OVERVIEW OF THE SDSS-IV MaNGA SURVEY: MAPPING NEARBY GALAXIES AT APACHE POINT OBSERVATORY
Kavli Institute for the Physics and Mathematics of the Universe · The University of Tokyo · +45 more institutions
Abstract
We present an overview of a new integral field spectroscopic survey called MaNGA (Mapping Nearby Galaxies at Apache Point Observatory), one of three core programs in the fourth-generation Sloan Digital Sky Survey (SDSS-IV) that began on 2014 July 1. MaNGA will investigate the internal kinematic structure and composition of gas and stars in an unprecedented sample of 10,000 nearby galaxies. We summarize essential characteristics of the instrument and survey design in the context of MaNGA’s key science goals and present prototype observations to demonstrate MaNGA’s scientific potential. MaNGA employs dithered observations with 17 fiber-bundle integral field units that vary in diameter from 12<i>"</i>…
Citation impact
- FWCI
- 46.72
- Percentile
- 100%
- References
- 95
Authors
68- KBKevin BundyCorresponding
Kavli Institute for the Physics and Mathematics of the Universe, The University of Tokyo
- MAMatthew A. Bershady
University of Wisconsin–Madison
- DRDavid R. Law
University of Toronto, Canadian Institute for Theoretical Astrophysics
- RYRenbin Yan
University of Kentucky
- NDNiv Drory
The University of Texas at Austin
Topics & keywords
- Galaxy
- Sky
- Observatory
- Context (archaeology)
- Stars
- Luminosity
- Redshift
- Star formation