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Cited article:

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Kuiper Belt–like Hot and Cold Populations of Planetesimal Inclinations in the β Pictoris Belt Revealed by ALMA

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A Model-independent Mass and Moderate Eccentricity for β Pic b

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Spectroscopic transit search: a self-calibrating method for detecting planets around bright stars

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The mass of the young planet Beta Pictoris b through the astrometric motion of its host star

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