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Table 4

Data used on each star to apply the SPIPS method.

Star RVs BV JHK Diam.

β Dor d, h, i d, l, n, q, u v, x A, C, F
ζ Gem c, f, g, h, j l, g, p, q, s, u, m w B, C
X Sgr j d, l, p, q, u w, z A, C
Y Sgr d, h, j d, l, p, q, u z
W Sgr c, i l, p, q, u, m z A, C
FF Aql e, f, g l, p, r, t, u z E
RT Aur f, g k, l, g, p, r, u j, y
T Vul b, c, g k, l, g, p, r, u, m j, z E
Car a, d, h, i d, l, o, u, n x A, C, D

Notes. We gathered all the best quality radial velocities, photometry in bands BVRI and JHK, and interferometric diameters (Diam.) from the literature.

Reference. (a) Anderson (2014); (b) Barnes et al. (2005); (c) Bersier et al. (1994b); (d) Bersier (2002); (e) Evans et al. (1990); (f) Gorynya et al. (1998); (g) Kiss (1998); (h) Nardetto et al. (2009); (i) Petterson et al. (2005); (j) Storm et al. (2011); (k) Barnes et al. (1997); (l) Berdnikov (2008); (m) Bersier et al. (1994a); (n) Dean et al. (1977); (o) Madore (1975); (p) Moffett & Barnes (1984); (q) Shobbrook (1992); (r) Szabados (1977); (s) Szabados (1981); (t) Szabados (1991); (u) ESA (1997); (v) Lloyd Evans (1980); (w) Feast et al. (2008); (x) Laney & Stobie (1992); (y) Monson & Pierce (2011); (z) Welch et al. (1984); (A) VINCI/VLTI and FLUOR/IOTA data (Kervella et al. 2004b); (B) PTI data (Lane et al. 2002); (C) PIONIER data (present work); (D) SUSI data (Davis et al. 2009); (E) FLUOR/CHARA data (Gallenne et al. 2012); (F) SUSI data (Jacob 2008).

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