The paper explores the asymptotic charges and their algebra in the partial Bondi gauge, a gauge that allows for the study of gravitational waves and asymptotic symmetries in general relativity. In this gauge, the solution space is defined by three conditions on the metric, allowing for a residual freedom in the radial coordinate. The authors compute the asymptotic charges, which include super-translations, super-rotations, and Weyl transformations, as well as two new asymptotic symmetries associated with non-vanishing charges. These new symmetries arise from a weaker definition of the radial coordinate and involve traces in the transverse metric. The paper also presents complete gauge fixing conditions in which these extra asymptotic symmetries and charges survive. As a byproduct, the charges in the Newman–Unti gauge are obtained, and the paper applies the results to the Kerr spacetime in Bondi coordinates. The study of these charges is important for understanding the asymptotic structure of spacetime, particularly in relation to gravitational waves, holography, and the infrared triangle. The paper also discusses the implications of these results for the study of asymptotic symmetries and charges in general relativity.The paper explores the asymptotic charges and their algebra in the partial Bondi gauge, a gauge that allows for the study of gravitational waves and asymptotic symmetries in general relativity. In this gauge, the solution space is defined by three conditions on the metric, allowing for a residual freedom in the radial coordinate. The authors compute the asymptotic charges, which include super-translations, super-rotations, and Weyl transformations, as well as two new asymptotic symmetries associated with non-vanishing charges. These new symmetries arise from a weaker definition of the radial coordinate and involve traces in the transverse metric. The paper also presents complete gauge fixing conditions in which these extra asymptotic symmetries and charges survive. As a byproduct, the charges in the Newman–Unti gauge are obtained, and the paper applies the results to the Kerr spacetime in Bondi coordinates. The study of these charges is important for understanding the asymptotic structure of spacetime, particularly in relation to gravitational waves, holography, and the infrared triangle. The paper also discusses the implications of these results for the study of asymptotic symmetries and charges in general relativity.