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Table 3

The observational quantities, D, pobs, and fgrad, are listed for each line of Table 2.

HARPS-N observations Hydrodynamical model
Line D a pobs ± σfluor−stat ± σd−stat ± σd−syst b fgrad c phydro d p0 e

Line 1 0.281 ±0.001 1.287 ±0.031±0.014±0.023 0.983 ±0.007 1.307 1.360
Line 2 0.147 ±0.001 1.323 ±0.031±0.014±0.023 0.991 ±0.004 1.328 1.365
Line 3 0.348 ±0.001 1.280 ±0.031±0.014±0.023 0.979 ±0.009 1.304 1.369
Line 4 0.573 ±0.001 1.282 ±0.031±0.014±0.023 0.967 ±0.014 1.292 1.375
Line 5 0.297 ±0.001 1.297 ±0.031±0.014±0.023 0.982 ±0.008 1.309 1.375
Line 6 0.612 ±0.001 1.282 ±0.031±0.014±0.023 0.964 ±0.015 1.288 1.375
Line 7 0.562 ±0.001 1.273 ±0.031±0.014±0.023 0.967 ±0.014 1.272 1.376
Line 8 0.500 ±0.001 1.285 ±0.031±0.014±0.023 0.971 ±0.012 1.297 1.378
Line 9 0.364 ±0.001 1.307 ±0.031±0.014±0.023 0.979 ±0.009 1.302 1.383
Line 10 0.326 ±0.001 1.329 ±0.031±0.014±0.023 0.981 ±0.008 1.301 1.387
Line 11 0.429 ±0.001 1.295 ±0.031±0.014±0.023 0.975 ±0.011 1.304 1.385
Line 12 0.283 ±0.001 1.300 ±0.031±0.014±0.023 0.983 ±0.007 1.312 1.385
Line 13 0.290 ±0.002 1.294 ±0.031±0.014±0.023 0.983 ±0.008 1.304 1.386
Line 14 0.317 ±0.002 1.292 ±0.031±0.014±0.023 0.981 ±0.008 1.310 1.387
Line 15 0.497 ±0.001 1.280 ±0.031±0.014±0.023 0.971 ±0.012 1.290 1.389
Line 16 0.348 ±0.001 1.301 ±0.031±0.014±0.023 0.979 ±0.009 1.301 1.389
Line 17 0.366 ±0.001 1.323 ±0.031±0.014±0.023 0.978 ±0.009 1.297 1.390

Notes. The quantities phydro, p0 and fo−g are derived from hydrodynamical model.

(a)

The line depth D is calculated at minimum radius of the star.

(b)

The observational projection factors pobs is derived from HARPS-N and FLUOR/CHARA interferometric data using the inverse BW approach (Sect. 3.2).

(c)

The fgrad coefficient involved in the projection factor decomposition (p = p0fgradfo−g, Nardetto et al. 2007) is derived from Eqs. 5 and 6 (Sect. 4.2).

(d)

The inverse projection factors phydro is calculated with the hydrodynamical model (Sect. 4.1).

(e)

The modeled geometric projection factor p0 is derived in the continuum next to each spectral line. The fo−g quantity, which is obtained using the projection factor decomposition (), is derived in Sect. 5.

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