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Table 7.

Overview of UD measurements in the literature.

Star Distance Distance Variability Period Period UD diam. Flux at freq. UD
[pc] Ref. type [days] Ref. [mas] [mJy] [GHz] Ref.
R Dor 55 ± 3 1 SRb 332, 175 5 61.8 221.4 225 1
W Hya 87 9 + 11 $ 87 ^{+11}_{-9} $ 2 Mira 402 VSX 50 a 210 a 240 3
Mira A 100 ± 20 3 Mira 331 VSX 43.3 99.61 229.13 3
R Leo 100 ± 5 2 Mira 312 VSX 41.88 107.83 232.53 3
R Lep 471 64 + 88 $ 471 ^{+88}_{-64} $ 2 Mira 437 VSX 14.2 37.3 405.0 6
CW Leo 123 ± 14 4 Mira 630 VSX 53 b 372 258 c 7

Notes. (a) Values interpolated from higher and lower frequency observations. (b) Parameters given are for a Gaussian fit performed on the data, and hence are not directly comparable to UD fits. (c) Approximate estimates. 1: Vlemmings et al. (2024); 2: Andriantsaralaza et al. (2022); 3: Vlemmings et al. (2019); 4: Groenewegen et al. (2012); 5: Bedding et al. (1998); 6: Asaki et al. (2023); 7: Velilla-Prieto et al. (2023); VSX indicates a period taken directly from the VSX database.

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