Open Access

Table E.5

Comparison between stars of Tucana IV in our sample and Simon et al. (2020).

star ID RA DEC vrad
[km s−1]
evrad
[km s−1]
vrad,Simon [km s−1] evrad,Simon [km s−1] Our member Member for Simon [Fe/H] σ[Fe/H] [Fe/H]Simon σ[Fe/H],Simon
3 0.71819 −60.73536 164.4 2.1 162.0 0.70 × ×
5 0.79783 −60.74766 16.6 0.2 14.7 1.1 −1.38 0.07
6* 0.60930 −60.77164 5.6 2.1
7 0.71638 −60.80579 13.5 0.7 9.8 1.5 −2.75 0.17 −2.59 0.30
8 0.73765 −60.86140 16.9 1.4 16.5 2.2 −2.09 0.25 −2.20 0.32
9 0.43461 −60.83191 29.3 1.3 31.7 7.3 Δ × −1.28 0.24
10* 0.76487 −60.84038 19.6 1.0 18.3 2.5
11* 0.61753 −60.80400 14.0 1.3 13.5 3.3
12* 0.93365 −60.80132 20.5 1.5 21.1 2.8
13 0.75174 −60.86246 −203.8 1.8 −205.4 5.2 × ×
15 0.81263 −60.99411 143.3 1.1 ×
16 0.81460 −60.74894 −18.1 1.7 −19.3 2.6 Δ × −2.46 0.29
17 0.58846 −60.97393 59.3 1.7 Δ −2.32 0.29
22 1.03213 −60.74080 60.3 1.7 Δ −1.86 0.30
23 1.05756 −60.80160 125.3 1.9 ×
113 0.49597 −60.74761 43.5 0.4 Δ −1.48 0.11
125* 0.84454 −60.77233 −40.0 2.5 Δ

Notes. The "*" symbol identifies the HB stars. The Δ represents the "unlikely member" stars.

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