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Cited article:

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The EBLM Project—From False Positives to Benchmark Stars and Circumbinary Exoplanets

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The first view of δ Scuti and γ Doradus stars with the TESS mission

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T Tauri stars in the SuperWASP and NSVS surveys

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A revisit to the enigmatic variable star 21 Comae

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Gaia-derived luminosities ofKeplerA/F stars and the pulsator fraction across the δ Scuti instability strip

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CAOS spectroscopy of Am stars Kepler targets★

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Fundamental parameters of eight Am stars: comparing observations with theory★

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Absolute dimensions of detached eclipsing binaries – III. The metallic-lined system YZ Cassiopeiae

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THE ROLE OF TURBULENT PRESSURE AS A COHERENT PULSATIONAL DRIVING MECHANISM: THE CASE OF THE δ SCUTI STAR HD 187547

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https://doi.org/10.1088/0004-637X/796/2/118

High-frequency A-type pulsators discovered using SuperWASP★†

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Rapidly varying A-type stars in the SuperWASP archive

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Do the close binaries HD 22128 and HD 56495 contain Ap or Am stars?★

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A photometric study of chemically peculiar stars with the STEREO satellites – II. Non-magnetic chemically peculiar stars★

E. Paunzen, K. T. Wraight, L. Fossati, et al.
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https://doi.org/10.1093/mnras/sts318

Testing different methods for atmospheric parameters determination. The case study of the Am star HD 71297★

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https://doi.org/10.1093/mnras/stt416

Atomic diffusion and observations of pulsating A stars

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Pulsational amplitude growth of the star KIC 3429637 (HD 178875) in the context of Am and ρ Pup stars

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Period decrease in three SuperWASP eclipsing binary candidates near the short-period limit

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https://doi.org/10.1051/0004-6361/201219158