https://www.selleckchem.com/products/SGI-1776.html
Practical stellar interferometry for space domain awareness is challenged by the relative motions of orbital objects and telescope arrays that require array phasing using guide stars. An orbital object's image sensitivity to the location and brightness of the guide star is problematic, possibly resulting in a degraded resolution or loss of image content when both objects fall within the interferometer's field of view. We characterized an orbital object's visibility using visibility contrast to noise ratios (CNRΔv) as a performance metr
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