@article{01JEDVGMHA7APKZY0PB6CNEZCJ,
  abstract     = {{The exquisite angular resolution and sensitivity of JWST are 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 similar to 5-50 pc. 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%) reduces the noise by a factor of approximate to 3. We also present the first public release (DR1.1.0) of the pjpipe processed eight-band 2-21 mu m imaging for all 19 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.}},
  articleno    = {{13}},
  author       = {{Williams, Thomas G. and Lee, Janice C. and Larson, Kirsten L. and Leroy, Adam K. and Sandstrom, Karin and Schinnerer, Eva and Thilker, David A. and Belfiore, Francesco and Egorov, Oleg V. and Rosolowsky, Erik and Sutter, Jessica and DePasquale, Joseph and Pagan, Alyssa and Berger, Travis A. and Anand, Gagandeep S. and Barnes, Ashley T. and Bigiel, Frank and Boquien, Médéric and Cao, Yixian and Chastenet, Jérémy and Chevance, Mélanie and Chown, Ryan and Dale, Daniel A. and Deger, Sinan and Eibensteiner, Cosima and Emsellem, Eric and Faesi, Christopher M. and Glover, Simon C. O. and Grasha, Kathryn and Hannon, Stephen and Hassani, Hamid and Henshaw, Jonathan D. and Jiménez-Donaire, María J. and Kim, Jaeyeon and Klessen, Ralf S. and Koch, Eric W. and Li, Jing and Liu, Daizhong and van der Wel, Sharon Meidt and Méndez-Delgado, J. Eduardo and Murphy, Eric J. and Neumann, Justus and Neumann, Lukas and Neumayer, Nadine and Oakes, Elias K. and Pathak, Debosmita and Pety, Jérôme and Pinna, Francesca and Querejeta, Miguel and Ramambason, Lise and Romanelli, Andrea and Sormani, Mattia C. and Stuber, Sophia K. and Sun, Jiayi and Teng, Yu-Hsuan and Usero, Antonio and Watkins, Elizabeth J. and Weinbeck, Tony D.}},
  issn         = {{0067-0049}},
  journal      = {{ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES}},
  keywords     = {{HIGH ANGULAR RESOLUTION,MIDINFRARED EMISSION,NEARBY GALAXIES,STAR-FORMATION,FEEDBACK,ASTROPY,SPITZER,DUST,HST,REDUCTION}},
  language     = {{eng}},
  number       = {{1}},
  pages        = {{20}},
  title        = {{PHANGS-JWST : data-processing pipeline and first full public data release}},
  url          = {{http://doi.org/10.3847/1538-4365/ad4be5}},
  volume       = {{273}},
  year         = {{2024}},
}

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