The Data Reduction Pipeline for the SDSS-IV MaNGA IFU Galaxy Survey

Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) is an optical fiber-bundle integral-field unit (IFU) spectroscopic survey that is one of three core programs in the fourth-generation Sloan Digital Sky Survey (SDSS-IV). With a spectral coverage of 3622 - 10,354 Angstroms and an average foo...

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Veröffentlicht in:	arXiv.org 2016-08
Hauptverfasser:	Law, David R, Cherinka, Brian, Yan, Renbin, Andrews, Brett H, Bershady, Matthew A, Bizyaev, Dmitry, Blanc, Guillermo A, Blanton, Michael R, Bolton, Adam S, Brownstein, Joel R, Bundy, Kevin, Chen, Yanmei, Drory, Niv, D'Souza, Richard, Fu, Hai, Jones, Amy, Kauffmann, Guinevere, MacDonald, Nicholas, Masters, Karen L, Newman, Jeffrey A, Parejko, John K, Sánchez-Gallego, José R, Sánchez, Sebastian F, Schlegel, David J, Thomas, Daniel, Wake, David A, Weijmans, Anne-Marie, Westfall, Kyle B, Zhang, Kai
Format:	Artikel
Sprache:	eng
Schlagworte:	Algorithms Apertures Calibration Cubes Data reduction Data transmission Galaxies Mapping Optical fibers Physics - Instrumentation and Methods for Astrophysics Red shift Sky surveys (astronomy) Spatial resolution Spectra Spectral resolution Spectrophotometry Stars & galaxies Subtraction Surface brightness
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