Gaussian processes (GP) provide an elegant and model-independent method for extracting
cosmological information from the observational data. In this work, we employ GP to
perform a joint analysis by using the geometrical cosmological probes such as Supernova
Type Ia (SN), Cosmic chronometers (CC), Baryon Acoustic Oscillations (BAO), and the
H0LiCOW lenses sample to constrain the Hubble constant
H0
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