A multi-wavelength study of the young star V1118 Orionis in outburst

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Volume 511 (February 2010)

A&A, 511 (2010) A63

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Table A.1:

Comparison stars for the SMARTS photometry.
Comparison	B	V	R	I	$\delta V$	$\delta I$
IV Ori	16.19 $\pm$ 0.35	14.94 $\pm$ 0.26	13.97 $\pm$ 0.22	13.19 $\pm$ 0.13
CSV 6218	17.40 $\pm$ 0.13	15.90 $\pm$ 0.13	14.74 $\pm$ 0.13	13.68 $\pm$ 0.15	0.20	0.36
V759 Ori	16.81 $\pm$ 0.12	15.44 $\pm$ 0.09	14.32 $\pm$ 0.10	13.14 $\pm$ 0.13	0.10	0.24
NGC 1977 311	14.32 $\pm$ 0.11	13.24 $\pm$ 0.09	12.46 $\pm$ 0.09	11.73 $\pm$ 0.12
V1175 Ori	16.59 $\pm$ 0.10	15.19 $\pm$ 0.07	14.19 $\pm$ 0.09	13.26 $\pm$ 0.12	0.08	0.14
JW 94	20.82 $\pm$ 0.35	19.10 $\pm$ 0.17	17.37 $\pm$ 0.10	15.45 $\pm$ 0.13	0.10	0.29
JW 100	20.25 $\pm$ 0.32	18.48 $\pm$ 0.15	17.09 $\pm$ 0.10	15.44 $\pm$ 0.12	0.03	0.23
Par 1606	17.18 $\pm$ 0.10	15.61 $\pm$ 0.07	14.38 $\pm$ 0.08	13.22 $\pm$ 0.12	0.03	0.12
CXORRS J053447.9-053544	22.00 $\pm$ 0.99	19.79 $\pm$ 0.32	17.76 $\pm$ 0.13	15.79 $\pm$ 0.12	0.67	0.23
NSV2246	11.32 $\pm$ 0.26	10.30 $\pm$ 0.17	9.78 $\pm$ 0.16	9.25 $\pm$ 0.13	0.08	0.06
JW 33	18.75 $\pm$ 0.32	17.30 $\pm$ 0.10	16.16 $\pm$ 0.09	14.84 $\pm$ 0.12	-0.03	0.15

Notes. $\delta V$ and $\delta I$ are the difference between these V, Ideterminations and those published by Hillenbrand (1997).

Source LaTeX | All tables | In the text

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