Paper Citation Record · LEDGER

Can the sound horizon-free measurement of $H_0$ constrain early new physics?

As of 4 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2501.16883.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2501.16883 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-04T06:34:03.388597+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T12:53:40.365662Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-07-08T15:55:04.846434Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
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External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 71de9bc9-efc5-4de7-b349-623f11d8ddda · inbound

BAO miscalibration cannot rescue late-time solutions to the Hubble tension cites this paper.

BAO miscalibration cannot rescue late-time solutions to the Hubble tension Can the sound horizon-free measurement of $H_0$ constrain early new physics?

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-04T12:53:40.365662Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 00ee9d37-a1a2-444b-aed5-cbc2d04390e2 · inbound

Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data cites this paper.

Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data Can the sound horizon-free measurement of $H_0$ constrain early new physics?

Reference 25

Resolution: verified exact; arxiv_id, observed 2026-07-04T02:19:23.674007Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation d9d9db1c-b05e-4ad7-a56f-0dbf4d53dd33 · inbound

Imprint of swampland-inspired coupled early dark energy cites this paper.

Imprint of swampland-inspired coupled early dark energy Can the sound horizon-free measurement of $H_0$ constrain early new physics?

Reference 59

Resolution: verified exact; local_arxiv, observed 2026-07-08T15:55:04.847628Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

Observation c61efb8b-1bd1-4851-842b-aee5b548dcbe · inbound

Hubble tension: the shape wall cites this paper.

Hubble tension: the shape wall Can the sound horizon-free measurement of $H_0$ constrain early new physics?

Reference 155

Resolution: unresolved; no resolver link, observed 2026-08-01T08:08:48.669056Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.