Single peaked CO emission line profiles from the inner regions of protoplanetary disks

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Volume 527 (March 2011)

A&A, 527 (2011) A119

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Table 2

Journal of observations.

Source	Obs. time	Settings (μm)^a	Standard star	Spectral type
				standard star

AS 205 A	Apr. 07	4.760, 4.662, 4.676, 4.773	BS 4757	A0
	Aug. 07	4.730	BS 5812	B2.5
	Apr. 08	4.730	BS 6084	B1
	Aug. 09	5100, 5115	BS 5984	B0.5
DR Tau	Oct. 07	4.716, 4.730, 4.833, 4.868	BS 3117, BS 838	B3, B8
	Dec. 08	4.716, 4.946	BS 1791	B7
RU Lup	Apr. 07	4.716, 4.730, 4.833, 4.929	BS 5883	B9
	Apr. 08	4.730	BS 6084	B1
S CrA	Apr. 07	4.730, 4.716	BS 6084	B1
	Aug. 07	4.730	BS 7235, BS 7920	A0, A9
	Aug. 08	4.868, 4.946	BS 6084, BS 7236	B1, B9
VV CrA A	Apr. 07	4.716, 4.730, 4.840	BS 7362	A4
	Aug. 07	4.770, 4.779	BS 7236	B9
	Aug. 08	4.946	BS 7236	B9
VW Cha	Dec. 08	4.716, 4.800, 4.820, 4.946	BS 5571, HR 4467	B2, B9
VZ Cha	Dec. 08	4.716, 4.800, 4.820, 4.946	BS 5571, HR 4467	B2, B9

^(a)

The reference wavelength of a given setting is centered on the third detector.

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