Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Millisecond Pulsars from Accretion Induced Collapse as the Origin of the Galactic Centre Gamma-ray Excess Signal
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2106.00222.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-02T21:27:50.899079Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-14T01:23:34.470385Z
Reference resolution
0 of 0 outbound references displayed
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- 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 a5c3b25c-76bc-4aa4-99a9-499decee0e7a · inbound
Galactic Center gamma-ray excess from a generic triaxial halo cites this paper.
Galactic Center gamma-ray excess from a generic triaxial halo Millisecond Pulsars from Accretion Induced Collapse as the Origin of the Galactic Centre Gamma-ray Excess Signal
Reference 28
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T21:27:50.899079Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e6349608-f601-473f-ae54-f40598175b2b · inbound
Search for TeV emission from spider millisecond pulsars with HAWC cites this paper.
Search for TeV emission from spider millisecond pulsars with HAWC Millisecond Pulsars from Accretion Induced Collapse as the Origin of the Galactic Centre Gamma-ray Excess Signal
Reference 51
- Resolution
- verified exact
- arxiv_id, observed 2026-05-14T01:23:34.482306Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation dc9a8ff7-d7d5-457c-b396-73c104221401 · inbound
LHC Mono-$W/Z$ Signatures as a Probe for Dark Matter Explanations of Astrophysical Excesses cites this paper.
LHC Mono-$W/Z$ Signatures as a Probe for Dark Matter Explanations of Astrophysical Excesses Millisecond Pulsars from Accretion Induced Collapse as the Origin of the Galactic Centre Gamma-ray Excess Signal
Reference 14
- Resolution
- verified exact
- arxiv_id, observed 2026-05-11T01:40:52.494988Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 96e9f7c0-3dd5-4bc6-9267-070abcb04226 · inbound
Spirited Away: Advective Loss of Cosmic Rays into the Milky Way's Circumgalactic Medium Explains the Large Magellanic Cloud's Low Gamma-ray Luminosity cites this paper.
Spirited Away: Advective Loss of Cosmic Rays into the Milky Way's Circumgalactic Medium Explains the Large Magellanic Cloud's Low Gamma-ray Luminosity Millisecond Pulsars from Accretion Induced Collapse as the Origin of the Galactic Centre Gamma-ray Excess Signal
Reference 78
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T07:56:16.199903Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.