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Speckle Imaging with an Electron-multiplying CCD Camera at the WIYN Telescope

Resource type
Authors/contributors
Title
Speckle Imaging with an Electron-multiplying CCD Camera at the WIYN Telescope
Abstract
Electron-multiplying CCD (EMCCD) cameras have extremely strong characteristics for speckle imaging including high quantum efficiency, extremely low effective read noise, and high bandwidth. We report on our first results for binary star astrometry and photometry using an Andor iXon EMCCD at the WIYN 3.5-m Telescope at Kitt Peak. We find that diffraction-limited image reconstructions can be achieved to approximately 15th magnitude and that the device appears to deliver reliable differential photometry of the components of binary star systems. Some implications for stellar astrophysics are discussed.
Publication
Bulletin of the American Astronomical Society
Date
2009-05-01
Volume
40
Pages
16.04
Citation Key
horchSpeckleImagingElectronmultiplying2009
Accessed
11/8/23, 7:57 PM
Library Catalog
NASA ADS
Extra
Conference Name: AAS/Division of Dynamical Astronomy Meeting #40 ADS Bibcode: 2009DDA....40.1604H
Citation
Horch, E., Anderson, L., DeSousa, M., & van Altena, W. F. (2009). Speckle Imaging with an Electron-multiplying CCD Camera at the WIYN Telescope. Bulletin of the American Astronomical Society, 40, 16.04. https://ui.adsabs.harvard.edu/abs/2009DDA....40.1604H