Oxygen lines in solar granulation - I. Testing 3D models against new observations with high spatial and spectral resolution

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Table 1:

Observing runs selected for analysis.
UT date	$\mu$	Coordinates	$\Delta I_{\rm {rms}}$ [%]
20/5/2007 08:00	$0.999 \pm 0.001$	0.2S, 0.5E	9.2
25/5/2007 08:30	$0.816 \pm 0.010$	26.7N, 22.1E	5.4
27/5/2007 15:30	$0.793 \pm 0.012$	1.3N, 37.5W	6.0
25/5/2007 09:56	$0.608 \pm 0.020$	51.1S, 3.7E	4.7
20/5/2007 09:27	$0.424 \pm 0.024$	29.9S, 61.4W	5.2
25/5/2007 07:40	$0.197 \pm 0.003$	18.0S, 82.4E	3.4

Coordinates are given in the Heliographic Stonyhurst system. The spread in $\mu$ is given by the approximate spatial coverage of the slit. The $\Delta I_{\rm {rms}}$ is given as the maximum continuum contrast of a single frame in the 615 nm wavelength region.

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