The Tremaine-Weinberg method at high redshifts | Astronomy & Astrophysics (A&A)

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Fig. B.1

Minimum projected bar length, $l_{b}^{\min}$ $l_{\rm{b}}^{\min }$ , required for the TW method as a function of redshift. The vertical lines indicate the redshift ranges where two successive filters overlap. As indicated in the legends, the different colors on the main curve, represent different filters.

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