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NULLING DATA REDUCTION AND ON-SKY PERFORMANCE OF THE LARGE BINOCULAR TELESCOPE INTERFEROMETER

  • Authors: D. Defrère, P. M. Hinz, B. Mennesson, W. F. Hoffmann, R. Millan-Gabet, A. J. Skemer, V. Bailey, W. C. Danchi, E. C. Downey, O. Durney, P. Grenz, J. M. Hill, T. J. McMahon, M. Montoya, E. Spalding, A. Vaz, O. Absil, P. Arbo, H. Bailey, G. Brusa, G. Bryden, S. Esposito, A. Gaspar, C. A. Haniff, G. M. Kennedy, J. M. Leisenring, L. Marion, M. Nowak, E. Pinna, K. Powell, A. Puglisi, G. Rieke, A. Roberge, E. Serabyn, R. Sosa, K. Stapeldfeldt, K. Su, A. J. Weinberger, and M. C. Wyatt

2016 The Astrophysical Journal 824 66.

  • Provider: AAS Journals

Caption: Figure 10.

Left: null depth measurements per OB as a function of UT time obtained on 2015 February 8. The blue squares show the calibrator measurements, while the red diamonds represent the β Leo measurements. The estimated instrumental null floor is represented by the solid black line and the corresponding 1σ uncertainty by the dotted lines. Right: corresponding null depth measurements per pointing (same notation). The longer time spent to acquire the second β Leo pointing increased the background bias and hence the dispersion of the null depth measurements per OB in the left-hand plot. This effect results in a larger systematic error for this pointing (see Table 1) and explains the larger error bar in the right-hand plot.

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