CEERS Epoch 1 NIRCam Imaging: Reduction Methods and Simulations Enabling Early JWST Science Results
We present the data release and data reduction process for the Epoch 1 NIRCam observations for the Cosmic Evolution Early Release Science Survey (CEERS). These data consist of NIRCam imaging in six broadband filters (F115W, F150W, F200W, F277W, F356W and F444W) and one medium-band filter (F410M) ove...
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2023 |
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In: The Astrophysical Journal Letters - IOP Publishing, 2022, 946(2023), 1, p L12 |
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volume:946 ; year:2023 ; number:1, p L12 |
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DOI / URN: |
10.3847/2041-8213/acbb08 |
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DOAJ089152891 |
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520 | |a We present the data release and data reduction process for the Epoch 1 NIRCam observations for the Cosmic Evolution Early Release Science Survey (CEERS). These data consist of NIRCam imaging in six broadband filters (F115W, F150W, F200W, F277W, F356W and F444W) and one medium-band filter (F410M) over four pointings, obtained in parallel with primary CEERS MIRI observations. We reduced the NIRCam imaging with the JWST Calibration Pipeline, with custom modifications and reduction steps designed to address additional features and challenges with the data. Here we provide a detailed description of each step in our reduction and a discussion of future expected improvements. Our reduction process includes corrections for known prelaunch issues such as 1/ f noise, as well as in-flight issues including snowballs, wisps, and astrometric alignment. Many of our custom reduction processes were first developed with prelaunch simulated NIRCam imaging over the full 10 CEERS NIRCam pointings. We present a description of the creation and reduction of this simulated data set in the Appendix. We provide mosaics of the real images in a public release, as well as our reduction scripts with detailed explanations to allow users to reproduce our final data products. These represent one of the first official public data sets released from the Directors Discretionary Early Release Science (DD-ERS) program. | ||
650 | 4 | |a Near infrared astronomy | |
650 | 4 | |a Direct imaging | |
650 | 4 | |a Astronomy data reduction | |
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700 | 0 | |a Steven L. Finkelstein |e verfasserin |4 aut | |
700 | 0 | |a Anton M. Koekemoer |e verfasserin |4 aut | |
700 | 0 | |a Henry C. Ferguson |e verfasserin |4 aut | |
700 | 0 | |a Pablo Arrabal Haro |e verfasserin |4 aut | |
700 | 0 | |a Mark Dickinson |e verfasserin |4 aut | |
700 | 0 | |a Jeyhan S. Kartaltepe |e verfasserin |4 aut | |
700 | 0 | |a Casey Papovich |e verfasserin |4 aut | |
700 | 0 | |a Pablo G. Pérez-González |e verfasserin |4 aut | |
700 | 0 | |a Nor Pirzkal |e verfasserin |4 aut | |
700 | 0 | |a Rachel S. Somerville |e verfasserin |4 aut | |
700 | 0 | |a Christopher N. A. Willmer |e verfasserin |4 aut | |
700 | 0 | |a Guang Yang |e verfasserin |4 aut | |
700 | 0 | |a L. Y. Aaron Yung |e verfasserin |4 aut | |
700 | 0 | |a Adriano Fontana |e verfasserin |4 aut | |
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700 | 0 | |a Norman A. Grogin |e verfasserin |4 aut | |
700 | 0 | |a Michaela Hirschmann |e verfasserin |4 aut | |
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700 | 0 | |a Stephen M. Wilkins |e verfasserin |4 aut | |
700 | 0 | |a Antonello Calabrò |e verfasserin |4 aut | |
700 | 0 | |a M. C. Cooper |e verfasserin |4 aut | |
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700 | 0 | |a Russell Ryan |e verfasserin |4 aut | |
700 | 0 | |a Xin Wang |e verfasserin |4 aut | |
700 | 0 | |a Stijn Wuyts |e verfasserin |4 aut | |
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10.3847/2041-8213/acbb08 doi (DE-627)DOAJ089152891 (DE-599)DOAJ643d267f26954c308d8f20b5a85b253c DE-627 ger DE-627 rakwb eng QB460-466 Micaela B. Bagley verfasserin aut CEERS Epoch 1 NIRCam Imaging: Reduction Methods and Simulations Enabling Early JWST Science Results 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present the data release and data reduction process for the Epoch 1 NIRCam observations for the Cosmic Evolution Early Release Science Survey (CEERS). These data consist of NIRCam imaging in six broadband filters (F115W, F150W, F200W, F277W, F356W and F444W) and one medium-band filter (F410M) over four pointings, obtained in parallel with primary CEERS MIRI observations. We reduced the NIRCam imaging with the JWST Calibration Pipeline, with custom modifications and reduction steps designed to address additional features and challenges with the data. Here we provide a detailed description of each step in our reduction and a discussion of future expected improvements. Our reduction process includes corrections for known prelaunch issues such as 1/ f noise, as well as in-flight issues including snowballs, wisps, and astrometric alignment. Many of our custom reduction processes were first developed with prelaunch simulated NIRCam imaging over the full 10 CEERS NIRCam pointings. We present a description of the creation and reduction of this simulated data set in the Appendix. We provide mosaics of the real images in a public release, as well as our reduction scripts with detailed explanations to allow users to reproduce our final data products. These represent one of the first official public data sets released from the Directors Discretionary Early Release Science (DD-ERS) program. Near infrared astronomy Direct imaging Astronomy data reduction Astrophysics Steven L. Finkelstein verfasserin aut Anton M. Koekemoer verfasserin aut Henry C. Ferguson verfasserin aut Pablo Arrabal Haro verfasserin aut Mark Dickinson verfasserin aut Jeyhan S. Kartaltepe verfasserin aut Casey Papovich verfasserin aut Pablo G. Pérez-González verfasserin aut Nor Pirzkal verfasserin aut Rachel S. Somerville verfasserin aut Christopher N. A. Willmer verfasserin aut Guang Yang verfasserin aut L. Y. Aaron Yung verfasserin aut Adriano Fontana verfasserin aut Andrea Grazian verfasserin aut Norman A. Grogin verfasserin aut Michaela Hirschmann verfasserin aut Lisa J. Kewley verfasserin aut Allison Kirkpatrick verfasserin aut Dale D. Kocevski verfasserin aut Jennifer M. Lotz verfasserin aut Aubrey Medrano verfasserin aut Alexa M. Morales verfasserin aut Laura Pentericci verfasserin aut Swara Ravindranath verfasserin aut Jonathan R. Trump verfasserin aut Stephen M. Wilkins verfasserin aut Antonello Calabrò verfasserin aut M. C. Cooper verfasserin aut Luca Costantin verfasserin aut Alexander de la Vega verfasserin aut Bryan Hilbert verfasserin aut Taylor A. Hutchison verfasserin aut Rebecca L. Larson verfasserin aut Ray A. Lucas verfasserin aut Elizabeth J. McGrath verfasserin aut Russell Ryan verfasserin aut Xin Wang verfasserin aut Stijn Wuyts verfasserin aut In The Astrophysical Journal Letters IOP Publishing, 2022 946(2023), 1, p L12 (DE-627)312189028 (DE-600)2006858-X 20418213 nnns volume:946 year:2023 number:1, p L12 https://doi.org/10.3847/2041-8213/acbb08 kostenfrei https://doaj.org/article/643d267f26954c308d8f20b5a85b253c kostenfrei https://doi.org/10.3847/2041-8213/acbb08 kostenfrei https://doaj.org/toc/2041-8205 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 946 2023 1, p L12 |
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10.3847/2041-8213/acbb08 doi (DE-627)DOAJ089152891 (DE-599)DOAJ643d267f26954c308d8f20b5a85b253c DE-627 ger DE-627 rakwb eng QB460-466 Micaela B. Bagley verfasserin aut CEERS Epoch 1 NIRCam Imaging: Reduction Methods and Simulations Enabling Early JWST Science Results 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present the data release and data reduction process for the Epoch 1 NIRCam observations for the Cosmic Evolution Early Release Science Survey (CEERS). These data consist of NIRCam imaging in six broadband filters (F115W, F150W, F200W, F277W, F356W and F444W) and one medium-band filter (F410M) over four pointings, obtained in parallel with primary CEERS MIRI observations. We reduced the NIRCam imaging with the JWST Calibration Pipeline, with custom modifications and reduction steps designed to address additional features and challenges with the data. Here we provide a detailed description of each step in our reduction and a discussion of future expected improvements. Our reduction process includes corrections for known prelaunch issues such as 1/ f noise, as well as in-flight issues including snowballs, wisps, and astrometric alignment. Many of our custom reduction processes were first developed with prelaunch simulated NIRCam imaging over the full 10 CEERS NIRCam pointings. We present a description of the creation and reduction of this simulated data set in the Appendix. We provide mosaics of the real images in a public release, as well as our reduction scripts with detailed explanations to allow users to reproduce our final data products. These represent one of the first official public data sets released from the Directors Discretionary Early Release Science (DD-ERS) program. Near infrared astronomy Direct imaging Astronomy data reduction Astrophysics Steven L. Finkelstein verfasserin aut Anton M. Koekemoer verfasserin aut Henry C. Ferguson verfasserin aut Pablo Arrabal Haro verfasserin aut Mark Dickinson verfasserin aut Jeyhan S. Kartaltepe verfasserin aut Casey Papovich verfasserin aut Pablo G. Pérez-González verfasserin aut Nor Pirzkal verfasserin aut Rachel S. Somerville verfasserin aut Christopher N. A. Willmer verfasserin aut Guang Yang verfasserin aut L. Y. Aaron Yung verfasserin aut Adriano Fontana verfasserin aut Andrea Grazian verfasserin aut Norman A. Grogin verfasserin aut Michaela Hirschmann verfasserin aut Lisa J. Kewley verfasserin aut Allison Kirkpatrick verfasserin aut Dale D. Kocevski verfasserin aut Jennifer M. Lotz verfasserin aut Aubrey Medrano verfasserin aut Alexa M. Morales verfasserin aut Laura Pentericci verfasserin aut Swara Ravindranath verfasserin aut Jonathan R. Trump verfasserin aut Stephen M. Wilkins verfasserin aut Antonello Calabrò verfasserin aut M. C. Cooper verfasserin aut Luca Costantin verfasserin aut Alexander de la Vega verfasserin aut Bryan Hilbert verfasserin aut Taylor A. Hutchison verfasserin aut Rebecca L. Larson verfasserin aut Ray A. Lucas verfasserin aut Elizabeth J. McGrath verfasserin aut Russell Ryan verfasserin aut Xin Wang verfasserin aut Stijn Wuyts verfasserin aut In The Astrophysical Journal Letters IOP Publishing, 2022 946(2023), 1, p L12 (DE-627)312189028 (DE-600)2006858-X 20418213 nnns volume:946 year:2023 number:1, p L12 https://doi.org/10.3847/2041-8213/acbb08 kostenfrei https://doaj.org/article/643d267f26954c308d8f20b5a85b253c kostenfrei https://doi.org/10.3847/2041-8213/acbb08 kostenfrei https://doaj.org/toc/2041-8205 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 946 2023 1, p L12 |
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10.3847/2041-8213/acbb08 doi (DE-627)DOAJ089152891 (DE-599)DOAJ643d267f26954c308d8f20b5a85b253c DE-627 ger DE-627 rakwb eng QB460-466 Micaela B. Bagley verfasserin aut CEERS Epoch 1 NIRCam Imaging: Reduction Methods and Simulations Enabling Early JWST Science Results 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present the data release and data reduction process for the Epoch 1 NIRCam observations for the Cosmic Evolution Early Release Science Survey (CEERS). These data consist of NIRCam imaging in six broadband filters (F115W, F150W, F200W, F277W, F356W and F444W) and one medium-band filter (F410M) over four pointings, obtained in parallel with primary CEERS MIRI observations. We reduced the NIRCam imaging with the JWST Calibration Pipeline, with custom modifications and reduction steps designed to address additional features and challenges with the data. Here we provide a detailed description of each step in our reduction and a discussion of future expected improvements. Our reduction process includes corrections for known prelaunch issues such as 1/ f noise, as well as in-flight issues including snowballs, wisps, and astrometric alignment. Many of our custom reduction processes were first developed with prelaunch simulated NIRCam imaging over the full 10 CEERS NIRCam pointings. We present a description of the creation and reduction of this simulated data set in the Appendix. We provide mosaics of the real images in a public release, as well as our reduction scripts with detailed explanations to allow users to reproduce our final data products. These represent one of the first official public data sets released from the Directors Discretionary Early Release Science (DD-ERS) program. Near infrared astronomy Direct imaging Astronomy data reduction Astrophysics Steven L. Finkelstein verfasserin aut Anton M. Koekemoer verfasserin aut Henry C. Ferguson verfasserin aut Pablo Arrabal Haro verfasserin aut Mark Dickinson verfasserin aut Jeyhan S. Kartaltepe verfasserin aut Casey Papovich verfasserin aut Pablo G. Pérez-González verfasserin aut Nor Pirzkal verfasserin aut Rachel S. Somerville verfasserin aut Christopher N. A. Willmer verfasserin aut Guang Yang verfasserin aut L. Y. Aaron Yung verfasserin aut Adriano Fontana verfasserin aut Andrea Grazian verfasserin aut Norman A. Grogin verfasserin aut Michaela Hirschmann verfasserin aut Lisa J. Kewley verfasserin aut Allison Kirkpatrick verfasserin aut Dale D. Kocevski verfasserin aut Jennifer M. Lotz verfasserin aut Aubrey Medrano verfasserin aut Alexa M. Morales verfasserin aut Laura Pentericci verfasserin aut Swara Ravindranath verfasserin aut Jonathan R. Trump verfasserin aut Stephen M. Wilkins verfasserin aut Antonello Calabrò verfasserin aut M. C. Cooper verfasserin aut Luca Costantin verfasserin aut Alexander de la Vega verfasserin aut Bryan Hilbert verfasserin aut Taylor A. Hutchison verfasserin aut Rebecca L. Larson verfasserin aut Ray A. Lucas verfasserin aut Elizabeth J. McGrath verfasserin aut Russell Ryan verfasserin aut Xin Wang verfasserin aut Stijn Wuyts verfasserin aut In The Astrophysical Journal Letters IOP Publishing, 2022 946(2023), 1, p L12 (DE-627)312189028 (DE-600)2006858-X 20418213 nnns volume:946 year:2023 number:1, p L12 https://doi.org/10.3847/2041-8213/acbb08 kostenfrei https://doaj.org/article/643d267f26954c308d8f20b5a85b253c kostenfrei https://doi.org/10.3847/2041-8213/acbb08 kostenfrei https://doaj.org/toc/2041-8205 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 946 2023 1, p L12 |
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10.3847/2041-8213/acbb08 doi (DE-627)DOAJ089152891 (DE-599)DOAJ643d267f26954c308d8f20b5a85b253c DE-627 ger DE-627 rakwb eng QB460-466 Micaela B. Bagley verfasserin aut CEERS Epoch 1 NIRCam Imaging: Reduction Methods and Simulations Enabling Early JWST Science Results 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present the data release and data reduction process for the Epoch 1 NIRCam observations for the Cosmic Evolution Early Release Science Survey (CEERS). These data consist of NIRCam imaging in six broadband filters (F115W, F150W, F200W, F277W, F356W and F444W) and one medium-band filter (F410M) over four pointings, obtained in parallel with primary CEERS MIRI observations. We reduced the NIRCam imaging with the JWST Calibration Pipeline, with custom modifications and reduction steps designed to address additional features and challenges with the data. Here we provide a detailed description of each step in our reduction and a discussion of future expected improvements. Our reduction process includes corrections for known prelaunch issues such as 1/ f noise, as well as in-flight issues including snowballs, wisps, and astrometric alignment. Many of our custom reduction processes were first developed with prelaunch simulated NIRCam imaging over the full 10 CEERS NIRCam pointings. We present a description of the creation and reduction of this simulated data set in the Appendix. We provide mosaics of the real images in a public release, as well as our reduction scripts with detailed explanations to allow users to reproduce our final data products. These represent one of the first official public data sets released from the Directors Discretionary Early Release Science (DD-ERS) program. Near infrared astronomy Direct imaging Astronomy data reduction Astrophysics Steven L. Finkelstein verfasserin aut Anton M. Koekemoer verfasserin aut Henry C. Ferguson verfasserin aut Pablo Arrabal Haro verfasserin aut Mark Dickinson verfasserin aut Jeyhan S. Kartaltepe verfasserin aut Casey Papovich verfasserin aut Pablo G. Pérez-González verfasserin aut Nor Pirzkal verfasserin aut Rachel S. Somerville verfasserin aut Christopher N. A. Willmer verfasserin aut Guang Yang verfasserin aut L. Y. Aaron Yung verfasserin aut Adriano Fontana verfasserin aut Andrea Grazian verfasserin aut Norman A. Grogin verfasserin aut Michaela Hirschmann verfasserin aut Lisa J. Kewley verfasserin aut Allison Kirkpatrick verfasserin aut Dale D. Kocevski verfasserin aut Jennifer M. Lotz verfasserin aut Aubrey Medrano verfasserin aut Alexa M. Morales verfasserin aut Laura Pentericci verfasserin aut Swara Ravindranath verfasserin aut Jonathan R. Trump verfasserin aut Stephen M. Wilkins verfasserin aut Antonello Calabrò verfasserin aut M. C. Cooper verfasserin aut Luca Costantin verfasserin aut Alexander de la Vega verfasserin aut Bryan Hilbert verfasserin aut Taylor A. Hutchison verfasserin aut Rebecca L. Larson verfasserin aut Ray A. Lucas verfasserin aut Elizabeth J. McGrath verfasserin aut Russell Ryan verfasserin aut Xin Wang verfasserin aut Stijn Wuyts verfasserin aut In The Astrophysical Journal Letters IOP Publishing, 2022 946(2023), 1, p L12 (DE-627)312189028 (DE-600)2006858-X 20418213 nnns volume:946 year:2023 number:1, p L12 https://doi.org/10.3847/2041-8213/acbb08 kostenfrei https://doaj.org/article/643d267f26954c308d8f20b5a85b253c kostenfrei https://doi.org/10.3847/2041-8213/acbb08 kostenfrei https://doaj.org/toc/2041-8205 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 946 2023 1, p L12 |
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Micaela B. Bagley @@aut@@ Steven L. Finkelstein @@aut@@ Anton M. Koekemoer @@aut@@ Henry C. Ferguson @@aut@@ Pablo Arrabal Haro @@aut@@ Mark Dickinson @@aut@@ Jeyhan S. Kartaltepe @@aut@@ Casey Papovich @@aut@@ Pablo G. Pérez-González @@aut@@ Nor Pirzkal @@aut@@ Rachel S. Somerville @@aut@@ Christopher N. A. Willmer @@aut@@ Guang Yang @@aut@@ L. Y. Aaron Yung @@aut@@ Adriano Fontana @@aut@@ Andrea Grazian @@aut@@ Norman A. Grogin @@aut@@ Michaela Hirschmann @@aut@@ Lisa J. Kewley @@aut@@ Allison Kirkpatrick @@aut@@ Dale D. Kocevski @@aut@@ Jennifer M. Lotz @@aut@@ Aubrey Medrano @@aut@@ Alexa M. Morales @@aut@@ Laura Pentericci @@aut@@ Swara Ravindranath @@aut@@ Jonathan R. Trump @@aut@@ Stephen M. Wilkins @@aut@@ Antonello Calabrò @@aut@@ M. C. Cooper @@aut@@ Luca Costantin @@aut@@ Alexander de la Vega @@aut@@ Bryan Hilbert @@aut@@ Taylor A. Hutchison @@aut@@ Rebecca L. Larson @@aut@@ Ray A. Lucas @@aut@@ Elizabeth J. McGrath @@aut@@ Russell Ryan @@aut@@ Xin Wang @@aut@@ Stijn Wuyts @@aut@@ |
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CEERS Epoch 1 NIRCam Imaging: Reduction Methods and Simulations Enabling Early JWST Science Results |
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We present the data release and data reduction process for the Epoch 1 NIRCam observations for the Cosmic Evolution Early Release Science Survey (CEERS). These data consist of NIRCam imaging in six broadband filters (F115W, F150W, F200W, F277W, F356W and F444W) and one medium-band filter (F410M) over four pointings, obtained in parallel with primary CEERS MIRI observations. We reduced the NIRCam imaging with the JWST Calibration Pipeline, with custom modifications and reduction steps designed to address additional features and challenges with the data. Here we provide a detailed description of each step in our reduction and a discussion of future expected improvements. Our reduction process includes corrections for known prelaunch issues such as 1/ f noise, as well as in-flight issues including snowballs, wisps, and astrometric alignment. Many of our custom reduction processes were first developed with prelaunch simulated NIRCam imaging over the full 10 CEERS NIRCam pointings. We present a description of the creation and reduction of this simulated data set in the Appendix. We provide mosaics of the real images in a public release, as well as our reduction scripts with detailed explanations to allow users to reproduce our final data products. These represent one of the first official public data sets released from the Directors Discretionary Early Release Science (DD-ERS) program. |
abstractGer |
We present the data release and data reduction process for the Epoch 1 NIRCam observations for the Cosmic Evolution Early Release Science Survey (CEERS). These data consist of NIRCam imaging in six broadband filters (F115W, F150W, F200W, F277W, F356W and F444W) and one medium-band filter (F410M) over four pointings, obtained in parallel with primary CEERS MIRI observations. We reduced the NIRCam imaging with the JWST Calibration Pipeline, with custom modifications and reduction steps designed to address additional features and challenges with the data. Here we provide a detailed description of each step in our reduction and a discussion of future expected improvements. Our reduction process includes corrections for known prelaunch issues such as 1/ f noise, as well as in-flight issues including snowballs, wisps, and astrometric alignment. Many of our custom reduction processes were first developed with prelaunch simulated NIRCam imaging over the full 10 CEERS NIRCam pointings. We present a description of the creation and reduction of this simulated data set in the Appendix. We provide mosaics of the real images in a public release, as well as our reduction scripts with detailed explanations to allow users to reproduce our final data products. These represent one of the first official public data sets released from the Directors Discretionary Early Release Science (DD-ERS) program. |
abstract_unstemmed |
We present the data release and data reduction process for the Epoch 1 NIRCam observations for the Cosmic Evolution Early Release Science Survey (CEERS). These data consist of NIRCam imaging in six broadband filters (F115W, F150W, F200W, F277W, F356W and F444W) and one medium-band filter (F410M) over four pointings, obtained in parallel with primary CEERS MIRI observations. We reduced the NIRCam imaging with the JWST Calibration Pipeline, with custom modifications and reduction steps designed to address additional features and challenges with the data. Here we provide a detailed description of each step in our reduction and a discussion of future expected improvements. Our reduction process includes corrections for known prelaunch issues such as 1/ f noise, as well as in-flight issues including snowballs, wisps, and astrometric alignment. Many of our custom reduction processes were first developed with prelaunch simulated NIRCam imaging over the full 10 CEERS NIRCam pointings. We present a description of the creation and reduction of this simulated data set in the Appendix. We provide mosaics of the real images in a public release, as well as our reduction scripts with detailed explanations to allow users to reproduce our final data products. These represent one of the first official public data sets released from the Directors Discretionary Early Release Science (DD-ERS) program. |
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