SDSS-IV MaStar: a large and comprehensive empirical stellar spectral library—first release

Renbin Yan; Yanping Chen; Daniel Lazarz; Dmitry Bizyaev; Claudia Maraston; Guy S. Stringfellow; Kyle McCarthy; Sofia Meneses-Goytia; David R. Law; Daniel Thomas; Jesus Falcon Barroso; José R. Sánchez-Gallego; Edward Schlafly; Zheng Zheng; Maria Argudo-Fernández; Rachael L. Beaton; Timothy C. Beers; Matthew Bershady; Michael R. Blanton; Joel Brownstein; Kevin Bundy; Kenneth C. Chambers; Brian Cherinka; Nathan De Lee; Niv Drory; Lluís Galbany; Jon Holtzman; Julie Imig; Nick Kaiser; Karen Kinemuchi; Chao Liu; A-Li Luo; Eugene Magnier; Steven Majewski; Preethi Nair; Audrey Oravetz; Daniel Oravetz; Kaike Pan; Jennifer Sobeck; Keivan Stassun; Michael Talbot; Christy Tremonti; Christopher Waters; Anne-Marie Weijmans; Ronald Wilhelm; Gail Zasowski; Gang Zhao; Yong-Heng Zhao

doi:10.3847/1538-4357/ab3ebc

SDSS-IV MaStar: a large and comprehensive empirical stellar spectral library—first release

Renbin Yan, Yanping Chen, Daniel Lazarz, Dmitry Bizyaev, Claudia Maraston, Guy S. Stringfellow, Kyle McCarthy, Sofia Meneses-Goytia, David R. Law, Daniel Thomas, Jesus Falcon Barroso, José R. Sánchez-Gallego, Edward Schlafly, Zheng Zheng, Maria Argudo-Fernández, Rachael L. Beaton, Timothy C. Beers, Matthew Bershady, Michael R. Blanton, Joel BrownsteinKevin Bundy, Kenneth C. Chambers, Brian Cherinka, Nathan De Lee, Niv Drory, Lluís Galbany, Jon Holtzman, Julie Imig, Nick Kaiser, Karen Kinemuchi, Chao Liu, A-Li Luo, Eugene Magnier, Steven Majewski, Preethi Nair, Audrey Oravetz, Daniel Oravetz, Kaike Pan, Jennifer Sobeck, Keivan Stassun, Michael Talbot, Christy Tremonti, Christopher Waters, Anne-Marie Weijmans, Ronald Wilhelm, Gail Zasowski, Gang Zhao, Yong-Heng Zhao

School of Physics and Astronomy

Research output: Contribution to journal › Article › peer-review

Abstract

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.

Original language	English
Article number	175
Pages (from-to)	1-26
Number of pages	26
Journal	Astrophysical Journal
Volume	883
Issue number	2
DOIs	https://doi.org/10.3847/1538-4357/ab3ebc
Publication status	Published - 3 Oct 2019

Keywords

Catalogs
Galaxy: stellar content
Stars: fundamental parameters
Stars: general
Techniques: spectroscopic

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10.3847/1538-4357/ab3ebc

Yan_2019_ApJ_883_175
Copyright © American Astronomical Society. This work has been made available online in accordance with publisher policies or with permission. Permission for further reuse of this content should be sought from the publisher or the rights holder. This is the final published version of the work, which was originally published at https://doi.org/10.3847/1538-4357/ab3ebc
Final published version, 3.07 MB

http://adsabs.harvard.edu/abs/2018arXiv181202745Y

SDSS-IV Data Release 15 (DR15)
Weijmans, A.-M. (Creator), Sloan Digitial Sky Survey IV (SDSS-IV), 10 Dec 2018
http://www.sdss.org/dr15
Dataset

Cite this

Yan, R., Chen, Y., Lazarz, D., Bizyaev, D., Maraston, C., Stringfellow, G. S., McCarthy, K., Meneses-Goytia, S., Law, D. R., Thomas, D., Falcon Barroso, J., Sánchez-Gallego, J. R., Schlafly, E., Zheng, Z., Argudo-Fernández, M., Beaton, R. L., Beers, T. C., Bershady, M., Blanton, M. R., ... Zhao, Y.-H. (2019). SDSS-IV MaStar: a large and comprehensive empirical stellar spectral library—first release. Astrophysical Journal, 883(2), 1-26. Article 175. https://doi.org/10.3847/1538-4357/ab3ebc

@article{e041a815b259420c9a777e9f11c82439,

title = "SDSS-IV MaStar: a large and comprehensive empirical stellar spectral library—first release",

abstract = "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 {\AA} 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.",

keywords = "Catalogs, Galaxy: stellar content, Stars: fundamental parameters, Stars: general, Techniques: spectroscopic",

author = "Renbin Yan and Yanping Chen and Daniel Lazarz and Dmitry Bizyaev and Claudia Maraston and Stringfellow, {Guy S.} and Kyle McCarthy and Sofia Meneses-Goytia and Law, {David R.} and Daniel Thomas and {Falcon Barroso}, Jesus and S{\'a}nchez-Gallego, {Jos{\'e} R.} and Edward Schlafly and Zheng Zheng and Maria Argudo-Fern{\'a}ndez and Beaton, {Rachael L.} and Beers, {Timothy C.} and Matthew Bershady and Blanton, {Michael R.} and Joel Brownstein and Kevin Bundy and Chambers, {Kenneth C.} and Brian Cherinka and {De Lee}, Nathan and Niv Drory and Llu{\'i}s Galbany and Jon Holtzman and Julie Imig and Nick Kaiser and Karen Kinemuchi and Chao Liu and A-Li Luo and Eugene Magnier and Steven Majewski and Preethi Nair and Audrey Oravetz and Daniel Oravetz and Kaike Pan and Jennifer Sobeck and Keivan Stassun and Michael Talbot and Christy Tremonti and Christopher Waters and Anne-Marie Weijmans and Ronald Wilhelm and Gail Zasowski and Gang Zhao and Yong-Heng Zhao",

year = "2019",

month = oct,

day = "3",

doi = "10.3847/1538-4357/ab3ebc",

language = "English",

volume = "883",

pages = "1--26",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "American Astronomical Society",

number = "2",

}

Yan, R, Chen, Y, Lazarz, D, Bizyaev, D, Maraston, C, Stringfellow, GS, McCarthy, K, Meneses-Goytia, S, Law, DR, Thomas, D, Falcon Barroso, J, Sánchez-Gallego, JR, Schlafly, E, Zheng, Z, Argudo-Fernández, M, Beaton, RL, Beers, TC, Bershady, M, Blanton, MR, Brownstein, J, Bundy, K, Chambers, KC, Cherinka, B, De Lee, N, Drory, N, Galbany, L, Holtzman, J, Imig, J, Kaiser, N, Kinemuchi, K, Liu, C, Luo, A-L, Magnier, E, Majewski, S, Nair, P, Oravetz, A, Oravetz, D, Pan, K, Sobeck, J, Stassun, K, Talbot, M, Tremonti, C, Waters, C, Weijmans, A-M, Wilhelm, R, Zasowski, G, Zhao, G & Zhao, Y-H 2019, 'SDSS-IV MaStar: a large and comprehensive empirical stellar spectral library—first release', Astrophysical Journal, vol. 883, no. 2, 175, pp. 1-26. https://doi.org/10.3847/1538-4357/ab3ebc

TY - JOUR

T1 - SDSS-IV MaStar

T2 - 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 - Falcon Barroso, Jesus

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: spectroscopic

U2 - 10.3847/1538-4357/ab3ebc

DO - 10.3847/1538-4357/ab3ebc

M3 - Article

SN - 0004-637X

VL - 883

SP - 1

EP - 26

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 2

M1 - 175

ER -

SDSS-IV MaStar: a large and comprehensive empirical stellar spectral library—first release

Abstract

Keywords

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SDSS-IV Data Release 15 (DR15)

Cite this