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MyGIsFOS: an automated code for parameter determination and detailed abundance analysis in cool stars

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Astronomy & Astrophysics 564 A109 (2014)
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Effective temperatures of solar type stars

I. N. Glushneva, V. I. Shenavrin and I. A. Roshchina
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Implications of a New Temperature Scale for Halo Dwarfs on LiBeB and Chemical Evolution

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Characterizing Kepler asteroseismic targets★

J. Molenda-Żakowicz, D. W. Latham, G. Catanzaro, A. Frasca and S. N. Quinn
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The puzzling abundance pattern of HD 134439 and HD 134440★

Y. Q. Chen and G. Zhao
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Beryllium in Disk and Halo Stars: Evidence for a Beryllium Dispersion in Old Stars

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Generation of a Near Infra-Red Guide Star Catalog for Thirty-Meter Telescope Observations

Smitha Subramanian, Annapurni Subramaniam, Luc Simard, et al.
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C. Liu, G. Ruchti, S. Feltzing, et al.
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Cosmic Ray Production of Beryllium and Boron at High Redshift

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The Astrophysical Journal 673 (2) 676 (2008)
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Benchmark stars forGaiaFundamental properties of the Population II star HD 140283 from interferometric, spectroscopic, and photometric data

O. L. Creevey, F. Thévenin, P. Berio, et al.
Astronomy & Astrophysics 575 A26 (2015)
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AN EXAMINATION OF RECENT TRANSFORMATIONS TO THEBV(RI)CPHOTOMETRIC SYSTEM FROM THE PERSPECTIVE OF STELLAR MODELS FOR OLD STARS

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The Astronomical Journal 140 (4) 1020 (2010)
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TMCalc – a fast code to derive Teff and [Fe/H] for FGK stars

S. G. Sousa, N. C. Santos and G. Israelian
Astronomy & Astrophysics 544 A122 (2012)
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Angular Diameters of the G Subdwarf μ Cassiopeiae A and the K Dwarfs σ Draconis and HR 511 from Interferometric Measurements with the CHARA Array

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The ability of intermediate-band Strömgren photometry to correctly identify dwarf, subgiant, and giant stars and provide stellar metallicities and surface gravities

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Confronting the Gaia and NLTE spectroscopic parallaxes for the FGK stars

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Influence of Inelastic Collisions with Hydrogen Atoms on Non-LTE Oxygen Abundance Determinations

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Observational constraints on potassium synthesis during the formation of stars of the Galactic disk

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Astronomy Reports 47 (9) 750 (2003)
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The atmospheric lithium abundances of solar analogues

A. I. Galeev, I. F. Bikmaev, L. I. Mashonkina, F. A. Musaev and G. A. Galazutdinov
Astronomy Reports 48 (6) 511 (2004)
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Sulfur Abundances in Metal-Poor Stars Based on OAO-1.88 m/HIDES Spectra

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Publications of the Astronomical Society of Japan 57 (2) 347 (2005)
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The Top Ten solar analogs in the ELODIE library

C. Soubiran and A. Triaud
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Li in NGC 6752 and the formation of globular clusters

L. Pasquini, P. Bonifacio, P. Molaro, et al.
Astronomy & Astrophysics 441 (2) 549 (2005)
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Detailed chemical composition of the open cluster IC 4651: The iron peak, $\mathsf{\alpha}$ elements, and Li

L. Pasquini, S. Randich, M. Zoccali, et al.
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IRFM T$_{\sf\sl eff}$ calibrations for cluster and field giants in the Vilnius, Geneva, RI$_{\sf\sl (C)}$ and DDO photometric systems

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DOI: 10.1051/0004-6361:20031764
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Na, Mg and Al abundances as a population discriminant for nearby metal-poor stars

T. Gehren, J. R. Shi, H. W. Zhang, G. Zhao and A. J. Korn
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Effective temperature scale and bolometric corrections from 2MASS photometry

E. Masana, C. Jordi and I. Ribas
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Basic physical parameters of a selected sample of evolved stars

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MAFAGS-OS: New opacity sampling model atmospheres for A, F and G stars

F. Grupp
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Chemical abundances of 10 metal-poor halo stars

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Spectral line ratios as ${\vec T}_{\bf \sf eff}$ indicators in solar-like stars

B. Caccin, V. Penza and M. T. Gomez
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Elemental abundance analyses with DAO spectrograms

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Analysis of neutron capture elements in metal-poor stars

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Non-LTE line formation for heavy elements in four very metal-poor stars

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Luciana Pompeia, Beatriz Barbuy and Michel Grenon
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Lithium Isotope Ratios in Halo Stars. II.

L. M. Hobbs and J. A. Thorburn
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Evolutionary Stellar Population Synthesis at 2 A Spectral Resolution

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Precise Spectropolarimetric Measurements of Magnetic Fields on Some Solar‐like Stars

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Boron in Very Metal‐poor Stars

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Rubidium in Metal‐deficient Disk and Halo Stars

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The Revival of Galactic Cosmic‐Ray Nucleosynthesis?

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Model Photospheres for Late‐Type Stars from the Inversion of High‐Resolution Spectroscopic Observations: Groombridge 1830 and ε Eridani

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The Astrophysical Journal 528 (2) 885 (2000)
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Primordial Lithium Abundance as a Stringent Constraint on the Baryonic Content of the Universe

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The Astrophysical Journal 540 (1) 99 (2000)
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Abundances in the Metal‐poor Common Proper Motion Star BD +00°2058A

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Publications of the Astronomical Society of the Pacific 111 (761) 817 (1999)
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Models of Metal‐poor Stars with Gravitational Settling and Radiative Accelerations. II. The Age of the Oldest Stars

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Rapid Rotation of Ultra–Li‐depleted Halo Stars and Their Association with Blue Stragglers

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A Search for Cool Subdwarfs: Stellar Parameters for 134 Candidates

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The Distances to Open Clusters as Derived from Main‐Sequence Fitting. II. Construction of Empirically Calibrated Isochrones

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The Astrophysical Journal 600 (2) 946 (2004)
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Boron Benchmarks for the Galactic Disk

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The Astrophysical Journal 606 (1) 306 (2004)
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The Rise of thes‐Process in the Galaxy

Jennifer Simmerer, Christopher Sneden, John J. Cowan, et al.
The Astrophysical Journal 617 (2) 1091 (2004)
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Beryllium in the Ultra-Lithium-deficient, Metal-Poor Halo Dwarf G186-26

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The Astrophysical Journal 633 (2) L125 (2005)
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The Gaia-ESO survey: 3D NLTE abundances in the open cluster NGC 2420 suggest atomic diffusion and turbulent mixing are at the origin of chemical abundance variations

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Astronomy & Astrophysics 643 A164 (2020)
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Lithium abundances of halo dwarfs based on excitation temperatures

A. Hosford, A. E. García Pérez, R. Collet, et al.
Astronomy and Astrophysics 511 A47 (2010)
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A new benchmark T8-9 brown dwarf and a couple of new mid-T dwarfs from the UKIDSS DR5+ LAS★

B. Goldman, S. Marsat, T. Henning, C. Clemens and J. Greiner
Monthly Notices of the Royal Astronomical Society no (2010)
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Revisiting ΔY/ΔZ from multiple main sequences in globular clusters: insight from nearby stars

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Monthly Notices of the Royal Astronomical Society no (2010)
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Chromium: NLTE abundances in metal-poor stars and nucleosynthesis in the Galaxy

M. Bergemann and G. Cescutti
Astronomy & Astrophysics 522 A9 (2010)
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The helium abundance and ΔY/ΔZ in lower main-sequence stars

Luca Casagrande, Chris Flynn, Laura Portinari, Leo Girardi and Raul Jimenez
Monthly Notices of the Royal Astronomical Society 382 (4) 1516 (2007)
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Primordial Nuclei and Their Galactic Evolution

F. Spite, M. Spite and V. Hill
Space Sciences Series of ISSI, Primordial Nuclei and Their Galactic Evolution 4 155 (1998)
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Fundamental Stellar Properties: The Interaction Between Observation and Theory

Michael S. Bessell
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LITHIUM AND PROTON-CAPTURE ELEMENTS IN GLOBULAR CLUSTER DWARFS: THE CASE OF 47 TUC

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The Astrophysical Journal 713 (1) L1 (2010)
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EXTREME ENHANCEMENTS OF r -PROCESS ELEMENTS IN THE COOL METAL-POOR MAIN-SEQUENCE STAR SDSS J2357–0052

Wako Aoki, Timothy C. Beers, Satoshi Honda and Daniela Carollo
The Astrophysical Journal 723 (2) L201 (2010)
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A Catalog of 10,000 Very Metal-poor Stars from LAMOST DR3

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The Astrophysical Journal Supplement Series 238 (2) 16 (2018)
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A Planet Orbiting the Star ρ Coronae Borealis

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The Astrophysical Journal 483 (2) L111 (1997)
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Detection of the L[CLC]i[/CLC] [CSC]i[/CSC] λ6104 Transition in the Population II Star HD 140283

Piercarlo Bonifacio and Paolo Molaro
The Astrophysical Journal 500 (2) L175 (1998)
DOI: 10.1086/311408
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Primordial Lithium and Big Bang Nucleosynthesis

Sean G. Ryan, Timothy C. Beers, Keith A. Olive, Brian D. Fields and John E. Norris
The Astrophysical Journal 530 (2) L57 (2000)
DOI: 10.1086/312492
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Reappraising the Spite Lithium Plateau: Extremely Thin and Marginally Consistent with WMAP Data

Jorge Meléndez and Iván Ramírez
The Astrophysical Journal 615 (1) L33 (2004)
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Abundances and kinematics of carbon-enhanced metal-poor stars in the Galactic halo

C. J. Hansen, T. T. Hansen, A. Koch, et al.
Astronomy & Astrophysics 623 A128 (2019)
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An empirical metallicity tracer in CEMP and C-normal stars

D. Singh, C. J. Hansen, J. S. Byrgesen, M. Reichert and H. M. Reggiani
Astronomy & Astrophysics 634 A72 (2020)
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