Paper Citation Record · LEDGER

Dark sector interaction and the supernova absolute magnitude tension

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2107.09151.

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

pith.paper-citation-record.v1
2107.09151 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T19:20:16.906863Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T07:47:45.269406Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
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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 00469451-c137-4c8e-af66-ba9bb82b5337 · inbound

Sign Switching in Dark Sector Coupling Interactions as a Candidate for Resolving Cosmological Tensions cites this paper.

Sign Switching in Dark Sector Coupling Interactions as a Candidate for Resolving Cosmological Tensions Dark sector interaction and the supernova absolute magnitude tension

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-10T19:20:16.906863Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c9b2596a-36be-46de-82c1-3f52f5e23c42 · inbound

Dark Energy Is Not That Into You: Variable Couplings after DESI DR2 BAO cites this paper.

Dark Energy Is Not That Into You: Variable Couplings after DESI DR2 BAO Dark sector interaction and the supernova absolute magnitude tension

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-05T16:03:01.345251Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4ac1db43-0750-4521-8f73-f8580662a728 · 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 Dark sector interaction and the supernova absolute magnitude tension

Reference 227

Resolution: unresolved; no resolver link, observed 2026-08-04T12:53:52.338407Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5d2d0954-9220-4c9f-9088-88631c17a363 · inbound

Robust Preference for Dark Sector Interactions cites this paper.

Robust Preference for Dark Sector Interactions Dark sector interaction and the supernova absolute magnitude tension

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.814655Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 016ffd33-86f4-4b2e-b54a-c98843000848 · inbound

Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension cites this paper.

Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension Dark sector interaction and the supernova absolute magnitude tension

Reference 92

Resolution: verified exact; arxiv_id, observed 2026-05-16T12:17:52.377978Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 79cb4072-136d-4fe0-ae03-c22cfb20abdb · inbound

Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions cites this paper.

Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions Dark sector interaction and the supernova absolute magnitude tension

Reference 179

Resolution: verified exact; arxiv_id, observed 2026-07-01T16:45:51.078520Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 38f028b7-1645-4cdd-8141-235f081631f6 · inbound

What it takes to solve the Hubble tension through Modifications of Cosmological Recombination II: in light of ACT DR6 and DESI DR2 cites this paper.

What it takes to solve the Hubble tension through Modifications of Cosmological Recombination II: in light of ACT DR6 and DESI DR2 Dark sector interaction and the supernova absolute magnitude tension

Reference 44

Resolution: verified exact; arxiv_id, observed 2026-07-02T15:37:06.232511Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 2ec607f0-9e45-4330-93e6-59105b6746a8 · inbound

Non-linear Structure Formation in Planck+DESI Favoured Interacting Dark Energy Cosmologies cites this paper.

Non-linear Structure Formation in Planck+DESI Favoured Interacting Dark Energy Cosmologies Dark sector interaction and the supernova absolute magnitude tension

Reference 47

Resolution: verified exact; arxiv_id, observed 2026-07-03T07:47:45.270713Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.