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Table 1

Average longitudinal magnetic field values obtained from the FORS 2 and HARPS observations.

FORS 2

Reduction Date HJD No. of Exp. S / N BzV (G) BzN (G) BzV (G) BzN (G)
2 450 000 frames time (s) Hydrogen All

Bonn 07-Feb.-2014 6696.7341 10 35 2359 −655 ± 109 22 ± 81 −504 ± 54 69 ± 46
Potsdam −639 ± 121 −16 ± 119 −460 ± 65 76 ± 66

Bonn 08-Feb.-2014 6697.7162 10 30 2398 −978 ± 88 −36 ± 76 −653 ± 47 40 ± 43
Potsdam −877 ± 91 −102 ± 105 −521 ± 62 23 ± 63

HARPS

Reduction Date HJD No. of Exp. S/N BzV (G) Detection FAP
2 450 000 frames time (s)

Bonn (LSD) −592 ± 7 DD < 10-15
Potsdam (SVD) 23-Apr.-2014 6770.4993 4 2700 347 −583 ± 9 DD < 10-16
Potsdam (MT) −584 ± 15

Notes. Column 1 indicates the group that performed the data reduction and analysis, which led to the results shown in the following columns. The heliocentric Julian date shown in Col. 3 indicates the beginning of the sequence of exposures. Column 4 gives the number of frames obtained during each night of observation and Col. 5 the exposure time of each frame. Column 6 gives the S/N per pixel of Stokes I calculated at about 4950 Å over a wavelength range of 100 Å. In the FORS 2 subtable, Cols. 7 and 8 give the Bz values obtained using the spectral regions covered by the hydrogen lines obtained from the Stokes V and N parameter spectrum, respectively. The same is given in Cols. 9 and 10, but using the full spectrum (see Sect. 3.1). In the HARPS subtable, Cols. 7 and 8 give the BzV values and the detection flag (DD, definite detection). Column 9 gives the false alarm probability (FAP) for those methods that provide it. The different detection techniques are listed in Col. 1 (see Sect. 3.2).

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