Compilation of Hubble constant values obtained using different observations and techniques from the recent literature including the value from this work. The literature references are written on the y-axis. Two independent estimates from early Universe (Planck Collaboration XIII 2016; Abbott et al. 2018) are shown at the bottom. The next is an estimate using extragalactic background light γ ray attenuation (Domínguez et al. 2019) and another from BAO at all redshifts + BBN estimate (Cuceu et al. 2019). Then we show measurements from SNe Ia calibrated with TRGB (Freedman et al. 2019), SNe Ia calibrated with Cepheids (SH0ES sample, Riess et al. 2016, 2019), using near-infrared (NIR) filters (Burns et al. 2018) and SNe Ia with Mira variables (Huang et al. 2020). Then we show the H₀ values estimated using 6 masers in the Hubble flow (Pesce et al. 2020). The next H₀ value shown is inferred via gravitational lensing time delays using six lensed quasars (Wong et al. 2020) and a more recent value obtained using 40 strong lenses (Birrer et al. 2020). Finally we shows the H₀ derived with gravitational-wave signals from binary compact object mergers (Abbott et al. 2019).