4 August 2010 Heterogeneous array imaging with the CARMA Telescope
Author Affiliations +
The CARMA telescope is a heterogeneous array of 10.4, 6.1 and 3.5 m antennas, with antenna configurations providing spacings from ~3.5 m to 2 km. This heterogeneous array is well suited to imaging a wide range of spatial scales. In compact configurations the heterogeneous array provides high quality short spacing data for aperture synthesis. In extended configurations, the antennas can be paired, with 6.1 and 10.4m antennas making science observations in the 3 mm and 1 mm bands, while 3.5 m antennas are simultaneously observing calibration sources within a few degrees in the 1 cm band. This unique Paired Antenna Calibration System allows us to to correct for atmospheric phase fluctuations and make images at 0.15 arcec resolution in a wide range of atmospheric seeing conditions. In this paper we discuss some results and lessons learned using these heterogeneous observing techniques. These results are relevant to all aperture synthesis arrays, including millimeter/submillimeter wavelength arrays like ALMA, and cm/m wavelength arrays like ATA and SKA.
© (2010) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
M. C. H. Wright, M. C. H. Wright, } "Heterogeneous array imaging with the CARMA Telescope", Proc. SPIE 7733, Ground-based and Airborne Telescopes III, 77331B (4 August 2010); doi: 10.1117/12.856707; https://doi.org/10.1117/12.856707


An information theoretic approach to optical interferometry
Proceedings of SPIE (February 21 2003)
Imaging interferometry: lessons from the ground
Proceedings of SPIE (September 10 1993)
An interferometry imaging beauty contest
Proceedings of SPIE (October 20 2004)

Back to Top