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Supplementary Figure 1 Light-polarization-dependent the crystal b-axis. Scale bar, 25 m. (b) Polarization-dependent absorption spectra of bilayer ReS 2. (c) Corresponding spectral weights of Lorentzian L contributions off X 1 (blue absorption of bilayer ReSS 2. (a) optical image of bilayer ReS 2. Thick yellow line indicates 2 dots) and X 2 (red dots). Solid fit lines are proportional to cos ( ) with offset, where values are polarization angles of the excitons ( 16 for X 1 andd 78 for X 2 ). Supplementary Figure 2 Observation of the optical Stark effect e in bilayer ReS 2 at room temperature. (a) bsorption spectrum of bilayer ReS 2 with circularly polarized light. The black arrow indicates the pump photon energy of 1.49 ev for the followingg pump-probe measurements. (b) Transient DT spectra with linearr pump polarization of = 40. (c) Correspondingg DT spectrum at = 0 (circles). Blue (red) vertical lines in (a) andd (c) show the energy of the X 1 (X 2 ) exciton state without pump. (d) DT time-traces near X 1 (blue) andd X 2 (red) exciton energies. Corresponding probe photon energies are shown on the right.

Supplementary Figure 3 Pump-polarization-dependent optical Stark effect e of excitons in bilayer ReS 2 at room temperature. (a) DT spectra at = 0 fss of linearly polarized optical excitations with two important polarization angles of = 20 (blue) and 80 (red), at whichh the pump light is closely y aligned to X 1 and X 2, respectively. The probe is circularly polarized. The blue- (red-) X 1 (X 2 ) state. Inset: light-polarization-dependent absorption a shaded area represents thee spectral region where the DT signal is dominated by thee shift of thee spectral weights of X 1 (blue) and X 2 (red) (arbitrary units). The yellow line indicates the b-axis direction. Double-sided arrows show the angles of the pump-polarizations of the DT spectra s in the main panel. (b)( Pump- and polarization-dependent DT spectra at a = 0. (c) Corresponding absolute DT values at 1.529 ev (blue circles) at 1.619 ev (red circles). Solid liness are fits. Supplementary Figure 4 Pump-fluence dependence of the exciton shifts of few-layer ReS 2 at 78 K. (a,b) Pump-fluence-dependent DT spectraa at = 0 fs with co-linear pump-probe polarization configurations at = 20 (a) and = 90 (b).. Pump photon energy is fixed at 1.444 ev. (c,d) Corresponding pump-induced shift of X 1 (c) and X 2 (d). Solid lines are guides to the eye.

Supplementary Figure 5 Estimation of EE 1 of few-layer ReS 2 at 787 K. (a) DTT trace at the fixed probe photon energy of 1.526 ev. Polarizations of pump and probe are both = 20. (b,c) Corresponding DT spectrum at = 0 fs (b) and 350 fs (c). Note that ( b) is identical to the middle panel of Fig. 3a in the main text. (d) Black dots are background-subtracted DT spectrum (left axis) and red solid line is / E / 1 scaled by E (right axis). a Supplementary Figure 6 Spectral distance between X 1 and X 2. Blue B and red lines are background subtracted absorption spectra of few-layer ReS 2 at 78 K with light polarization of = 20 (blue) and = 90 (red). Original spectra are shown in thee top panels of Fig. 3a and 3b of the main text. Black arrow shows spectra distance between X 1 andd X 2. Green arrows indicate their halff linewidths. We can see that the spectral distance between X 1 andd X 2 excitons (0.033 ev, black b arrow) ) is about 1.65 times larger than the sum of their half linewidths l (0.011 ev + 0.009 ev, green arrows), meaning that the two exciton levels are well separated. This fact further justifies that our findings in Fig. 3 of the main text possess energy-selectivity for the excitonic optical Stark effect.

Supplementary Figure 7 Pump-polarization-dependent DT spectra. (a,b) Pump-fluence-- dependent DT spectra at = 0 fs with probe polarization of = 20 (a) and = 90 (b). Pump photon energy is fixed at 1.44 ev. Offsett for clarity. Supplementary Note 1. Tunable optical Stark effect in bilayer ReS 2 at room temperature. In this section, we present optical Stark effect of excitons in bilayer ReS 2 at room temperature (see Supplementary Figure 1a for the optical image of the bilayer sample). Similar to the t results in the main text, excitons in bilayer ReS 2 also show pump-polarization-dependent optical Stark shiftss as follows.. In this experiment, unlike the main text, while we used polarization-controlled linear pump pulses to excite the sample,, we used circularly polarized pulses p (possessing the whole electric-field directions) to probe DT. The reason for this was too focus solely on the influence of the pump polarization on the system ss optical response, and to experimentally exclude the contribution of probe light on the measured polarization-dependent signals. However, unlike the discussion in the main text (where linearly polarized probee beams are used to selectively measuree the shift of one exciton state, see Fig. 3 in the main text), such measurements

requires many parameters for estimating the shifts of excitons because both X 1 and X 2 have effects on DT spectrum 1. For this reason, we analyze the data in this section without estimating E. We first measured the light-polarization dependent equilibrium absorption spectra, as shown in Supplementary Figure 1b. Similar to the few-layer sample (Fig. 1d in the main text), the absorption peaks (X 1 and X 2 ) arise from the two exciton states and show strong polarization dependence 2. Corresponding -dependent Lorentzian spectral weights are shown in Supplementary Figure 1c, where the excitons are polarized at different angles ( ~ 16 and ~ 78 for X 1 and X 2, respectively). We now explore the detailed DT response of bilayer ReS 2 with fixed pump polarization ( = 40) to confirm the excitonic optical Stark effect. Supplementary Figure 2a shows the equilibrium absorption spectrum with circularly polarized light. Two absorption peaks due to X 1 and X 2 are observed near 1.55 ev and 1.60 ev, respectively (see vertical lines) 2. To measure the optical Stark shifts of these two states, we excited the sample with pump photon energy detuned to 60 mev below X 1 transition (see black arrow in Supplementary Figure 2a) and monitored the time-resolved DT spectra, as shown in Supplementary Figure 2b. Here, the line-cut DT spectrum at = 0 fs (circles in Supplementary Figure 2c) clearly shows positiveto-negative sign changes near X 1 and X 2, indicating optical Stark shifts of both excitons. This is corroborated by the DT time-traces (Supplementary Figure 2d). Next, we investigate how the optical Stark effects of the excitons change depending on light polarization. For this purpose, we measured the DT spectra at = 0 while varying the polarization () of the pump with photon energy detuned to 60 mev below the X 1 level and -2 fluence fixed at0.42mjcm. First, we compare the two representative DT responses at =

20 and = 80, at which the pump polarizations are closely aligned along X 1 (~ 16) and X 2 (~ 78), respectively. The main panel of Supplementary Figure 3a clearly shows that when the spectral region is dominated by the optical Stark shift of X 1 resonance (blue-shaded area), the amplitude of the DT signals at = 20 (blue dots) is larger than that at = 80 (red dots). On the contrary, in the X 2 -dominated spectral region (red-shaded area), the DT amplitude at = 80 shows a larger signal compared to that at = 20. This result implies that the optical Stark effect is strong when the orientation of pump light is parallel with the polarization of each exciton, agreeing well with results in the main text. We also measured the pump-polarization-dependent DT spectra by tuning the angles of pump polarization continuously at = 0 fs (Supplementary Figure 3b). In Supplementary Figure 3c, we plot corresponding absolute DT values at 1.529 ev (1.619 ev), at which the response is dominated by X 1 (X 2 ). s indicated by the solid lines in Supplementary Figure 3c, their gradual changes as a function of can be well fit with a simple function E 2 a bcos ( ), setting to the individual excitons original polarizations (i.e., = 16 for X 1 and = 78 for X 2 ). These results are well in accordance with the behavior of the few-layer sample in the main text. notable fact is that DT for both exciton states is not negligible even when the pump polarization is orthogonal to, which is a feature not seen in the absorption spectral weight (Supplementary Figure 1c). This may be because the two excitonic transitions share either the same conduction band or valence band which forms the exciton states 1,3,4. Supplementary Note 2. Pump-fluence-dependent shifts of exciton levels. Supplementary Figure 4a (4b) shows the pump-fluence-dependent DT spectra at = 0 fs

under the same conditions described in the caption of the middle panel of Fig. 3a (3b) in the main text. We see that corresponding magnitudes of the shift in X 1 (X 2 ) resonance shows characteristic linear-dependence on the pump fluence, as shown in Supplementary Figure 4c. Considering the relation of E 2 F (where is electric field intensity; F is pump fluence, see main text), these results further confirm that the measured DT arises from the optical Stark effect of excitons 5. Supplementary Note 3. Estimation of the optical Stark effect from the DT response In this section, we discuss the estimation procedure of the optical Stark shift (E). Generally, DT is given by 6. T T E E 1 with pump E E, (1) where no E ( with pump E pump ) is absorption without (with) pump excitation. When blueshift of an exciton dominates the DT response, E E, which yields 7 with pump E can be approximated by T T E E E E E E 1 E E E 1. (2) This result tells us that the DT arising from the optical Stark effect resembles the derivative of absorption, as discussed in the main text (see Fig. 2b in the main text). In addition, we can see that the magnitude of the shift (E) can be estimated by comparing the measured DT lineshape with the E/ 1 / spectrum scaled by E (wheree is only a

free parameter) 8,9. s an example, let us trace the procedure for estimating the blue-shift of X 1 (E 1 ) from the measured DT spectrum in the middle panel of Fig. 3a (note that Supplementary Figure 5b shows same graph). lthough the optical Stark effect dominates the DT response, its somewhat asymmetric (Supplementary Figure 5b) with a small deviation from the derivative of absorption, considering that the derivative of a single exciton resonance is generally symmetric. This is because the DT response at = 0 fs is affected by pump-excited real carriers, which are generated by two-photon- or phonon-mediated-absorption of pump photons 5,10. Such a mixed response is corroborated by the DT trace in Supplementary Figure 5a, where a spike-like peak at = 0 fs due to the optical Stark effect is followed by longlasting signals originating from pump-generated carriers. Indeed, the transient DT spectrum directly after the optical Stark shift (at = 350 fs, see Supplementary Figure 5c) shows a typical bleaching-like shape of X 1 transition 11. In order to distinguish the bleaching effect from the Stark shift, we subtract the DT at = 350 fs (Supplementary Figure 5c) from the DT at = 0 fs (Supplementary Figure 5b) 7, producing an almost symmetric shape, as indicated by black dots in Supplementary Figure 5d. This background-subtracted DT spectrum now closely follows the lineshape of E/ 1 / (red line in Supplementary Figure 5d), which enables us to estimate E by comparing two graphs in Supplementary Figure 5d. Supplementary References 1. Choi, C. K. et al. Polarization dependence of the excitonic optical stark effect in GaN. Phys 65, 155206 (2002). 2. slan, O. B., Chenet, D. a., van der Zande,. M., Hone, J. C. & Heinz, T. F. Linearly polarized excitons in single- and few-layer ReS 2 crystals. CS Photonics 3, 96 101 (2016).

3. Gupta, J. a, Knobel, R., Samarth, N. & wschalom, D. D. Ultrafast manipulation of electron spin coherence. Science. 292, 2458 2461 (2001). 4. Joffre, M., Hulin, D., Migus,. & Combescot, M. Laser-induced exciton splitting. Phys. Rev. Lett. 62, 74 (1988). 5. Von Lehmen,., Chemla, D. S., Zucker, J. E. & Heritage, J. P. Optical Stark effect on excitons in Gas quantum wells. Opt. Lett. 11, 609 611 (1986). 6. Schmidt, R. et al. Ultrafast Coulomb intervalley coupling in atomically thin WS 2. Nano Lett. 16, 2945 (2016). 7. Sie, E. J. et al. Valley-selective optical Stark effect in monolayer WS 2. Nat. Mater. 14, 290 (2014). 8. Song, D. et al. Measurement of the optical Stark effect in semiconducting carbon nanotubes. ppl. Phys. 96, 283 287 (2009). 9. Kim, J. et al. Ultrafast generation of pseudo-magnetic field for valley excitons in WSe2 monolayers. Science 346, 1205 (2014). 10. Knox, W. H., Chemla, D. S., Miller, D. a B., Stark, J. B. & Schmitt-Rink, S. Femtosecond ac Stark effect in semiconductor quantum wells: Extreme low- and highintensity limits. Phys. Rev. Lett. 62, 1189 1192 (1989). 11. Sim, S. et al. Exciton dynamics in atomically thin MoS 2 : Interexcitonic interaction and broadening kinetics. Phys. Rev. B 88, (2013).