Data reduction for stellar speckle interferograms of binary stars based on the shift-and-add method

Details Data reduction for stellar speckle interferograms of binary stars based on the shift-and-add method Data reduction for stellar speckle interferograms of binary stars based on the shift-and-add method

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987apopt..26.2306b&link_type=abstract

Applied Optics (ISSN 0003-6935), vol. 26, June 15, 1987, p. 2306-2310. MOESC-supported research.

Physics

Optics

2

Binary Stars, Speckle Interferometry, Stellar Magnitude, Astronomical Maps, Computerized Simulation, Cross Sections

Scientific paper

The shift-and-add (SAA) method is used to estimate the magnitude
difference of binary star components. A simple procedure based on the
SAA method enables an accurate estimation of the magnitude difference.
Some computer simulations confirm this. The use of this procedure in
stellar speckle interferograms is also demonstrated.

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