Notes. See text for description, and table notes for references. An asterisk indicates indirect determinations of θ_LD and F_bol values determined from calibrations. The column headed “Band” indicates the wavelength band of the interferometric observations – “opt” for several optical wavelengths, H for several wavelengths from 1.5 to 1.8 μm, K or K′ for K-band (about 2 μm), or wavelength in nm.

Reference. For θ_LD: B06 ... Bigot et al. (2006); B11 ... Bigot et al. (2011); Ba ... Bazot et al. (2011); Bo08 ... Boyajian et al. (2008); C12 ... Creevey et al. (2012); C15 ... Creevey et al. (2015); C99 ... Cohen et al. (1999); Ch ... Chiavassa et al. (2012); D ... di Folco et al. (2007); K ... Kervella et al. (2003b); K08 ... Kervella et al. (2008); K04 ... indirect, using surface-brightness relations by Kervella et al. (2004a); M ... Mozurkewich et al. (2003); L ... Lacour et al. (2008, τ_Ross = 1; N07 ... North et al. (2007); N09 ... North et al. (2009); RR ... Richichi & Roccatagliata (2005); T ... Thévenin et al. (2005); Tp ... Thévenin et al., in prep., VLTI/AMBER measurement for β Ara, CHARA/VEGA for HD 220009; vB ... van Belle et al. (2007); W2/W3/W4 ... Wittkowski et al. (2004, 2006b,a, τ_Ross = 1. Additional references for F_bol: A ... Aufdenberg et al. (2005); A95 ... Alonso et al. (1995) calibration for dwarf stars; A96 ... Alonso et al. (1996a, their Table 4); B98 ... Blackwell & Lynas-Gray (1998), uncertainties of 1.1% for dwarfs and 2.6% for giants and subgiants following di Benedetto (1998, Sect. 3.2, p. 863); Bo13 ... Boyajian et al. (2013), G ... Griffin & Lynas-Gray (1999), uncertainty of 2.6% from Koch & McWilliam (2008); H ... from the V magnitude and the bolometric correction BC_V derived from the calibration of Alonso et al. (1999b); M13 ... Mann et al. (2013).