Stellar Abundance and Galactic Chemical Evolution through LAMOST Spectroscopic Survey

By Gang Zhao, Yuqin Chen, Jian-rong Shi, Yan-chun Liang, J. Hou, Li Chen, Huawei Zhang, Aigen Li. 2006

141 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/3da6a2d4b112a26ad5967c4bc7111743b052dd52

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The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. Timothy C. Beers
2. Martin Asplund
3. Jo Bovy
4. Hans-Walter Rix
5. A. Frebel
6. I. Minchev
7. D. Huber
8. J. Norris

In Instrumentation

1. Timothy C. Beers
2. I. Minchev
3. D. Huber
4. A. Frebel
5. Jo Bovy
6. Hans-Walter Rix
7. D. Stello
8. J. Norris

Citations in the corpus

• Stellar Abundances for the Galactic Archeology (SAGA) Database — Compilation of the Characteristics of Known Extremely Metal-Poor Stars (2008, background): “LAMOST (Zhao et al. 2006) is a multi-fiber 4m telescope project that will enable up to 4000 stellar spectra to be obtained simultaneously in each exposure.”
• Gaia FGK benchmark stars: Metallicity (2013, background): “This is particularly important for the many Galactic surveys of stellar spectra under development (RAVE, Steinmetz et al. 2006); (LAMOST, Zhao et al. 2006); (APOGEE, Allende Prieto et al. 2008a); (HERMES, Freeman 2010); (Gaia, Perryman et al. 2001); (Gaia-ESO, Gilmore et al. 2012).”
• Chemodynamics of the Milky Way - I. The first year of APOGEE data (2013, unknown): “G A ] 5 F eb medium- and low-resolution surveys such as RAVE (Steinmetz et al. 2006), LAMOST/LEGUE (Zhao et al. 2006; Newberg et al. 2012) and SEGUE (Yanny et al. 2009), together with information coming from high-resolution surveys such as Gaia-ESO (GES, Gilmore et al. 2012); HERMES/GALAH (Zucker…”
• THE MOST METAL-POOR STARS. II. CHEMICAL ABUNDANCES OF 190 METAL-POOR STARS INCLUDING 10 NEW STARS WITH [Fe/H] ⩽ −3.5,, (2012, background): “Further mining of existing data sets (HK, HES, SDSS, etc.) as well as new and upcoming surveys and facilities (e.g., SkyMapper; Keller et al. 2007, LAMOST; Zhao et al. 2006) should increase the numbers of the most metal-poor stars.”
• Coudé-feed stellar spectral library – atmospheric parameters (2010, background): “The latter application is a key step in the analysis of large spectroscopic surveys, such as RAVE (Steinmetz et al. 2006), SDSS/SEGUE, APOGEE and SEGUE-2 (Rockosi et al. 2009), the Guoshoujing Telescope1 survey (Zhao et al. 2006) or GAIA (Perryman et al. 2001).”
• Constraining the Milky Way assembly history with Galactic Archaeology (2016, background): “…to obtaining spectroscopic information for a large number of stars, e.g., RAVE ⋆ Corresponding author: iminchev@aip.de (Steinmetz et al., 2006), SEGUE (Yanny et al., 2009), APOGEE (Majewski et al., 2010), HERMES (Freeman, 2010), Gaia-ESO (Gilmore et al., 2012), and LAMOST (Zhao et al., 2006).”
• THE APOKASC CATALOG: AN ASTEROSEISMIC AND SPECTROSCOPIC JOINT SURVEY OF TARGETS IN THE KEPLER FIELDS (2014, background): “Dong et al. (2013) performed a related exercise comparing LAMOST and KIC metallicities for dwarfs.”
• Multiple populations in globular clusters (2012, background): “…data will be produced by spectroscopic surveys just starting or planned for the immediate future, such as HERMES (Freeman 2011), LAMOST (e.g., Zhao et al. 2006), and the FLAMES public ESO survey (PIs Gilmore and Randich, see http://www.gaia-eso.eu) that will start in 2012 and will target…”