On the consistency of magnetic field measurements of Ap stars: lessons learned from the FORS1 archive

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Volume 572 (December 2014)

A&A, 572 (2014) A113

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Table 2

Comparison of ⟨ B_z ⟩ values obtained with different grisms

MJD	Grism	λ range	R	t_int	⟨ B_z ⟩ (G)
		(Å)		(s)	(all lines)

HD 94660
54 181.161	600 B	3470 − 5890	1592	32	−1952 ± 59
54 181.147	1200 B	3800 − 4970	2707	48	−1998 ± 35

52 309.365	600 B	3480 − 5900	1488	39	−2567 ± 63
52 309.375	600 R	5260 − 7420	2175	73	−2905 ± 56

52 383.122	600 B	3480 − 5900	1616	80	−2642 ± 59
52 383.129	600 R	5250 − 7420	2429	160	−3224 ± 76

53 332.361	600 B	3470 − 5880	1640	40	−2552 ± 63
53 332.374	1200 g	4290 − 5470	2971	96	−2576 ± 40

HD 101065
52 383.198	600 B	3480 − 5900	1616	4780	−1469 ± 97
52 383.260	600 R	5250 − 7420	2429	870	−1445 ± 62

HD 137949
52 383.370	600 B	3480 − 5900	1616	1289	2689 ± 70
52 383.408	600 R	5250 − 7420	2429	320	2843 ± 64

HD 188041–42
52 130.176	600 B	3480 − 5900	1763	32	2069 ± 66
52 130.168	600 R	5350 − 7410	2732	40	2312 ± 61

HD 201601
53 976.260	600 B	3470 − 5880	1725	60	−1316 ± 64
53 976.268	1200 B	3800 − 4960	3052	122	−1462 ± 31
52 531.045	600 R	4760 − 6900	2206	330	−1658 ± 53
53 335.011	600 I	6900 − 9050	2956	16	−596 ± 57

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