Tully-Fisher Relation of Late-type Galaxies at $0.6 \leq z \leq 2.5$

Understand

We present a study of the stellar and baryonic Tully-Fisher relation within the redshift range of $0.6 \leq z \leq 2.5$ utilizing observations of \sfgs.

• This dataset, as explored in \citet{GS23}, comprises of disk-like galaxies spanning a stellar mass range of $8.89 \leq \log(M_{star} \ [\mathrm{M_\odot}]) \leq 11.5$, baryonic mass range of $9.0 \leq \log(M_{bar} [\mathrm{M_\odot}]) \leq 11.5$, and circular velocity range of $1.65 \leq \log(V_c \ [{\rm km/s}]) \leq 2.85$.
• Stellar masses of these objects are estimated using spectral energy distribution fitting techniques, while gas masses are determined via scaling relations.
• Circular velocities are directly derived from the Rotation Curves (RCs), after meticulously correcting for beam smearing and pressure support.