4.6 Article

SDSS-IV MaNGA: pyPipe3D Analysis Release for 10,000 Galaxies

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IOP Publishing Ltd
DOI: 10.3847/1538-4365/ac7b8f

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资金

  1. CONACYT [CB-285080, FC-2016-01-1916, CF19-39578]
  2. National Autonomous University of Mexico (UNAM) [DGAPA/PAPIIT BG100622]
  3. Alfred P. Sloan Foundation
  4. U.S. Department of Energy Office of Science
  5. Center for High Performance Computing at the University of Utah
  6. Brazilian Participation Group
  7. Carnegie Institution for Science
  8. Carnegie Mellon University
  9. Center for Astrophysics | Harvard Smithsonian
  10. Chilean Participation Group
  11. French Participation Group
  12. Instituto de Astrofisica de Canarias
  13. Johns Hopkins University
  14. Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo
  15. Korean Participation Group
  16. Lawrence Berkeley National Laboratory
  17. Leibniz Institut fur Astrophysik Potsdam (AIP)
  18. Max-Planck-Institut fur Astronomie (MPIA Heidelberg)
  19. Max-Planck-Institut fur Astrophysik (MPA Garching)
  20. Max-Planck-Institut fur Extraterrestrische Physik (MPE)
  21. National Astronomical Observatories of China
  22. New Mexico State University
  23. New York University
  24. University of Notre Dame
  25. Observatario Nacional/MCTI
  26. Ohio State University
  27. Pennsylvania State University
  28. Shanghai Astronomical Observatory
  29. United Kingdom Participation Group
  30. Universidad Nacional Autonoma de Mexico
  31. University of Arizona
  32. University of Colorado Boulder
  33. University of Oxford
  34. University of Portsmouth
  35. University of Utah
  36. University of Virginia
  37. University of Washington
  38. University of Wisconsin
  39. Vanderbilt University
  40. Yale University
  41. [PAPIIT-DGAPA-IN100519]
  42. [IG100622]

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In this article, we present an analysis of the final MaNGA data set included in the Sloan Digital Sky Survey data release 17 using the pyPipe3D pipeline. The pipeline extracts spatially resolved spectroscopic properties from the integral field spectroscopic (IFS) data cubes, including the stellar population and ionized gas emission lines. A detailed description of the analysis process, pipeline, adopted stellar population library, morphological and photometric analysis, data model for spatially resolved properties, and individual galaxy properties in the final catalog is provided. Comparisons with previous pipeline versions and other tools using the data set are also included, along with a practical example of how to use the full data set and final catalog.
We present here the analysis performed using the pyPipe3D pipeline for the final MaNGA data set included in the Sloan Digital Sky Survey data release 17. This data set comprises more than 10,000 individual data cubes, being the integral field spectroscopic (IFS) galaxy survey with the largest number of galaxies. pyPipe3D processes the IFS data cubes to extract spatially resolved spectroscopic properties of both the stellar population and the ionized gas emission lines. A brief summary of the properties of the sample and the characteristics of the analyzed data are included. The article provides details of: (i) the analysis performed; (ii) a description of the pipeline; (iii) the adopted stellar population library; (iv) the morphological and photometric analysis; (v) the adopted data model for the spatially resolved properties derived; and (vi) the individual integrated and characteristic galaxy properties included in the final catalog. Comparisons with the results from a previous version of the pipeline for earlier data releases and from other tools using this data set are included. A practical example of how to use the full data set and the final catalog illustrates how to handle the delivered product. Our full analysis can be accessed and downloaded from our web page.

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