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SDSS-IV MaNGA IFS GALAXY SURVEY-SURVEY DESIGN, EXECUTION, AND INITIAL DATA QUALITY
Yan, Renbin1; Bundy, Kevin2; Law, David R.3; Bershady, Matthew A.4; Andrews, Brett5,6; Cherinka, Brian7; Diamond-Stanic, Aleksandar M.4; Drory, Niv8; MacDonald, Nicholas9; Sanchez-Gallego, Jose R.9; Thomas, Daniel10,41; Wake, David A.11; Weijmans, Anne-Marie12; Westfall, Kyle B.10,41; Zhang, Kai1; Aragon-Salamanca, Alfonso13; Belfiore, Francesco14,15; Bizyaev, Dmitry16,17,18; Blanc, Guillermo A.19,20; Blanton, Michael R.21; Brownstein, Joel22; Cappellari, Michele23; D'Souza, Richard24; Emsellem, Eric25,26,27; Fu, Hai28; Gaulme, Patrick16,17; Graham, Mark T.23; Goddard, Daniel41; Gunn, James E.29; Harding, Paul30; Jones, Amy24; Kinemuchi, Karen16,17; Li, Cheng31,32,33; Li, Hongyu34,35; Maiolino, Roberto15; Mao, Shude32,33,34,36; Maraston, Claudia10,41; Masters, Karen10,41; Merrifield, Michael R.13; Oravetz, Daniel16,17; Pan, Kaike16,17; Parejko, John K.9; Sanchez, Sebastian F.37; Schlegel, David38; Simmons, Audrey16,17; Thanjavur, Karun39; Tinker, Jeremy21; Tremonti, Christy4; van den Bosch, Remco40; Zheng, Zheng34
2016-12-01
发表期刊ASTRONOMICAL JOURNAL
卷号152期号:6
摘要The MaNGA Survey (Mapping Nearby Galaxies at Apache Point Observatory) is one of three core programs in the Sloan Digital Sky Survey IV. It is obtaining integral field spectroscopy for 10,000. nearby galaxies at a spectral resolution of R similar to 2000 from 3622 to 10354 angstrom. The design of the survey is driven by a set of science requirements on the precision of estimates of the following properties: star formation rate surface density, gas metallicity, gravitational mass as a function of radius. We describe how these science requirements set the depth of the observations and dictate sample selection. The majority of targeted galaxies are selected to ensure uniform spatial coverage in units of effective radius (R-e) while maximizing spatial resolution. About two-thirds of the sample is covered out to 1.5R(e) (Primary sample), and one-third. of the sample is covered to 2.5R(e) (Secondary sample). We describe the survey execution with details that would be useful in the design of similar future surveys. We also present statistics on the achieved data quality, specifically. the point-spread function, sampling uniformity, spectral resolution, sky subtraction, and flux calibration. For our Primary sample, the median r-band signal-to-noise ratio is similar to 70 per 1.4 angstrom pixel for spectra stacked between 1R(e) and 1.5R(e). Measurements of various galaxy properties from the first-year data show that we are meeting or exceeding the defined requirements for the majority of our science goals.
文章类型Article
关键词Galaxies: Evolution Galaxies: General Surveys Techniques: Imaging Spectroscopy
WOS标题词Science & Technology ; Physical Sciences
资助者World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan ; World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan ; Leverhulme Trust Early Career Fellowship ; Leverhulme Trust Early Career Fellowship ; Grainger Foundation ; Grainger Foundation ; Royal Society University Research Fellowship ; Royal Society University Research Fellowship ; Strategic Priority Research Program "The Emergence of Cosmological Structures" of the Chinese Academy of Sciences(XDB09000000) ; Strategic Priority Research Program "The Emergence of Cosmological Structures" of the Chinese Academy of Sciences(XDB09000000) ; National Natural Science Foundation of China (NSFC)(11333003 ; National Natural Science Foundation of China (NSFC)(11333003 ; STFC ; STFC ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; U.S. Department of Energy Office of Science ; U.S. Department of Energy Office of Science ; Center for High-Performance Computing at the University of Utah ; Center for High-Performance Computing at the University of Utah ; Carnegie Institution for Science ; Carnegie Institution for Science ; Carnegie Mellon University ; Carnegie Mellon University ; Chilean Participation Group ; Chilean Participation Group ; French Participation Group ; French Participation Group ; Harvard-Smithsonian Center for Astrophysics ; Harvard-Smithsonian Center for Astrophysics ; Instituto de Astrofisica de Canarias ; Instituto de Astrofisica de Canarias ; Johns Hopkins University ; Johns Hopkins University ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Leibniz Institut fur Astrophysik Potsdam (AIP) ; Leibniz Institut fur Astrophysik Potsdam (AIP) ; Max-Planck-Institut fur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fur Astrophysik (MPA Garching) ; Max-Planck-Institut fur Astrophysik (MPA Garching) ; Max-Planck-Institut fur Extraterrestrische Physik (MPE) ; Max-Planck-Institut fur Extraterrestrische Physik (MPE) ; National Astronomical Observatory of China ; National Astronomical Observatory of China ; New Mexico State University ; New Mexico State University ; New York University ; New York University ; University of Notre Dame ; University of Notre Dame ; Observatario Nacional/MCTI ; Observatario Nacional/MCTI ; Ohio State University ; Ohio State University ; Pennsylvania State University ; Pennsylvania State University ; Shanghai Astronomical Observatory ; Shanghai Astronomical Observatory ; United Kingdom Participation Group ; United Kingdom Participation Group ; Universidad Nacional Autonoma de Mexico ; Universidad Nacional Autonoma de Mexico ; University of Arizona ; University of Arizona ; University of Colorado Boulder ; University of Colorado Boulder ; University of Oxford ; University of Oxford ; University of Portsmouth ; University of Portsmouth ; University of Utah ; University of Utah ; University of Virginia ; University of Virginia ; University of Washington ; University of Washington ; University of Wisconsin ; University of Wisconsin ; Vanderbilt University ; Vanderbilt University ; Yale University ; Yale University ; (NSF/AST 1517007) ; (NSF/AST 1517007) ; (RSF 14-50-00043) ; (RSF 14-50-00043) ; 11390372) ; 11390372) ; World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan ; World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan ; Leverhulme Trust Early Career Fellowship ; Leverhulme Trust Early Career Fellowship ; Grainger Foundation ; Grainger Foundation ; Royal Society University Research Fellowship ; Royal Society University Research Fellowship ; Strategic Priority Research Program "The Emergence of Cosmological Structures" of the Chinese Academy of Sciences(XDB09000000) ; Strategic Priority Research Program "The Emergence of Cosmological Structures" of the Chinese Academy of Sciences(XDB09000000) ; National Natural Science Foundation of China (NSFC)(11333003 ; National Natural Science Foundation of China (NSFC)(11333003 ; STFC ; STFC ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; U.S. Department of Energy Office of Science ; U.S. Department of Energy Office of Science ; Center for High-Performance Computing at the University of Utah ; Center for High-Performance Computing at the University of Utah ; Carnegie Institution for Science ; Carnegie Institution for Science ; Carnegie Mellon University ; Carnegie Mellon University ; Chilean Participation Group ; Chilean Participation Group ; French Participation Group ; French Participation Group ; Harvard-Smithsonian Center for Astrophysics ; Harvard-Smithsonian Center for Astrophysics ; Instituto de Astrofisica de Canarias ; Instituto de Astrofisica de Canarias ; Johns Hopkins University ; Johns Hopkins University ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Leibniz Institut fur Astrophysik Potsdam (AIP) ; Leibniz Institut fur Astrophysik Potsdam (AIP) ; Max-Planck-Institut fur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fur Astrophysik (MPA Garching) ; Max-Planck-Institut fur Astrophysik (MPA Garching) ; Max-Planck-Institut fur Extraterrestrische Physik (MPE) ; Max-Planck-Institut fur Extraterrestrische Physik (MPE) ; National Astronomical Observatory of China ; National Astronomical Observatory of China ; New Mexico State University ; New Mexico State University ; New York University ; New York University ; University of Notre Dame ; University of Notre Dame ; Observatario Nacional/MCTI ; Observatario Nacional/MCTI ; Ohio State University ; Ohio State University ; Pennsylvania State University ; Pennsylvania State University ; Shanghai Astronomical Observatory ; Shanghai Astronomical Observatory ; United Kingdom Participation Group ; United Kingdom Participation Group ; Universidad Nacional Autonoma de Mexico ; Universidad Nacional Autonoma de Mexico ; University of Arizona ; University of Arizona ; University of Colorado Boulder ; University of Colorado Boulder ; University of Oxford ; University of Oxford ; University of Portsmouth ; University of Portsmouth ; University of Utah ; University of Utah ; University of Virginia ; University of Virginia ; University of Washington ; University of Washington ; University of Wisconsin ; University of Wisconsin ; Vanderbilt University ; Vanderbilt University ; Yale University ; Yale University ; (NSF/AST 1517007) ; (NSF/AST 1517007) ; (RSF 14-50-00043) ; (RSF 14-50-00043) ; 11390372) ; 11390372)
DOI10.3847/0004-6256/152/6/197
关键词[WOS]DIGITAL SKY SURVEY ; STAR-FORMING GALAXIES ; MASS-METALLICITY RELATION ; STELLAR POPULATION GRADIENTS ; EARLY DATA RELEASE ; 2.5 M TELESCOPE ; TO-LIGHT RATIO ; SAMI GALAXY ; NEARBY GALAXIES ; SAURON PROJECT
收录类别SCI
语种英语
资助者World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan ; World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan ; Leverhulme Trust Early Career Fellowship ; Leverhulme Trust Early Career Fellowship ; Grainger Foundation ; Grainger Foundation ; Royal Society University Research Fellowship ; Royal Society University Research Fellowship ; Strategic Priority Research Program "The Emergence of Cosmological Structures" of the Chinese Academy of Sciences(XDB09000000) ; Strategic Priority Research Program "The Emergence of Cosmological Structures" of the Chinese Academy of Sciences(XDB09000000) ; National Natural Science Foundation of China (NSFC)(11333003 ; National Natural Science Foundation of China (NSFC)(11333003 ; STFC ; STFC ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; U.S. Department of Energy Office of Science ; U.S. Department of Energy Office of Science ; Center for High-Performance Computing at the University of Utah ; Center for High-Performance Computing at the University of Utah ; Carnegie Institution for Science ; Carnegie Institution for Science ; Carnegie Mellon University ; Carnegie Mellon University ; Chilean Participation Group ; Chilean Participation Group ; French Participation Group ; French Participation Group ; Harvard-Smithsonian Center for Astrophysics ; Harvard-Smithsonian Center for Astrophysics ; Instituto de Astrofisica de Canarias ; Instituto de Astrofisica de Canarias ; Johns Hopkins University ; Johns Hopkins University ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Leibniz Institut fur Astrophysik Potsdam (AIP) ; Leibniz Institut fur Astrophysik Potsdam (AIP) ; Max-Planck-Institut fur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fur Astrophysik (MPA Garching) ; Max-Planck-Institut fur Astrophysik (MPA Garching) ; Max-Planck-Institut fur Extraterrestrische Physik (MPE) ; Max-Planck-Institut fur Extraterrestrische Physik (MPE) ; National Astronomical Observatory of China ; National Astronomical Observatory of China ; New Mexico State University ; New Mexico State University ; New York University ; New York University ; University of Notre Dame ; University of Notre Dame ; Observatario Nacional/MCTI ; Observatario Nacional/MCTI ; Ohio State University ; Ohio State University ; Pennsylvania State University ; Pennsylvania State University ; Shanghai Astronomical Observatory ; Shanghai Astronomical Observatory ; United Kingdom Participation Group ; United Kingdom Participation Group ; Universidad Nacional Autonoma de Mexico ; Universidad Nacional Autonoma de Mexico ; University of Arizona ; University of Arizona ; University of Colorado Boulder ; University of Colorado Boulder ; University of Oxford ; University of Oxford ; University of Portsmouth ; University of Portsmouth ; University of Utah ; University of Utah ; University of Virginia ; University of Virginia ; University of Washington ; University of Washington ; University of Wisconsin ; University of Wisconsin ; Vanderbilt University ; Vanderbilt University ; Yale University ; Yale University ; (NSF/AST 1517007) ; (NSF/AST 1517007) ; (RSF 14-50-00043) ; (RSF 14-50-00043) ; 11390372) ; 11390372) ; World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan ; World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan ; Leverhulme Trust Early Career Fellowship ; Leverhulme Trust Early Career Fellowship ; Grainger Foundation ; Grainger Foundation ; Royal Society University Research Fellowship ; Royal Society University Research Fellowship ; Strategic Priority Research Program "The Emergence of Cosmological Structures" of the Chinese Academy of Sciences(XDB09000000) ; Strategic Priority Research Program "The Emergence of Cosmological Structures" of the Chinese Academy of Sciences(XDB09000000) ; National Natural Science Foundation of China (NSFC)(11333003 ; National Natural Science Foundation of China (NSFC)(11333003 ; STFC ; STFC ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; U.S. Department of Energy Office of Science ; U.S. Department of Energy Office of Science ; Center for High-Performance Computing at the University of Utah ; Center for High-Performance Computing at the University of Utah ; Carnegie Institution for Science ; Carnegie Institution for Science ; Carnegie Mellon University ; Carnegie Mellon University ; Chilean Participation Group ; Chilean Participation Group ; French Participation Group ; French Participation Group ; Harvard-Smithsonian Center for Astrophysics ; Harvard-Smithsonian Center for Astrophysics ; Instituto de Astrofisica de Canarias ; Instituto de Astrofisica de Canarias ; Johns Hopkins University ; Johns Hopkins University ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Leibniz Institut fur Astrophysik Potsdam (AIP) ; Leibniz Institut fur Astrophysik Potsdam (AIP) ; Max-Planck-Institut fur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fur Astrophysik (MPA Garching) ; Max-Planck-Institut fur Astrophysik (MPA Garching) ; Max-Planck-Institut fur Extraterrestrische Physik (MPE) ; Max-Planck-Institut fur Extraterrestrische Physik (MPE) ; National Astronomical Observatory of China ; National Astronomical Observatory of China ; New Mexico State University ; New Mexico State University ; New York University ; New York University ; University of Notre Dame ; University of Notre Dame ; Observatario Nacional/MCTI ; Observatario Nacional/MCTI ; Ohio State University ; Ohio State University ; Pennsylvania State University ; Pennsylvania State University ; Shanghai Astronomical Observatory ; Shanghai Astronomical Observatory ; United Kingdom Participation Group ; United Kingdom Participation Group ; Universidad Nacional Autonoma de Mexico ; Universidad Nacional Autonoma de Mexico ; University of Arizona ; University of Arizona ; University of Colorado Boulder ; University of Colorado Boulder ; University of Oxford ; University of Oxford ; University of Portsmouth ; University of Portsmouth ; University of Utah ; University of Utah ; University of Virginia ; University of Virginia ; University of Washington ; University of Washington ; University of Wisconsin ; University of Wisconsin ; Vanderbilt University ; Vanderbilt University ; Yale University ; Yale University ; (NSF/AST 1517007) ; (NSF/AST 1517007) ; (RSF 14-50-00043) ; (RSF 14-50-00043) ; 11390372) ; 11390372)
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
WOS记录号WOS:000396039500001
引用统计
文献类型期刊论文
条目标识符http://ir.bao.ac.cn/handle/114a11/8257
专题星系宇宙学研究部
作者单位1.Univ Kentucky, Dept Phys & Astron, 505 Rose St, Lexington, KY 40506 USA
2.Univ Tokyo, Kavli IPMU WPI, UTIAS, Kashiwa, Chiba 2778583, Japan
3.Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA
4.Univ Wisconsin, Dept Astron, 475 N Charter St, Madison, WI 53706 USA
5.Univ Pittsburgh, Dept Phys & Astron, 3941 OHara St, Pittsburgh, PA 15260 USA
6.Univ Pittsburgh, Pittsburgh Particle Phys Astrophys & Cosmol Ctr P, 3941 OHara St, Pittsburgh, PA 15260 USA
7.Johns Hopkins Univ, Bloomberg Ctr, Dept Phys & Astron, 3400 N Charles St, Baltimore, MD 21218 USA
8.Univ Texas Austin, McDonald Observ, 1 Univ Stn, Austin, TX 78712 USA
9.Univ Washington, Dept Astron, Box 351580, Seattle, WA 98195 USA
10.Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth, Hants, England
11.Open Univ, Dept Phys Sci, Milton Keynes MK7 6AA, Bucks, England
12.Univ St Andrews, Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland
13.Univ Nottingham, Sch Phys & Astron, Univ Pk, Nottingham NG7 2RD, England
14.Univ Cambridge, Cavendish Lab, 19 JJ Thomson Ave, Cambridge CB3 0HE, England
15.Univ Cambridge, Kavli Inst Cosmol, Madingley Rd, Cambridge CB3 0HA, England
16.Apache Point Observ, POB 59, Sunspot, NM 88349 USA
17.New Mexico State Univ, POB 59, Sunspot, NM 88349 USA
18.Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Univ Skij Pr 13, Moscow, Russia
19.Univ Chile, Dept Astron, Camino Observ 1515, Santiago, Chile
20.CATA, Camino Observ 1515, Santiago, Chile
21.NYU, Dept Phys, Ctr Cosmol & Particle Phys, 4 Washington Pl, New York, NY 10003 USA
22.Univ Utah, Dept Phys & Astron, 115 S 1400 E, Salt Lake City, UT 84112 USA
23.Univ Oxford, Subdept Astrophys, Dept Phys, DenysWilkinson Bldg,Keble Rd, Oxford OX1 3RH, England
24.Max Plank Inst Astrophys, D-85741 Garching, Germany
25.European Southern Observ, Karl Schwarzschild Str 2, D-85748 Garching, Germany
26.Univ Lyon 1, Observ Lyon, Ctr Rech Astrophys Lyon, 9 Ave Charles Andre, F-69561 St Genis Laval, France
27.Ecole Normale Super Lyon, 9 Ave Charles Andre, F-69230 St Genis Laval, France
28.Univ Iowa, Dept Phys & Astron, 203 Van Allen Hall, Iowa City, IA 52242 USA
29.Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA
30.Case Western Reserve Univ, Dept Astron, Cleveland, OH 44106 USA
31.Shanghai Astron Observ, Nandan Rd 80, Shanghai 200030, Peoples R China
32.Tsinghua Univ, Dept Phys, Beijing 100086, Peoples R China
33.Tsinghua Univ, Tsinghua Ctr Astrophys, Beijing 100086, Peoples R China
34.Chinese Acad Sci, Natl Astron Observ, 20A Datun Rd, Beijing 100012, Peoples R China
35.Univ Chinese Acad Sci, Beijing 100049, Peoples R China
36.Univ Manchester, Sch Phys & Astron, Jodrell Bank Ctr Astrophys, Oxford Rd, Oxford M13 9PL, England
37.Univ Nacl Autonoma Mexico, Inst Astron, AP 70-264, Mexico City 04510, DF, Mexico
38.Lawrence Berkeley Natl Lab, Div Phys, Berkeley, CA 94720 USA
39.Univ Victoria, Dept Phys & Astron, Victoria, BC V8P 5C2, Canada
40.Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany
41.SEPnet, South East Phys Network, Southampton, Hants, England
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GB/T 7714
Yan, Renbin,Bundy, Kevin,Law, David R.,et al. SDSS-IV MaNGA IFS GALAXY SURVEY-SURVEY DESIGN, EXECUTION, AND INITIAL DATA QUALITY[J]. ASTRONOMICAL JOURNAL,2016,152(6).
APA Yan, Renbin.,Bundy, Kevin.,Law, David R..,Bershady, Matthew A..,Andrews, Brett.,...&Zheng, Zheng.(2016).SDSS-IV MaNGA IFS GALAXY SURVEY-SURVEY DESIGN, EXECUTION, AND INITIAL DATA QUALITY.ASTRONOMICAL JOURNAL,152(6).
MLA Yan, Renbin,et al."SDSS-IV MaNGA IFS GALAXY SURVEY-SURVEY DESIGN, EXECUTION, AND INITIAL DATA QUALITY".ASTRONOMICAL JOURNAL 152.6(2016).
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