Corpus ID: 55387148

MaNGA: Mapping Nearby Galaxies at Apache Point Observatory

@article{Weijmans2015MaNGAMN,
  title={MaNGA: Mapping Nearby Galaxies at Apache Point Observatory},
  author={A. Weijmans and on behalf of the MaNGA Team},
  journal={arXiv: Astrophysics of Galaxies},
  year={2015}
}
  • A. Weijmans, on behalf of the MaNGA Team
  • Published 2015
  • Physics
  • arXiv: Astrophysics of Galaxies
  • MaNGA (Mapping Nearby Galaxies at APO) is a galaxy integral-field spectroscopic survey within the fourth generation Sloan Digital Sky Survey (SDSS-IV). It will be mapping the composition and kinematics of gas and stars in 10,000 nearby galaxies, using 17 differently sized fiber bundles. MaNGA's goal is to provide new insights in galaxy formation and evolution, and to deliver a local benchmark for current and future high-redshift studies. 
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    SHOWING 1-2 OF 2 REFERENCES
    Observing Strategy for the SDSS-IV/MaNGA IFU Galaxy Survey
    • 137
    • PDF
    P-MaNGA: gradients in recent star formation histories as diagnostics for galaxy growth and death
    • 45
    • PDF