Table 1: The collected spectra for each stellar target, giving the corresponding spectrograph, the resolving power, the Julian date (HJD) and signal-to-noise ratio ( S/N) for each observation. The S/N for ÉLODIE spectra is estimated at 5550 Å. Values of $v~\sin{i}$ are from Royer et al. (2002) and given in km s^-1.
Object Sp. type Instrument $\lambda/\Delta \lambda$ HJD S/N $v~\sin{i}$

Altair A7IV/V ÉLODIE 42 000 24 52 914.2574 180 $\sim$ 220

2 452 914.2600 200

2 452 914.2628 280

2 452 914.2655 230

2 452 914.2683 250

HD 27819 A7IV/V ÉLODIE 42 000 2 450 499.4221 180 $\sim$ 40

$\gamma$ Boo A7III/IV FOCES 40 000 2 452 336.0736 300 $\sim$ 130

HD 118623 A7III FOCES 40 000 2 452 332.1416 300 $\sim$ 210

**Table 1:** The collected spectra for each stellar target, giving the corresponding spectrograph, the resolving power, the Julian date (HJD) and signal-to-noise ratio ( *S/N*) for each observation. The *S/N* for ÉLODIE spectra is estimated at 5550 Å. Values of $v~\sin{i}$ are from Royer et al. (2002) and given in km s^-1.
Object	Sp. type	Instrument	$\lambda/\Delta \lambda$	HJD	S/N	$v~\sin{i}$
Altair	A7IV/V	ÉLODIE	42 000	24 52 914.2574	180	$\sim$ 220
				2 452 914.2600	200
				2 452 914.2628	280
				2 452 914.2655	230
				2 452 914.2683	250
HD 27819	A7IV/V	ÉLODIE	42 000	2 450 499.4221	180	$\sim$ 40
$\gamma$ Boo	A7III/IV	FOCES	40 000	2 452 336.0736	300	$\sim$ 130
HD 118623	A7III	FOCES	40 000	2 452 332.1416	300	$\sim$ 210

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