Wavelength Dependence of the ACS Coronagraphic PSF

Details Wavelength Dependence of the ACS Coronagraphic PSF Wavelength Dependence of the ACS Coronagraphic PSF

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aas...201.2103s&link_type=abstract

American Astronomical Society, 201st AAS Meeting, #21.03; Bulletin of the American Astronomical Society, Vol. 34, p.1138

Astronomy and Astrophysics

Astronomy

Scientific paper

In principle, the wavelength dependence of diffraction and scattering structure in a space-based coronagraphic PSF can be used to good effect in removing the halo light of the host star (Sparks and Ford 2002). Here, we test application of this ``spectral deconvolution'' method using observations of the double brown dwarf near HD130948A with the Aberrated Beam Coronagraph on HST's Advanced Camera for Surveys.

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