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Paper Citation Record · LEDGER

Where will supersymmetric dark matter first be seen?

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1107.1916.

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

pith.paper-citation-record.v1
1107.1916 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-05T06:32:48.257954+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-14T07:56:20.592048Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-03T02:47:36.900592Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

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 086a4aea-915d-4617-b973-da4d5e682e34 · inbound

Too Heavy to Hide: Gamma-Ray Constraints on Annihilating Dark Matter beyond Unitarity cites this paper.

Too Heavy to Hide: Gamma-Ray Constraints on Annihilating Dark Matter beyond Unitarity Where will supersymmetric dark matter first be seen?

Reference 109

Resolution
verified exact
local_arxiv, observed 2026-07-03T02:47:36.901721Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=pdf_text observed=2026-06-27T15:45:26.154619Z digest=sha256:6254e46e539eb10023e6fccb8039215ad5039aa6a191b0f903c9168ec9f02c9b

Observation bd098424-30d0-4576-978e-4733cc09199d · inbound

Constraints on Annihilating Dark Matter from Gamma-Ray Background-Galaxy Shape Correlations: Model-independent Null Results and Moderate Template-based Signals cites this paper.

Constraints on Annihilating Dark Matter from Gamma-Ray Background-Galaxy Shape Correlations: Model-independent Null Results and Moderate Template-based Signals Where will supersymmetric dark matter first be seen?

Reference 39

Resolution
unresolved
no resolver link, observed 2026-07-14T07:56:20.592048Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T07:56:20.592048Z digest=sha256:68f326b7d87effd0b289a3c20576c2d89e74ca966bc5ae6bcdbe52adee023243