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Fig. A.6

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The photometry of the intended target, HH Nor, is heavily dominated by the brighter, nearby object VSX J154329.4–515037, which is indeed a variable RR Lyr star (RRAB) with a period of 0.59 days. In fact, HH Nor is an eclipsing binary with mean V magnitude of 10.9 and a period of 8.58 days.

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