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Cited article:

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How Magnetic Activity Alters What We Learn from Stellar Spectra

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The Astrophysical Journal 895 (1) 52 (2020)
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Velocity Field Diagnostics of the Quiet Sun Using the Lambda-Meter Method: Si I 1082.7 nm Line

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Kinematics and Physics of Celestial Bodies 36 (1) 1 (2020)
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Diagnostics of the velocity field of the quiet Sun using the lambda-meter method: The Si I  1082.7 nm line

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Kinematika i fizika nebesnyh tel (Online) 36 (1) 3 (2020)
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The diagnostic potential of the weak field approximation for investigating the quiet Sun magnetism: the Si I 10 827 Å line

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The effect of stellar activity on the spectroscopic stellar parameters of the young solar twin HIP 36515

Jhon Yana Galarza, Jorge Meléndez, Diego Lorenzo-Oliveira, Adriana Valio, Henrique Reggiani, Marília Carlos, Geisa Ponte, Lorenzo Spina, Raphaëlle D Haywood and Davide Gandolfi
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High-precision stellar abundances of the elements: methods and applications

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Non-LTE line formation of Fe in late-type stars – IV. Modelling of the solar centre-to-limb variation in 3D

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The metal-rich abundance pattern – spectroscopic properties and abundances for 107 main-sequence stars

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A Si I atomic model for NLTE spectropolarimetric diagnostics of the 10 827 Å line

N. G. Shchukina, A. V. Sukhorukov and J. Trujillo Bueno
Astronomy & Astrophysics 603 A98 (2017)
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Impact of surface dynamo magnetic fields on the solar abundance of the CNO elements

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Astronomy & Astrophysics 586 A145 (2016)
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