Translator Disclaimer
9 July 2018 Stellar photon correlation detection with the Southern Connecticut stellar interferometer
Author Affiliations +
The Southern Connecticut Stellar Interferometer (SCSI) is a portable optical intensity interferometer located on the campus of Southern Connecticut State University in New Haven, Connecticut. Since its completion in 2016, the instrument has been used to take engineering data of bright stars. This paper will discuss the data collection and analysis methods, as well as the progress toward reliably measuring a significant stellar photon correlation. Vega has been the main star chosen for test observations to date because its diameter is well known by other methods, and it is not an extended source for the baselines used. The correlation peak in the processed data is compared to theoretical expectations. Given our expected sensitivity, a significant correlation peak is expected for small baselines (~2 m) to appear after a few hours of observation. So far, the observations indicate that the correlation peak is at the expected time delay, and the signal-to-noise ratio roughly scales as predicted.
Conference Presentation
© (2018) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Samuel A. Weiss, Justin D. Rupert, and Elliott P. Horch "Stellar photon correlation detection with the Southern Connecticut stellar interferometer ", Proc. SPIE 10701, Optical and Infrared Interferometry and Imaging VI, 107010X (9 July 2018); doi: 10.1117/12.2313922;


SCSI: the Southern Connecticut Stellar Interferometer
Proceedings of SPIE (August 03 2016)
Status of PRIMA for the VLTI: heading to astrometry
Proceedings of SPIE (September 11 2012)
Portable intensity interferometry
Proceedings of SPIE (September 11 2012)
Interferometric measurements of stellar intensity profiles
Proceedings of SPIE (February 20 2003)

Back to Top