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Paper Citation Record · LEDGER

CTA and SWGO can Discover Higgsino Dark Matter Annihilation

As of 24 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2405.13104.

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

pith.paper-citation-record.v1
2405.13104 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 7 of 7 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-23T06:30:58.430688+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T17:29:58.427935Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-02T09:46:50.332896Z

Reference resolution

0 of 0 outbound references displayed

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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 b3c640a8-b523-43fa-84a6-ebb5bbfff079 · inbound

The curtain lowers on directly detectable higgsino dark matter cites this paper.

The curtain lowers on directly detectable higgsino dark matter CTA and SWGO can Discover Higgsino Dark Matter Annihilation

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-11T17:29:58.427935Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T17:29:58.427935Z digest=sha256:e63eb62682bca4f3e96ef020ad4db7482b24e60365ead4984576c63c4a6393d4

Observation 7e3a31eb-e31f-4079-ae32-61bf4654de8b · inbound

Theoretical Predictions for the Inner Dark Matter Distribution in the Milky Way Informed by Simulations cites this paper.

Theoretical Predictions for the Inner Dark Matter Distribution in the Milky Way Informed by Simulations CTA and SWGO can Discover Higgsino Dark Matter Annihilation

Reference 63

Resolution
unresolved
no resolver link, observed 2026-08-10T14:57:14.235484Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T14:57:14.235484Z digest=sha256:55852e01a1fe6e188ead7fa9dd92cfc380148cb6d173228ec390bf073797e08d

Observation 837c0c42-b1ba-412c-af58-d50a17c256d7 · inbound

Discovering the Higgsino at CTAO-North within the Decade cites this paper.

Discovering the Higgsino at CTAO-North within the Decade CTA and SWGO can Discover Higgsino Dark Matter Annihilation

Reference 13

Resolution
unresolved
no resolver link, observed 2026-08-07T05:27:43.656332Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T05:27:43.656332Z digest=sha256:f1c8cba3f4be2104a90e890072fdc8773794c4ee4855ac938f9263673cf81ed3

Observation 96696da3-d433-4144-97fb-bfcf696bea53 · inbound

Fermi-LAT Galactic Center Excess morphology of dark matter in simulations of the Milky Way galaxy cites this paper.

Fermi-LAT Galactic Center Excess morphology of dark matter in simulations of the Milky Way galaxy CTA and SWGO can Discover Higgsino Dark Matter Annihilation

Reference 53

Resolution
unresolved
no resolver link, observed 2026-08-05T22:51:59.306497Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-05T22:51:59.306497Z digest=sha256:5755cbe0449756743d5ff2aee8cabc3d206027ffeb952b02968ac602ae230474

Observation 999bf0e1-7509-482d-b8f8-82138e4214be · inbound

Breaking Dark: Hunting Heavy Decaying Dark Matter with Tibet AS$_\gamma$ and LHAASO-KM2A cites this paper.

Breaking Dark: Hunting Heavy Decaying Dark Matter with Tibet AS$_\gamma$ and LHAASO-KM2A CTA and SWGO can Discover Higgsino Dark Matter Annihilation

Reference 111

Resolution
unresolved
no resolver link, observed 2026-08-04T21:29:16.326271Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T21:29:16.326271Z digest=sha256:84be8acee501fba314354a3e68ef3100b08b78849652131f5bab1cb7b9e75825

Observation 36fe7782-d1b0-4913-b65b-e1487961df71 · inbound

Heavy-element paleodetectors for Higgsino dark matter cites this paper.

Heavy-element paleodetectors for Higgsino dark matter CTA and SWGO can Discover Higgsino Dark Matter Annihilation

Reference 21

Resolution
verified exact
arxiv_id, observed 2026-07-02T09:46:50.334339Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-06-28T05:23:17.857704Z digest=sha256:0658f2f38582e65b0806fe5ff2a8a6fa1555a1bb9d650f7b14f7f3b9745f1e5a

Observation d23bb08c-801a-47d3-93e4-c4b37df6de8a · inbound

Accidentally Stable Dark Matter in a Parity Solution to the Strong CP Problem cites this paper.

Accidentally Stable Dark Matter in a Parity Solution to the Strong CP Problem CTA and SWGO can Discover Higgsino Dark Matter Annihilation

Reference 61

Resolution
unresolved
no resolver link, observed 2026-08-01T09:57:12.441465Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T09:57:12.441465Z digest=sha256:146fa082f1ff175bdac2e0068c6b3be50025cbeee529bbd4d7c4f7d719b650cd