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

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Fig. 6

Distribution of the ratio $Ω_{p}^{TW} / Ω_{p}^{DSS}$ $\Omega _{\rm{p}}^{{\rm{TW}}}/\Omega _{\rm{p}}^{{\rm{DSS}}}$ (blue histogram) for 32 galaxies (9 with weak bars and 23 with strong bars) that are sufficiently extended to be detected by the TW method at ɀ ≃ 1.2. Here $Ω_{p}^{TW}$ $\Omega _{\rm{p}}^{{\rm{TW}}}$ is measured at ɀ ≃ 1.2, while $Ω_{p}^{DSS}$ $\Omega _{\rm{p}}^{{\rm{DSS}}}$ is measured at ɀ ≃ 0. The blue curve represents the continuous probability density functions derived from the data.

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