Tully-Fisher relation for the sample of spatially resolved galaxies in the MUSE-HDFS. Labels indicate the galaxy ID. The points are color-coded as a function of the V/σ ratio. Galaxies in close pairs and/or showing signatures of recent gravitational interactions are identified with black squares. Previous IFS samples of (massive) star-forming galaxies in similar redshift ranges: IMAGES (gray triangles; Puech et al. 2010) and MASSIV (gray squares; Epinat et al. 2012) are also shown for comparison. The TFR defined in the high-mass regime (M_⋆> 10⁹M_⊙) from previous surveys in a similar redshift range (z = 0.2 − 1.4; Miller et al. 2011; Vergani et al. 2012) is shown with a magenta line. The TFR defined in the low-mass regime (M_⋆< 10⁹M_⊙; Kassin et al. 2007, 2012; Miller et al. 2014; z = 0.2 − 1.0) is shown with a green line. The dotted lines show the dispersion around these relations. A comparison with the predictions from the EAGLE cosmological hydrodynamical simulations for z ≈ 0.1 galaxies (Schaye et al. 2015) is also shown (black line with the dashed lines representing the 16% and 84% percentiles).