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We examine the variable Chaplygin gas (VCG) model with the aim ofestablishing tight constraints by using type-Ia supernovae, lookback timemeasurements, Baryon Acoustic Oscillations (BAO) and the Gamma Ray Bursts. Wereport the parameter constraints obtained via statistical analysis of cosmicobservables namely, luminosity distance, BAO distance and lookback timemeasurement

Variable Chaplygin Gas: Constraints from Supernovae, BAO, Look Back Time, and GRBs