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SARAS 3 tests a reported cosmic-dawn absorption profile

Contribution grade

Observational cosmology · Source-reported experimental result or reusable measurement method

Reference score100,000Provisional editorial estimate of this exact contribution; its grade is assessed separately.

What changed

The SARAS 3 radiometer measured a sky-averaged radio spectrum and compared it with the absorption profile previously reported by EDGES. With the paper’s foreground and calibration model, its fit disfavoured the earlier best-fitting profile at 95.3% confidence; the authors also tested the wider set of profiles allowed by EDGES.

Scientific scope

The SARAS 3 radiometer measured a sky-averaged radio spectrum and compared it with the absorption profile previously reported by EDGES. With the paper’s foreground and calibration model, its fit disfavoured the earlier best-fitting profile at 95.3% confidence; the authors also tested the wider set of profiles allowed by EDGES. This is an independent observational challenge to a specific earlier best-fit profile, not a detection of the cosmic-dawn 21-cm signal or proof that every possible 21-cm absorption profile is absent. The reported 95.3% applies to one best-fit template; the paper gives 90.4% for the weighted set of allowed profiles. Results rely on the selected 55–85 MHz science band, sixth-order foreground model, assumed systematic-error treatment and finite sensitivity. The cause of the EDGES spectral feature is not independently identified. The EDGES report is recorded separately with its own authors.

Evidence

The linked original works support the scoped statement and contribution attribution. WRS has not independently replayed experiments or reconstructed a full mathematical proof. This is an independent observational challenge to a specific earlier best-fit profile, not a detection of the cosmic-dawn 21-cm signal or proof that every possible 21-cm absorption profile is absent. The reported 95.3% applies to one best-fit template; the paper gives 90.4% for the weighted set of allowed profiles. Results rely on the selected 55–85 MHz science band, sixth-order foreground model, assumed systematic-error treatment and finite sensitivity. The cause of the EDGES spectral feature is not independently identified. The EDGES report is recorded separately with its own authors.

Contributors

Provisional WRS assessment, edition 2026-10-28.1. Independent expert calibration is pending. This grade does not certify correctness or assign ownership.

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