TY - JOUR
T1 - SDSS-IV MaStar: a large and comprehensive empirical stellar spectral library-first release
AU - Yan, Renbin
AU - Chen, Yanping
AU - Lazarz, Daniel
AU - Bizyaev, Dmitry
AU - Maraston, Claudia
AU - Stringfellow, Guy S.
AU - McCarthy, Kyle
AU - Meneses-Goytia, Sofia
AU - Law, David R.
AU - Thomas, Daniel
AU - Barroso, Jesus Falcon
AU - Sánchez-Gallego, José R.
AU - Schlafly, Edward
AU - Zheng, Zheng
AU - Argudo-Fernández, Maria
AU - Beaton, Rachael L.
AU - Beers, Timothy C.
AU - Bershady, Matthew
AU - Blanton, Michael R.
AU - Brownstein, Joel
AU - Bundy, Kevin
AU - Chambers, Kenneth C.
AU - Cherinka, Brian
AU - De Lee, Nathan
AU - Drory, Niv
AU - Galbany, Lluís
AU - Holtzman, Jon
AU - Imig, Julie
AU - Kaiser, Nick
AU - Kinemuchi, Karen
AU - Liu, Chao
AU - Luo, A-Li
AU - Magnier, Eugene
AU - Majewski, Steven
AU - Nair, Preethi
AU - Oravetz, Audrey
AU - Oravetz, Daniel
AU - Pan, Kaike
AU - Sobeck, Jennifer
AU - Stassun, Keivan
AU - Talbot, Michael
AU - Tremonti, Christy
AU - Waters, Christopher
AU - Weijmans, Anne-Marie
AU - Wilhelm, Ronald
AU - Zasowski, Gail
AU - Zhao, Gang
AU - Zhao, Yong-Heng
PY - 2019/10/3
Y1 - 2019/10/3
N2 - We present the first release of the MaNGA Stellar Library (MaStar), which is a large, well-calibrated, high-quality empirical library covering the wavelength range 3622–10354 Å at a resolving power of R ~ 1800. The spectra were obtained using the same instrument as used by the Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) project, by piggybacking on the Sloan Digital Sky Survey (SDSS-IV)/Apache Point Observatory Galaxy Evolution Experiment 2-N (APOGEE-2N) observations. Compared to previous empirical libraries, the MaStar library will have a higher number of stars and a more comprehensive stellar-parameter coverage, especially of cool dwarfs, low-metallicity stars, and stars with different [α/Fe], achieved by a sophisticated target-selection strategy that takes advantage of stellar-parameter catalogs from the literature. This empirical library will provide a new basis for stellar-population synthesis and is particularly well suited for stellar-population analysis of MaNGA galaxies. The first version of the library contains 8646 high-quality per-visit spectra for 3321 unique stars. Compared to photometry, the relative flux calibration of the library is accurate to 3.9% in g − r, 2.7% in r − i, and 2.2% in i − z. The data are released as part of SDSS Data Release 15. We expect the final release of the library to contain more than 10,000 stars.
AB - We present the first release of the MaNGA Stellar Library (MaStar), which is a large, well-calibrated, high-quality empirical library covering the wavelength range 3622–10354 Å at a resolving power of R ~ 1800. The spectra were obtained using the same instrument as used by the Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) project, by piggybacking on the Sloan Digital Sky Survey (SDSS-IV)/Apache Point Observatory Galaxy Evolution Experiment 2-N (APOGEE-2N) observations. Compared to previous empirical libraries, the MaStar library will have a higher number of stars and a more comprehensive stellar-parameter coverage, especially of cool dwarfs, low-metallicity stars, and stars with different [α/Fe], achieved by a sophisticated target-selection strategy that takes advantage of stellar-parameter catalogs from the literature. This empirical library will provide a new basis for stellar-population synthesis and is particularly well suited for stellar-population analysis of MaNGA galaxies. The first version of the library contains 8646 high-quality per-visit spectra for 3321 unique stars. Compared to photometry, the relative flux calibration of the library is accurate to 3.9% in g − r, 2.7% in r − i, and 2.2% in i − z. The data are released as part of SDSS Data Release 15. We expect the final release of the library to contain more than 10,000 stars.
KW - catalogs
KW - Galaxy: stellar content
KW - stars: fundamental parameters
KW - stars: general
KW - techniques: spectrocopic
U2 - 10.3847/1538-4357/ab3ebc
DO - 10.3847/1538-4357/ab3ebc
M3 - Article
SN - 0004-637X
VL - 883
JO - Astrophysical Journal
JF - Astrophysical Journal
M1 - 175
ER -