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Table 2.

TESS sectors and cadence at which the sample of studied eclipsing binary systems have been observed, the time-span between the first and last eclipse included in this work, and their GaiaG magnitudes.

System Sector Cad. Δt G
[min] [d] [mag]
KX Cnc 21 2 20 7.0363(2)
AL Dor 1–6, 8–13, 27–29 2 783 7.5820(3)
RW Lac 16, 17 2 47 10.4381(3)
V530 Ori 6 30 18 9.6959(4)
HP Dra 14, 15, 26 2 344 7.8117(4)
TZ Men 12, 13, 27 2 428 6.1556(8)
V541 Cyg 14 2 22 10.3286(4)
LV Her 25, 26 2 34 10.8853(6)
V459 Cas 18, 24 2 186 10.2905(3)
RR Lyn 20 2 20 5.4696(14)
V501 Her 25, 26 2 47 10.9787(6)
KW Hya 8 2 20 6.0529(7)
V501 Mon 6 30 17 12.1884(2)
GG Ori 6 2 16 10.2372(5)
EY Cep 19, 25 2 186 9.7154(3)

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