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Table 1

Log of the spectroscopic (and polarimetric) observations of Vega.

Date JDfirst JDlast N spec texp (s) tcov (h) S/N
(1) (2) (3) (4) (5) (6) (7)

Jul. 26 2008 4674.3489 4674.6072 389 6 6.2 812  ±  50
Jul. 27 2008 4675.3748 4675.6551 390 6 6.7 822  ±  61
Jul. 29 2008 4677.3480 4677.6415 434 6 7.0 823  ±  82

Sep. 9 2009 5083.7400 5083.9066 402 4 4.0 865  ±  85
Sep. 10 2009 5084.7111 5084.8787 331 4 4.0 887  ±  69
Sep. 11 2009 5085.7122 5085.9498 560 4 5.7 736  ±  155

Jul. 15 2010 5393.3643 5393.5735 355 13 5.0 1117  ±  37
Jul. 16 2010 5394.3635 5394.6576 496 13 7.1 1051  ±  158
Jul. 17 2010 5395.3650 5395.6510 453 13 6.9 1197  ±  59
Jul. 18 2010 5396.3580 5396.4662 185 13 2.6 1222  ±  16
Jul. 19 2010 5397.3561 5397.6569 483 13 7.2 1170  ±  70

Notes. (1) Date of the observation (UT) (Petit et al. (2010) indicates the date in local time, leading to a −1 day shift for the Sept. 2009 CFHT data). (2) and (3) heliocentric Julian date (mean observation, 2 450 000+) of the first and the last stellar spectrum of the night, respectively; (4) number of high resolution RS Cha spectra; (5) exposure time (s); (6) total hours covered on the sky; (7) nightly average and standard deviation of signal to noise per resolved element at 520 nm.

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