{"about":{"site":"https://codewithpapers.app","non_affiliation":"Code with Papers and Syntology are not affiliated with, endorsed by, or sponsored by Papers with Code, Meta, or the pwc-archive mirror.","licence":"CC BY-SA 4.0","licence_url":"https://creativecommons.org/licenses/by-sa/4.0/legalcode","attribution":"https://codewithpapers.app/attribution","modified":"archive material modified by Syntology; see the attribution page"},"url":"/paper/the-pan-starrs1-surveys","title":"The Pan-STARRS1 Surveys","arxiv_id":"1612.05560","date":"2016-12-16","proceeding":null,"authors":["K. C. Chambers","E. A. Magnier","N. Metcalfe","H. A. Flewelling","M. E. Huber","C. Z. Waters","L. Denneau","P. W. Draper","D. Farrow","D. P. Finkbeiner","C. Holmberg","J. Koppenhoefer","P. A. Price","A. Rest","R. P. Saglia","E. F. Schlafly","S. J. Smartt","W. Sweeney","R. J. Wainscoat","W. S. Burgett","S. Chastel","T. Grav","J. N. Heasley","K. W. Hodapp","R. Jedicke","N. Kaiser","R. -P. Kudritzki","G. A. Luppino","R. H. Lupton","D. G. Monet","J. S. Morgan","P. M. Onaka","B. Shiao","C. W. Stubbs","J. L. Tonry","R. White","E. Bañados","E. F. Bell","R. Bender","E. J. Bernard","M. Boegner","F. Boffi","M. T. Botticella","A. Calamida","S. Casertano","W. -P. Chen","X. Chen","S. Cole","N. Deacon","C. Frenk","A. Fitzsimmons","S. Gezari","V. Gibbs","C. Goessl","T. Goggia","R. Gourgue","B. Goldman","P. Grant","E. K. Grebel","N. C. Hambly","G. Hasinger","A. F. Heavens","T. M. Heckman","R. Henderson","T. Henning","M. Holman","U. Hopp","W. -H. Ip","S. Isani","M. Jackson","C. D. Keyes","A. M. Koekemoer","R. Kotak","D. Le","D. Liska","K. S. Long","J. R. Lucey","M. Liu","N. F. Martin","G. Masci","B. McLean","E. Mindel","P. Misra","E. Morganson","D. N. A. Murphy","A. Obaika","G. Narayan","M. A. Nieto-Santisteban","P. Norberg","J. A. Peacock","E. A. Pier","M. Postman","N. Primak","C. Rae","A. Rai","A. Riess","A. Riffeser","H. W. Rix","S. Röser","R. Russel","L. Rutz","E. Schilbach","A. S. B. Schultz","D. Scolnic","L. Strolger","A. Szalay","S. Seitz","E. Small","K. W. Smith","D. R. Soderblom","P. Taylor","R. Thomson","A. N. Taylor","A. R. Thakar","J. Thiel","D. Thilker","D. Unger","Y. Urata","J. Valenti","J. Wagner","T. Walder","F. Walter","S. P. Watters","S. Werner","W. M. Wood-Vasey","R. Wyse"],"abstract":"Pan-STARRS1 has carried out a set of distinct synoptic imaging sky surveys including the $3\\pi$ Steradian Survey and the Medium Deep Survey in 5 bands ($grizy_{P1}$). The mean 5$\\sigma$ point source limiting sensitivities in the stacked 3$\\pi$ Steradian Survey in $grizy_{P1}$ are (23.3, 23.2, 23.1, 22.3, 21.4) respectively. The upper bound on the systematic uncertainty in the photometric calibration across the sky is 7-12 millimag depending on the bandpass. The systematic uncertainty of the astrometric calibration using the Gaia frame comes from a comparison of the results with Gaia: the standard deviation of the mean and median residuals ($ \\Delta ra, \\Delta dec $) are (2.3, 1.7) milliarcsec, and (3.1, 4.8) milliarcsec respectively. The Pan-STARRS system and the design of the PS1 surveys are described and an overview of the resulting image and catalog data products and their basic characteristics are described together with a summary of important results. The images, reduced data products, and derived data products from the Pan-STARRS1 surveys are available to the community from the Mikulski Archive for Space Telescopes (MAST) at STScI.","url_abs":"http://arxiv.org/abs/1612.05560v4","url_pdf":"http://arxiv.org/pdf/1612.05560v4.pdf","source":{"archive":"pwc-archive (Hugging Face), CC BY-SA 4.0","snapshot":"2025-07-28","licence_url":"https://creativecommons.org/licenses/by-sa/4.0/legalcode","row_kind":"links_only","authors_date_abstract":"arXiv metadata, CC0 1.0 (https://info.arxiv.org/help/license), from the Kaggle arXiv metadata snapshot of 2026-09-12"},"code_links":[{"paper_slug":"the-pan-starrs1-surveys","repo_url":"https://github.com/sshah1502/irgsc","is_official":0,"mentioned_in_paper":0,"mentioned_in_github":1,"framework":"tf","reach":{"status":"ok","spdx":"MIT"}},{"paper_slug":"the-pan-starrs1-surveys","repo_url":"https://github.com/tmtsoftware/dms-irgsc","is_official":0,"mentioned_in_paper":0,"mentioned_in_github":1,"framework":"tf","reach":{"status":"ok"}}],"tasks":[],"methods":[],"datasets_introduced":[],"methods_introduced":[],"results":[],"syntology":{"atlas_url":"https://app.syntology.ai/?focus=1612.05560","mcp":{"get_harvested_code_for_paper":{"arxiv_id":"1612.05560"}},"developers":"https://syntology.ai/developers","read_at":"2026-09-24T18:15:14+00:00","read_at_is":"when the build read Syntology's graph, not when any sample ran","claim":"Per-sample execution status on synthesized fixtures; not a correctness claim about the paper. 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