Calibrating the surface brightness – color relation for late-type red giants stars in the visible domain using VEGA/CHARA interferometric observations

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Volume 639 (July 2020)

A&A, 639 (2020) A67

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Table B.1

Observing log.

	Date	RJD	HA	λ_min	λ_max	Baseline	Bp	PA
	[yyyy.mm.dd]	[days]	[h]	[nm]	[nm]		[m]	[deg]
HD 11037	2013.10.27	56 592.686	−2.60	705	725	E2W2	144.95	−111.33	0.160_{±0.027±0.003}
	2013.10.27	56 592.686	−2.60	725	740	E2W2	144.95	−111.33	0.146_{±0.016±0.002}
	2014.10.19	56 949.773	−1.03	695	715	W1W2	97.74	−83.73	0.274_{±0.095±0.002}
	2014.10.19	56 949.793	−0.57	695	715	W1W2	102.47	−84.45	0.372_{±0.058±0.003}

HD 13468	2014.08.27	56 896.906	−1.66	690	710	E1E2	65.85	−115.41	0.632_{±0.027±0.003}
	2014.08.27	56 896.906	−1.66	690	710	E2W2	155.13	−111.55	0.099_{±0.050±0.003}
	2014.08.27	56 896.945	−0.65	690	710	E1E2	64.31	−115.57	0.647_{±0.041±0.003}
	2013.11.02	56 598.777	−0.51	705	725	W1W2	102.72	93.72	0.389_{±0.021±0.004}
	2013.11.02	56 598.777	−0.51	705	725	W2E2	154.24	68.88	0.055_{±0.033±0.001}
	2013.11.02	56 598.777	−0.51	725	740	W1W2	102.72	93.72	0.419_{±0.019±0.004}
	2013.11.02	56 598.777	−0.51	725	740	W2E2	154.24	68.88	0.157_{±0.029±0.004}

HD 22798	2014.08.22	56 892.002	−1.24	690	710	E2W2	156.25	−111.20	0.120_{±0.014±0.002}
	2014.10.20	56 950.816	−1.83	695	715	W2S2	130.75	−5.76	0.353_{±0.037±0.004}
	2014.10.20	56 950.853	−0.91	695	715	W2S2	136.30	−16.83	0.287_{±0.023±0.004}
	2014.10.20	56 950.890	−0.06	695	715	W2S2	145.01	−25.27	0.171_{±0.071±0.002}

HD 23526	2014.08.22	56 891.974	−1.96	680	700	E2W2	151.53	−110.15	0.045_{±0.050±0.001}
	2014.08.22	56 891.974	−1.96	700	720	E2W2	151.53	−110.15	0.053_{±0.050±0.001}
	2014.08.23	56 892.985	−1.64	680	700	E1E2	65.66	64.98	0.637_{±0.156±0.002}
	2014.08.23	56 892.985	−1.64	700	720	E1E2	65.66	64.98	0.886_{±0.140±0.002}
	2014.10.20	56 950.797	−2.38	680	700	W2S2	149.38	−178.82	0.138_{±0.052±0.002}
	2014.10.20	56 950.797	−2.38	700	720	W2S2	149.38	−178.82	0.050_{±0.082±0.001}
	2014.10.20	56 950.834	−1.51	700	720	W2S2	150.78	171.40	0.081_{±0.050±0.001}
	2014.10.20	56 950.872	0.59	680	700	W2S2	155.72	161.98	0.050_{±0.050±0.001}
	2014.10.20	56 950.872	0.59	700	720	W2S2	155.72	161.98	0.049_{±0.050±0.001}

HD 360	2013.08.26	56 530.922	0.55	695	715	W2S2	144.26	−31.84	0.112_{±0.063±0.002}
	2013.08.26	56 530.922	0.55	715	735	W2S2	144.26	−31.84	0.138_{±0.032±0.002}
	2013.07.24	56 497.945	−1.00	690	710	W2S2	124.66	−17.34	0.252_{±0.025±0.006}
	2013.07.24	56 497.971	−0.41	690	710	W2S2	131.20	−23.79	0.187_{±0.036±0.004}
	2013.07.24	56 497.971	−0.41	710	730	W2S2	131.20	−23.79	0.243_{±0.043±0.005}
	2013.07.24	56 498.003	0.35	690	710	W2S2	141.49	−30.45	0.117_{±0.020±0.003}
	2013.07.24	56 498.003	0.35	710	730	W2S2	141.49	−30.45	0.172_{±0.027±0.005}

H D40020	2013.10.27	56 592.860	− 2.63	725	745	E1E2	61.90	67.00	0.761_{±0.156±0.002}
	2013.11.26	56 622.863	0.59	725	745	E1E2	65.35	62.21	0.584_{±0.192±0.006}
	2013.11.26	56 622.955	1.57	705	725	E1E2	54.87	48.71	0.726_{±0.121±0.008}
	2014.10.22	56 952.938	− 1.05	700	720	W1W2	98.39	−80.11	0.319_{±0.050±0.010}
	2014.10.22	56 952.962	0.45	700	720	W1W2	103.90	−82.36	0.197_{±0.067±0.006}
	2014.10.23	56 953.976	0.04	700	720	W1W2	106.40	−83.77	0.284_{±0.050±0.007}

HD43023	2013.10.26	56 591.903	− 1.98	710	725	E2W2	153.65	−112.31	0.097_{±0.049±0.001}
	2013.10.26	56 591.903	− 1.98	725	740	E2W2	153.65	−112.31	0.124_{±0.022±0.001}
	2013.10.26	56 591.919	− 1.59	705	725	E2W2	155.62	−111.65	0.153_{±0.024±0.002}
	2013.10.26	56 591.919	− 1.59	725	740	E2W2	155.62	−111.65	0.118_{±0.021±0.001}
	2014.10.16	56 947.000	− 0.25	695	715	W1W2	104.65	−86.71	0.504_{±0.061±0.006}
	2014.10.16	56 947.019	0.19	695	715	W1W2	106.99	−86.35	0.419_{±0.049±0.005}
	2014.10.18	56 948.965	− 0.96	695	715	W1W2	98.08	−87.20	0.482_{±0.030±0.004}

HD 5268	2013.07.28	56 501.961	− 1.05	690	710	W2S2	124.28	163.39	0.388_{±0.077±0.009}
	2013.07.28	56 501.961	− 1.05	710	730	W2S2	124.28	163.39	0.336_{±0.072±0.008}

Notes. The columns list the date, the reduced Julian date (RJD = JD − 2 400 000), the hour angle (HA), the minimum and maximum wavelengths over which the squared visibility is calculated, the projected baseline length Bp, and its orientation PA. The last column provides the calibrated squared visibility V² together with the statistic error on V² and the systematic error on V² (see text for details). Only the visibilities with a signal-to-noise ratio on the fringe peak higher than 1.7 were considered. The data are available on the Jean-Marie Mariotti Center OiDB service (available at http://oidb.jmmc.fr).

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