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Companion detection limits with adaptive optics coronagraphy

Oppenheimer, B. R. and Dekany, R. G. and Hayward, T. and Brandl, B. and Troy, M. and Bloemhof, E. E. (2000) Companion detection limits with adaptive optics coronagraphy. In: Adaptive Optical Systems Technology. No.4007. Society of Photo-optical Instrumentation Engineers (SPIE) , Bellingham, WA, pp. 309-315. ISBN 9780819436320. https://resolver.caltech.edu/CaltechAUTHORS:20190118-102250480

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Abstract

We presented a detailed observational study of the capabilities of the Palomar Adaptive Optics System and the PHARO near infrared camera in coronagraphic mode. The camera provides two different focal plane occulting masks consisting of completely opaque circular disks of diameter 0.433 arcsec and 0.965 arcsec, both within the cryogenic dewar. In addition, three different pupil plane apodizing masks (a.k.a. Lyot masks) are provided which downsize the beam. The six different combinations of Lyot mask and focal plane mask provide for different levels of suppression of the point spread function of a bright star centered on the focal plane mask. We obtained images of the bright nearby star Gliese 614 with all six different configurations in the K-band filter. Herein, we provide an analysis of the dynamic range achievable with these configurations. The dynamic range (the ratio of the primary star intensity to the intensity of the faintest point source detectable in the images) is a complicated function of not only the angular separation of the primary star and companion, but also of the azimuthal angle because of the complex point spread function of the primary star, which is also wavelength dependent. However, beyond 2.5 arcseconds from the star, regardless of the wavelength of the observation, the detection limit of a companion is simply the limiting magnitude of the image, as determined by the sensitivity of the PHARO camera. Within that radius, the dynamic range is at least 8 magnitudes at the 5(sigma) level and as high as 12 in a one second exposure. This represents a substantial gain over similar techniques without adaptive optics, which are generally limited to radii beyond two arcsec. We provide a quantitative discussion and recommendation for the optimal configuration along with a detailed comparison with recent theoretical predictions of AO coronagraphic performance.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.1117/12.390385DOIArticle
ORCID:
AuthorORCID
Oppenheimer, B. R.0000-0001-7130-7681
Additional Information:© 2000 Society of Photo-optical Instrumentation Engineers (SPIE). BRO acknowledges the support of a Hubble Space Telescope Postdoctoral Fellowship and the support of FUTDI. We thank Anand Sivaramakrishnan for useful comments and a careful reading of the manuscript.
Funders:
Funding AgencyGrant Number
Hubble Space TelescopeUNSPECIFIED
FUTDIUNSPECIFIED
Subject Keywords:Adaptive Optics, Coronagraphy, High Dynamic Range Imaging
Issue or Number:4007
Record Number:CaltechAUTHORS:20190118-102250480
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190118-102250480
Official Citation:Ben R. Oppenheimer, Richard G. Dekany, Thomas L. Hayward, Bernhard Rainer Brandl, Mitchell Troy, Eric E. Bloemhof, "Companion detection limits with adaptive optics coronagraphy," Proc. SPIE 4007, Adaptive Optical Systems Technology, (7 July 2000); doi: 10.1117/12.390385
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:92368
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:21 Jan 2019 22:54
Last Modified:20 Feb 2020 19:08

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