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Observations with the Southern Connecticut Stellar Interferometer. II. First Three-telescope Observations and a New Diameter Measurement of Arcturus

  • Authors: Elliott P. Horch, Sebastian M. Lucero, Max Martone, Riley C. Barrett, Ana I. Baculima Durán, Fiona T. Powers Özyurt, Gage Posick, Alexander Petroski, James W. Davidson, Steven R. Majewski, Richard A. Pellegrino, Paul M. Klaucke, Xavier Lesley-Saldaña, Torrie Sutherland, Olivia S. Weiss

Elliott P. Horch et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 4.

Cross-correlation results obtained on Vega for the entire new dataset presented here. (a) In this case, the plots are made by binning the timing differences between photon pairs in 16 ps bins. The black solid curve is the data, the red dashed curve is a Gaussian fit to the data, and the green dotted lines indicate the expected locations of the peaks based on the timing corrections made throughout the dataset. (b) The same data, but using a bin width of 64 ps.

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