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PHANGS-JWST: Data Processing Pipeline and First Full Public Data Release

Fuente: arXiv

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Bibliographic Details
Main Authors:	Williams, Thomas G., Lee, Janice C., Larson, Kirsten L., Leroy, Adam K., Sandstrom, Karin, Schinnerer, Eva, Thilker, David A., Belfiore, Francesco, Egorov, Oleg V., Rosolowsky, Erik, Sutter, Jessica, DePasquale, Joseph, Pagan, Alyssa, Berger, Travis A., Anand, Gagandeep S., Barnes, Ashley T., Bigiel, Frank, Boquien, Médéric, Cao, Yixian, Chastenet, Jérémy, Chevance, Mélanie, Chown, Ryan, Dale, Daniel A., Deger, Sinan, Eibensteiner, Cosima, Emsellem, Eric, Faesi, Christopher M., Glover, Simon C. O., Grasha, Kathryn, Hannon, Stephen, Hassani, Hamid, Henshaw, Jonathan D., Jiménez-Donaire, María J., Kim, Jaeyeon, Klessen, Ralf S., Koch, Eric W., Li, Jing, Liu, Daizhong, Meidt, Sharon E., Méndez-Delgado, J. Eduardo, Murphy, Eric J., Neumann, Justus, Neumann, Lukas, Neumayer, Nadine, Oakes, Elias K., Pathak, Debosmita, Pety, Jérôme, Pinna, Francesca, Querejeta, Miguel, Ramambason, Lise, Romanelli, Andrea, Sormani, Mattia C., Stuber, Sophia K., Sun, Jiayi, Teng, Yu-Hsuan, Usero, Antonio, Watkins, Elizabeth J., Weinbeck, Tony D.
Format:	Preprint
Published:	2024
Subjects:	Astrophysics of Galaxies
Online Access:	Acceder al recurso
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_version_	1866929338078724096
author	Williams, Thomas G. Lee, Janice C. Larson, Kirsten L. Leroy, Adam K. Sandstrom, Karin Schinnerer, Eva Thilker, David A. Belfiore, Francesco Egorov, Oleg V. Rosolowsky, Erik Sutter, Jessica DePasquale, Joseph Pagan, Alyssa Berger, Travis A. Anand, Gagandeep S. Barnes, Ashley T. Bigiel, Frank Boquien, Médéric Cao, Yixian Chastenet, Jérémy Chevance, Mélanie Chown, Ryan Dale, Daniel A. Deger, Sinan Eibensteiner, Cosima Emsellem, Eric Faesi, Christopher M. Glover, Simon C. O. Grasha, Kathryn Hannon, Stephen Hassani, Hamid Henshaw, Jonathan D. Jiménez-Donaire, María J. Kim, Jaeyeon Klessen, Ralf S. Koch, Eric W. Li, Jing Liu, Daizhong Meidt, Sharon E. Méndez-Delgado, J. Eduardo Murphy, Eric J. Neumann, Justus Neumann, Lukas Neumayer, Nadine Oakes, Elias K. Pathak, Debosmita Pety, Jérôme Pinna, Francesca Querejeta, Miguel Ramambason, Lise Romanelli, Andrea Sormani, Mattia C. Stuber, Sophia K. Sun, Jiayi Teng, Yu-Hsuan Usero, Antonio Watkins, Elizabeth J. Weinbeck, Tony D.
author_facet	Williams, Thomas G. Lee, Janice C. Larson, Kirsten L. Leroy, Adam K. Sandstrom, Karin Schinnerer, Eva Thilker, David A. Belfiore, Francesco Egorov, Oleg V. Rosolowsky, Erik Sutter, Jessica DePasquale, Joseph Pagan, Alyssa Berger, Travis A. Anand, Gagandeep S. Barnes, Ashley T. Bigiel, Frank Boquien, Médéric Cao, Yixian Chastenet, Jérémy Chevance, Mélanie Chown, Ryan Dale, Daniel A. Deger, Sinan Eibensteiner, Cosima Emsellem, Eric Faesi, Christopher M. Glover, Simon C. O. Grasha, Kathryn Hannon, Stephen Hassani, Hamid Henshaw, Jonathan D. Jiménez-Donaire, María J. Kim, Jaeyeon Klessen, Ralf S. Koch, Eric W. Li, Jing Liu, Daizhong Meidt, Sharon E. Méndez-Delgado, J. Eduardo Murphy, Eric J. Neumann, Justus Neumann, Lukas Neumayer, Nadine Oakes, Elias K. Pathak, Debosmita Pety, Jérôme Pinna, Francesca Querejeta, Miguel Ramambason, Lise Romanelli, Andrea Sormani, Mattia C. Stuber, Sophia K. Sun, Jiayi Teng, Yu-Hsuan Usero, Antonio Watkins, Elizabeth J. Weinbeck, Tony D.
contents	The exquisite angular resolution and sensitivity of JWST is opening a new window for our understanding of the Universe. In nearby galaxies, JWST observations are revolutionizing our understanding of the first phases of star formation and the dusty interstellar medium. Nineteen local galaxies spanning a range of properties and morphologies across the star-forming main sequence have been observed as part of the PHANGS-JWST Cycle 1 Treasury program at spatial scales of $\sim$5-50pc. Here, we describe pjpipe, an image processing pipeline developed for the PHANGS-JWST program that wraps around and extends the official JWST pipeline. We release this pipeline to the community as it contains a number of tools generally useful for JWST NIRCam and MIRI observations. Particularly for extended sources, pjpipe products provide significant improvements over mosaics from the MAST archive in terms of removing instrumental noise in NIRCam data, background flux matching, and calibration of relative and absolute astrometry. We show that slightly smoothing F2100W MIRI data to 0.9" (degrading the resolution by about 30 percent) reduces the noise by a factor of $\approx$3. We also present the first public release (DR1.1.0) of the pjpipe processed eight-band 2-21 $μ$m imaging for all nineteen galaxies in the PHANGS-JWST Cycle 1 Treasury program. An additional 55 galaxies will soon follow from a new PHANGS-JWST Cycle 2 Treasury program.
format	Preprint
id	arxiv_https___arxiv_org_abs_2401_15142
institution	arXiv
publishDate	2024
record_format	arxiv
spellingShingle	PHANGS-JWST: Data Processing Pipeline and First Full Public Data Release Williams, Thomas G. Lee, Janice C. Larson, Kirsten L. Leroy, Adam K. Sandstrom, Karin Schinnerer, Eva Thilker, David A. Belfiore, Francesco Egorov, Oleg V. Rosolowsky, Erik Sutter, Jessica DePasquale, Joseph Pagan, Alyssa Berger, Travis A. Anand, Gagandeep S. Barnes, Ashley T. Bigiel, Frank Boquien, Médéric Cao, Yixian Chastenet, Jérémy Chevance, Mélanie Chown, Ryan Dale, Daniel A. Deger, Sinan Eibensteiner, Cosima Emsellem, Eric Faesi, Christopher M. Glover, Simon C. O. Grasha, Kathryn Hannon, Stephen Hassani, Hamid Henshaw, Jonathan D. Jiménez-Donaire, María J. Kim, Jaeyeon Klessen, Ralf S. Koch, Eric W. Li, Jing Liu, Daizhong Meidt, Sharon E. Méndez-Delgado, J. Eduardo Murphy, Eric J. Neumann, Justus Neumann, Lukas Neumayer, Nadine Oakes, Elias K. Pathak, Debosmita Pety, Jérôme Pinna, Francesca Querejeta, Miguel Ramambason, Lise Romanelli, Andrea Sormani, Mattia C. Stuber, Sophia K. Sun, Jiayi Teng, Yu-Hsuan Usero, Antonio Watkins, Elizabeth J. Weinbeck, Tony D. Astrophysics of Galaxies The exquisite angular resolution and sensitivity of JWST is opening a new window for our understanding of the Universe. In nearby galaxies, JWST observations are revolutionizing our understanding of the first phases of star formation and the dusty interstellar medium. Nineteen local galaxies spanning a range of properties and morphologies across the star-forming main sequence have been observed as part of the PHANGS-JWST Cycle 1 Treasury program at spatial scales of $\sim$5-50pc. Here, we describe pjpipe, an image processing pipeline developed for the PHANGS-JWST program that wraps around and extends the official JWST pipeline. We release this pipeline to the community as it contains a number of tools generally useful for JWST NIRCam and MIRI observations. Particularly for extended sources, pjpipe products provide significant improvements over mosaics from the MAST archive in terms of removing instrumental noise in NIRCam data, background flux matching, and calibration of relative and absolute astrometry. We show that slightly smoothing F2100W MIRI data to 0.9" (degrading the resolution by about 30 percent) reduces the noise by a factor of $\approx$3. We also present the first public release (DR1.1.0) of the pjpipe processed eight-band 2-21 $μ$m imaging for all nineteen galaxies in the PHANGS-JWST Cycle 1 Treasury program. An additional 55 galaxies will soon follow from a new PHANGS-JWST Cycle 2 Treasury program.
title	PHANGS-JWST: Data Processing Pipeline and First Full Public Data Release
topic	Astrophysics of Galaxies
url	https://arxiv.org/abs/2401.15142