>Hainline, Kevin</creatorcontrib><creatorcontrib>Jakobsen, Peter</creatorcontrib><creatorcontrib>Maiolino, Roberto</creatorcontrib><creatorcontrib>Bonaventura, Nina</creatorcontrib><creatorcontrib>Bunker, Andrew J</creatorcontrib><creatorcontrib>Cameron, Alex J</creatorcontrib><creatorcontrib>Cargile, Phillip A</creatorcontrib><creatorcontrib>Curtis-Lake, Emma</creatorcontrib><creatorcontrib>Hausen, Ryan</creatorcontrib><creatorcontrib>Puskás, Dávid</creatorcontrib><creatorcontrib>Rieke, Marcia</creatorcontrib><creatorcontrib>Sun, Fengwu</creatorcontrib><creatorcontrib>Willmer, Christopher N A</creatorcontrib><creatorcontrib>Willott, Chris</creatorcontrib><creatorcontrib>Alberts, Stacey</creatorcontrib><creatorcontrib>Arribas, Santiago</creatorcontrib><creatorcontrib>Baker, William M</creatorcontrib><creatorcontrib>Baum, Stefi</creatorcontrib><creatorcontrib>Bhatawdekar, Rachana</creatorcontrib><creatorcontrib>Carniani, Stefano</creatorcontrib><creatorcontrib>Charlot, Stephane</creatorcontrib><creatorcontrib>Chen, Zuyi</creatorcontrib><creatorcontrib>Chevallard, Jacopo</creatorcontrib><creatorcontrib>Curti, Mirko</creatorcontrib><creatorcontrib>DeCoursey, Christa</creatorcontrib><creatorcontrib>D'Eugenio, Francesco</creatorcontrib><creatorcontrib>de Graaff, Anna</creatorcontrib><creatorcontrib>Egami, Eiichi</creatorcontrib><creatorcontrib>Helton, Jakob M</creatorcontrib><creatorcontrib>Ji, Zhiyuan</creatorcontrib><creatorcontrib>Jones, Gareth C</creatorcontrib><creatorcontrib>Kumari, Nimisha</creatorcontrib><creatorcontrib>Lützgendorf, Nora</creatorcontrib><creatorcontrib>Laseter, Isaac</creatorcontrib><creatorcontrib>Looser, Tobias J</creatorcontrib><creatorcontrib>Lyu, Jianwei</creatorcontrib><creatorcontrib>Maseda, Michael V</creatorcontrib><creatorcontrib>Nelson, Erica</creatorcontrib><creatorcontrib>Parlanti, Eleonora</creatorcontrib><creatorcontrib>Rauscher, Bernard J</creatorcontrib><creatorcontrib>Rawle, Tim</creatorcontrib><creatorcontrib>Rieke, George</creatorcontrib><creatorcontrib>Hans-Walter Rix</creatorcontrib><creatorcontrib>Rujopakarn, Wiphu</creatorcontrib><creatorcontrib>Sandles, Lester</creatorcontrib><creatorcontrib>Saxena, Aayush</creatorcontrib><creatorcontrib>Scholtz, Jan</creatorcontrib><creatorcontrib>Sharpe, Katherine</creatorcontrib><creatorcontrib>Shivaei, Irene</creatorcontrib><creatorcontrib>Simmonds, Charlotte</creatorcontrib><creatorcontrib>Smit, Renske</creatorcontrib><creatorcontrib>Topping, Michael W</creatorcontrib><creatorcontrib>Übler, Hannah</creatorcontrib><creatorcontrib>Venturi, Giacomo</creatorcontrib><creatorcontrib>Williams, Christina C</creatorcontrib><creatorcontrib>Witstok, Joris</creatorcontrib><creatorcontrib>Woodrum, Charity</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science &amp; Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering Collection</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Eisenstein, Daniel J</au><au>Johnson, Benjamin D</au><au>Robertson, Brant</au><au>Tacchella, Sandro</au><au>Hainline, Kevin</au><au>Jakobsen, Peter</au><au>Maiolino, Roberto</au><au>Bonaventura, Nina</au><au>Bunker, Andrew J</au><au>Cameron, Alex J</au><au>Cargile, Phillip A</au><au>Curtis-Lake, Emma</au><au>Hausen, Ryan</au><au>Puskás, Dávid</au><au>Rieke, Marcia</au><au>Sun, Fengwu</au><au>Willmer, Christopher N A</au><au>Willott, Chris</au><au>Alberts, Stacey</au><au>Arribas, Santiago</au><au>Baker, William M</au><au>Baum, Stefi</au><au>Bhatawdekar, Rachana</au><au>Carniani, Stefano</au><au>Charlot, Stephane</au><au>Chen, Zuyi</au><au>Chevallard, Jacopo</au><au>Curti, Mirko</au><au>DeCoursey, Christa</au><au>D'Eugenio, Francesco</au><au>de Graaff, Anna</au><au>Egami, Eiichi</au><au>Helton, Jakob M</au><au>Ji, Zhiyuan</au><au>Jones, Gareth C</au><au>Kumari, Nimisha</au><au>Lützgendorf, Nora</au><au>Laseter, Isaac</au><au>Looser, Tobias J</au><au>Lyu, Jianwei</au><au>Maseda, Michael V</au><au>Nelson, Erica</au><au>Parlanti, Eleonora</au><au>Rauscher, Bernard J</au><au>Rawle, Tim</au><au>Rieke, George</au><au>Hans-Walter Rix</au><au>Rujopakarn, Wiphu</au><au>Sandles, Lester</au><au>Saxena, Aayush</au><au>Scholtz, Jan</au><au>Sharpe, Katherine</au><au>Shivaei, Irene</au><au>Simmonds, Charlotte</au><au>Smit, Renske</au><au>Topping, Michael W</au><au>Übler, Hannah</au><au>Venturi, Giacomo</au><au>Williams, Christina C</au><au>Witstok, Joris</au><au>Woodrum, Charity</au><format>book</format><genre>document</genre><ristype>GEN</ristype><atitle>The JADES Origins Field: A New JWST Deep Field in the JADES Second NIRCam Data Release</atitle><jtitle>arXiv.org</jtitle><date>2023-10-18</date><risdate>2023</risdate><eissn>2331-8422</eissn><abstract>We summarize the properties and initial data release of the JADES Origins Field (JOF), which will soon be the deepest imaging field yet observed with the James Webb Space Telescope (JWST). This field falls within the GOODS-S region about 8' south-west of the Hubble Ultra Deep Field (HUDF), where it was formed initially in Cycle 1 as a parallel field of HUDF spectroscopic observations within the JWST Advanced Deep Extragalactic Survey (JADES). This imaging will be greatly extended in Cycle 2 program 3215, which will observe the JOF for 5 days in six medium-band filters, seeking robust candidates for z&gt;15 galaxies. This program will also include ultra-deep parallel NIRSpec spectroscopy (up to 104 hours on-source, summing over the dispersion modes) on the HUDF. Cycle 3 observations from program 4540 will add 20 hours of NIRCam slitless spectroscopy to the JOF. With these three campaigns, the JOF will be observed for 380 open-shutter hours with NIRCam using 15 imaging filters and 2 grism bandpasses. Further, parts of the JOF have deep 43 hr MIRI observations in F770W. Taken together, the JOF will soon be one of the most compelling deep fields available with JWST and a powerful window into the early Universe. This paper presents the second data release from JADES, featuring the imaging and catalogs from the year 1 JOF observations.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><oa>free_for_read</oa></addata></record>
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subjects Galaxies
Hubble deep field
Hubble Space Telescope
Imaging
James Webb Space Telescope
Origins
Space telescopes
Spectroscopy
Spectrum analysis
title The JADES Origins Field: A New JWST Deep Field in the JADES Second NIRCam Data Release
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