Magnetic field and atmospheric chemical abundances of the magnetic Ap star HD 318107

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Volume 535 (November 2011)

A&A, 535 (2011) A25

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Table 1

The new spectroscopic and polarimetric data used in our analysis.

Instrument	HJD	Phase	SNR	⟨ B_z ⟩	⟨ B ⟩ (G)			Window	RV
				(G)	Fe ii λ6149	Nd iii λ5050	Nd iii λ6145	(Å)	(km s^-1)

ESPaDOnS	2 454 553.119	0.991	250	4900 ± 45	13 900 ± 380	12 600 ± 340	12 400 ± 280	3690–10 481	−9
ESPaDOnS	2 454 553.150	0.995	250	4856 ± 42				3690–10 481	−9
ESPaDOnS	2454 652.793	0.258	320	1985 ± 31	15 400 ± 380	16 300 ± 340	16 800 ± 280	3690–10 481	−9
HARPS	2 453 463.898	0.803	80		13 600 ± 420	14 900 ± 410	15 100 ± 420	3783–6914	−9
HARPS	2 453 582.645	0.034	90		13 600 ± 500	11 900 ± 680	12 000 ± 670	3783–6914	−9
HARPS	2 453 583.693	0.142	40		13 900 ± 420	14 100 ± 550	14 200 ± 570	3783–6914	−9
HARPS	2 454 223.642	0.056	70		13 200 ± 310	12 300 ± 510	13 000 ± 410	3783–6914	−9
HARPS	2 454 633.613	0.283	55		14 700 ± 250	16 400 ± 410	16 400 ± 340	3783–6914	−8
HARPS	2 454 869.850	0.615	70		13 800 ± 420	15 700 ± 680	15 300 ± 570	3783–6914	−8
HARPS	2 454 870.879	0.721	60		13 600 ± 420	14 700 ± 680	15 900 ± 570	3783–6914	−8
UVES	2 451 692.894	0.390	220		15 900 ± 210	17 000 ± 280	16 400 ± 380	4795-6745
FLAMES–UVES	2 454 256.625	0.453	150		16 500 ± 340	16 400 ± 510	16 900 ± 420	4200-6200	−8

Notes. Recorded are the HJD and derived phases for each spectra. The values of ⟨ B_z ⟩ for the ESPaDOnS spectra are shown followed by ⟨ B ⟩ values for all spectra measured from three spectral lines: Fe ii λ6149, Nd iii λ5050 and λ6145.

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