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Home All issues A&A, 386 1 (2002) 286-295 Article references

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Cited article:

Investigating the Temperature Sensitivity of UV Line Ratios in the 280 nm Region of Solar-like Stars

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The Astrophysical Journal 982 (2) 198 (2025)
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Stellar surface information from the Ca ii H&K lines – I. Intensity profiles of the solar activity components

M Cretignier, A G M Pietrow and S Aigrain
Monthly Notices of the Royal Astronomical Society 527 (2) 2940 (2023)
https://doi.org/10.1093/mnras/stad3292

Effective temperatures of classical Cepheids from line-depth ratios in the H-band

V Kovtyukh, B Lemasle, N Nardetto, G Bono, R da Silva, N Matsunaga, A Yushchenko, K Fukue and E K Grebel
Monthly Notices of the Royal Astronomical Society 523 (4) 5047 (2023)
https://doi.org/10.1093/mnras/stad1708

Stellar parameters of early-M dwarfs from ratios of spectral features at optical wavelengths

J. Maldonado, L. Affer, G. Micela, et al.
Astronomy & Astrophysics 577 A132 (2015)
https://doi.org/10.1051/0004-6361/201525797

Velocity and Temperature Response Functions of 77 Near-Infrared (800 – 1400 nm) Photospheric Lines – I

V. Penza and F. Berrilli
Solar Physics 277 (2) 227 (2012)
https://doi.org/10.1007/s11207-011-9916-1

An absolutely calibratedTeffscale from the infrared flux method

L. Casagrande, I. Ramírez, J. Meléndez, M. Bessell and M. Asplund
Astronomy and Astrophysics 512 A54 (2010)
https://doi.org/10.1051/0004-6361/200913204

Improving Stellar and Planetary Parameters of Transiting Planet Systems: The Case of TrES‐2

Alessandro Sozzetti, Guillermo Torres, David Charbonneau, et al.
The Astrophysical Journal 664 (2) 1190 (2007)
https://doi.org/10.1086/519214

Determinations of high-precision effective temperatures for giants based on spectroscopic criteria

V. V. Kovtyukh, T. V. Mishenina, T. I. Gorbaneva, et al.
Astronomy Reports 50 (2) 134 (2006)
https://doi.org/10.1134/S1063772906020065

Variations of total solar irradiance produced by structural changes of the solar interior

Sabatino Sofia
Eos, Transactions American Geophysical Union 85 (22) 217 (2004)
https://doi.org/10.1029/2004EO220001

The sensitivity of the C I 538.0 nm Fe I 537.9 nm and Ti II 538.1 nm lines to solar active regions

V. Penza, B. Caccin † and D. Del Moro
Astronomy & Astrophysics 427 (1) 345 (2004)
https://doi.org/10.1051/0004-6361:20041151

Global Parameter and Helioseismic Tests of Solar Variability Models

L. H. Li, S. Basu, S. Sofia, et al.
The Astrophysical Journal 591 (2) 1267 (2003)
https://doi.org/10.1086/375484

High precision effective temperatures for 181 F–K dwarfs from line-depth ratios

V. V. Kovtyukh, C. Soubiran, S. I. Belik and N. I. Gorlova
Astronomy & Astrophysics 411 (3) 559 (2003)
https://doi.org/10.1051/0004-6361:20031378