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This is a Observational study (also classified as: Findings Consistent with Meta-Analysis).

Determining H_0 from a distance sum rule that combines gamma-ray bursts with observational Hubble data and strong gravitational lensing

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The model-independent analysis reveals significant constraints on the hubble constant using strong gravitational lensing data.
Findings indicate that the value of the hubble constant agrees at the 1σ level with values derived from type Ia supernovae.
This method utilizes observational hubble data through Bézier interpolation, applied across late- and early-time data catalogs.
The research suggests that gamma-ray bursts can help trace expansion history while reconciling Hubble's tension.

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Analysis finds model-independent bounds on the hubble constant in relation to gamma-ray bursts and gravitational lensing.

Luongo et al. (2025) studied this question.

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