Table 6: The five spectroscopic binaries (SBs) and their orbital elements. Columns for the first part of the table (literature data): (1) HD number; (2) periastron date T₀ (HJD); (3) period P (days); (4) primary orbital semi-amplitude K₁ (km s^-1); (5) secondary orbital semi-amplitude K₂ (km s^-1; only for double-lined spectroscopic binaries, i.e., SB2s); (6) systemic velocity $\gamma$ (km s^-1); (7) orbital eccentricity $\epsilon$ (see the footnote to the table for literature sources). Columns for the second part of the table (data from this study): (1) HD number; (2) exposure number (Table 3); (3) instantaneous radial velocity (km s^-1); (4) primary component prediction using the ephemeris provided above (km s^-1); (5) secondary component prediction using the ephemeris provided above (km s^-1; only for SB2s).
HD T₀ [HJD] P [days] K₁ [km s^-1] K₂ [km s^-1] $\gamma$ [km s^-1] $\epsilon$

(1) (2) (3) (4) (5) (6) (7)

23180 $2445338.267\phantom{0} \pm 0.005$ $\phantom{0}4.4191447 \pm 0.0000082$ $111.8 \pm 1.4$ $155.0 \pm 2.4$ $+12.2 \pm 0.5$ 0

23625 $2400000.0\phantom{000} \pm 0.005$ $\phantom{0}1.940564\phantom{0} \pm 0.000004\phantom{0}$ $\phantom{0}82.0 \pm 2.0$ $114.0 \pm 3.0$ $+20.0 \pm 1.0$ 0

24190 $2435401.00\phantom{00} \pm 0.01\phantom{0}$ $26.111\phantom{0000} \pm 0.001\phantom{0000}$ $\phantom{0}13.0 \pm 1.0$ - $+26.7 \pm 1.0$ $0.08\phantom{0} \pm 0.01\phantom{0}$

25799 $2435152.835\phantom{0} \pm 0.013$ $\phantom{0}0.9121679 \pm 0.0000019$ $\phantom{0}17.6 \pm 1.2$ - $+24.3 \pm 0.8$ 0

25833 $2424946.5150 \phantom{ \pm 0.0000}$ $\phantom{0}2.0287298 \phantom{ \pm 0.0000000~~}$ $162.8 \pm 1.1$ $178.7 \pm 1.2$ $+24.7 \pm 0.9$ $0.071 \pm 0.001$

**Table 6:** The five spectroscopic binaries (SBs) and their orbital elements. Columns for the first part of the table (literature data): (1) HD number; (2) periastron date T₀ (HJD); (3) period P (days); (4) primary orbital semi-amplitude K₁ (km s^-1); (5) secondary orbital semi-amplitude K₂ (km s^-1; only for double-lined spectroscopic binaries, i.e., SB2s); (6) systemic velocity $\gamma$ (km s^-1); (7) orbital eccentricity $\epsilon$ (see the footnote to the table for literature sources). Columns for the second part of the table (data from this study): (1) HD number; (2) exposure number (Table 3); (3) instantaneous radial velocity (km s^-1); (4) primary component prediction using the ephemeris provided above (km s^-1); (5) secondary component prediction using the ephemeris provided above (km s^-1; only for SB2s).
HD	T₀ [HJD]	P [days]	K₁ [km s^-1]	K₂ [km s^-1]	$\gamma$ [km s^-1]	$\epsilon$
(1)	(2)	(3)	(4)	(5)	(6)	(7)
23180	$2445338.267\phantom{0} \pm 0.005$	$\phantom{0}4.4191447 \pm 0.0000082$	$111.8 \pm 1.4$	$155.0 \pm 2.4$	$+12.2 \pm 0.5$	0
23625	$2400000.0\phantom{000} \pm 0.005$	$\phantom{0}1.940564\phantom{0} \pm 0.000004\phantom{0}$	$\phantom{0}82.0 \pm 2.0$	$114.0 \pm 3.0$	$+20.0 \pm 1.0$	0
24190	$2435401.00\phantom{00} \pm 0.01\phantom{0}$	$26.111\phantom{0000} \pm 0.001\phantom{0000}$	$\phantom{0}13.0 \pm 1.0$	-	$+26.7 \pm 1.0$	$0.08\phantom{0} \pm 0.01\phantom{0}$
25799	$2435152.835\phantom{0} \pm 0.013$	$\phantom{0}0.9121679 \pm 0.0000019$	$\phantom{0}17.6 \pm 1.2$	-	$+24.3 \pm 0.8$	0
25833	$2424946.5150 \phantom{ \pm 0.0000}$	$\phantom{0}2.0287298 \phantom{ \pm 0.0000000~~}$	$162.8 \pm 1.1$	$178.7 \pm 1.2$	$+24.7 \pm 0.9$	$0.071 \pm 0.001$

HD 23180: Stickland & Lloyd (1998);
HD 23625: Blaauw & van Hoof (1963);
HD 24190: Lucy & Sweeney (1971);
HD 25799: Morris et al. (1988); this is a non-radial pulsator;
HD 25833: Giménez & Clausen (1994) (cf. Popper 1974).

HD Exposure $v_{\rm rad}$ [km s^-1] $v_{\rm rad,1}$ [km s^-1] $v_{\rm rad,2}$ [km s^-1]

(1) (2) (3) (4) (5)

23180 1* $-6.1 \pm 3.3$ $\phantom{\sim 0}-28.0 \pm \phantom{0}1.8$ $67.9 \pm \phantom{0}2.5$

2 $6.4 \pm 3.1$ $\phantom{\sim 0}-21.6 \pm \phantom{0}1.8$ $59.0 \pm \phantom{0}2.5$

3 $80.2 \pm 4.2$ $\phantom{\sim}108.7 \pm \phantom{0}1.6$ $-121.6 \pm \phantom{0}2.5$

23625 1 $1.7 \pm 3.0$ $\phantom{\sim 0}-34.7 \pm 19.1$ $96.1 \pm 26.5$

24190 1 $21.3 \pm 4.6$ $\phantom{\sim 0}20.6 \pm \phantom{0}1.9$ -

2* $22.2 \pm 4.6$ $\phantom{\sim 0}20.5 \pm \phantom{0}1.9$ -

25799 1 $38.3 \pm 4.0$ $\phantom{\sim 0}40.3 \pm \phantom{0}2.1$ -

2 $38.4 \pm 3.9$ $\phantom{\sim 0}41.2 \pm \phantom{0}1.7$ -

25833 1* $31.6 \pm 1.2$ $\sim$ $190 \phantom{ \pm 00.00~~~~~}$ $\sim$ $-150 \phantom{ \pm 00.00~~~~~}$

HD	Exposure	$v_{\rm rad}$ [km s^-1]	$v_{\rm rad,1}$ [km s^-1]	$v_{\rm rad,2}$ [km s^-1]
(1)	(2)	(3)	(4)	(5)
23180	1*	$-6.1 \pm 3.3$	$\phantom{\sim 0}-28.0 \pm \phantom{0}1.8$	$67.9 \pm \phantom{0}2.5$
	2	$6.4 \pm 3.1$	$\phantom{\sim 0}-21.6 \pm \phantom{0}1.8$	$59.0 \pm \phantom{0}2.5$
	3	$80.2 \pm 4.2$	$\phantom{\sim}108.7 \pm \phantom{0}1.6$	$-121.6 \pm \phantom{0}2.5$
23625	1	$1.7 \pm 3.0$	$\phantom{\sim 0}-34.7 \pm 19.1$	$96.1 \pm 26.5$
24190	1	$21.3 \pm 4.6$	$\phantom{\sim 0}20.6 \pm \phantom{0}1.9$	-
	2*	$22.2 \pm 4.6$	$\phantom{\sim 0}20.5 \pm \phantom{0}1.9$	-
25799	1	$38.3 \pm 4.0$	$\phantom{\sim 0}40.3 \pm \phantom{0}2.1$	-
	2	$38.4 \pm 3.9$	$\phantom{\sim 0}41.2 \pm \phantom{0}1.7$	-
25833	1*	$31.6 \pm 1.2$	$\sim$ $190 \phantom{ \pm 00.00~~~~~}$	$\sim$ $-150 \phantom{ \pm 00.00~~~~~}$