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  2. Dillard’s is an 86-year-old department store chain—and its ...

    www.aol.com/finance/dillard-86-old-department...

    Dillard's CEO Bill Dillard II talks with the media in Dillard's at Penn Square Mall Friday, May 8, 2020, in Oklahoma City, the fourth day the store has been open since temporarily closing due to ...

  3. Coupon (finance) - Wikipedia

    en.wikipedia.org/wiki/Coupon_(finance)

    Coupons are normally described in terms of the "coupon rate", which is calculated by adding the sum of coupons paid per year and dividing it by the bond's face value. [2] For example, if a bond has a face value of $1,000 and a coupon rate of 5%, then it pays total coupons of $50 per year.

  4. Interferometric visibility - Wikipedia

    en.wikipedia.org/wiki/Interferometric_visibility

    The interferometric visibility (also known as interference visibility and fringe visibility, or just visibility when in context) is a measure of the contrast of interference in any system subject to wave superposition.

  5. Dillard High School - Wikipedia

    en.wikipedia.org/wiki/Dillard_High_School

    Dillard is available to all of Broward County. The school is a magnet school for Emerging Computer Technology and Performing Arts. Dillard serves sections of Fort Lauderdale for middle school and sections of Fort Lauderdale and Lauderhill for high school. [3] [4] Dillard has an FCAT school grade of "A" for the 2013–2014 academic year. [5]

  6. List of optometric abbreviations - Wikipedia

    en.wikipedia.org/wiki/List_of_optometric...

    Abbreviation Term Description (notes) BC Base curve: BOZD Back optic zone diameter BOZR Back optic zone radius BVP Back vertex power CLAPC/CLIPC Contact-lens-associated/induced papillary conjunctivitis

  7. Airy disk - Wikipedia

    en.wikipedia.org/wiki/Airy_disk

    Thus the radius of the spurious disk of a faint star, where light of less than half the intensity of the central light makes no impression on the eye, is determined by [s = 1.17/a], whereas the radius of the spurious disk of a bright star, where light of 1/10 the intensity of the central light is sensible, is determined by [s = 1.97/a].

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