Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Dark Matter Constraints from Observations of 25 Milky Way Satellite Galaxies with the Fermi Large Area Telescope
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1310.0828.
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 2026-08-11T05:54:27.676178Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-04T11:59:51.378704Z
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 8068c38a-f14b-44fb-b74c-16204bfd3341 · inbound
Prospecting bipartite Dark Matter through Gravitational Waves cites this paper.
Prospecting bipartite Dark Matter through Gravitational Waves Dark Matter Constraints from Observations of 25 Milky Way Satellite Galaxies with the Fermi Large Area Telescope
Reference 126
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T05:54:27.676178Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0a9d6c83-3e62-45c1-869b-41ad8e3c3d7d · inbound
Searching for dark matter annihilating into light long-lived mediators from stars inside dwarf spheroidal galaxies cites this paper.
Searching for dark matter annihilating into light long-lived mediators from stars inside dwarf spheroidal galaxies Dark Matter Constraints from Observations of 25 Milky Way Satellite Galaxies with the Fermi Large Area Telescope
Reference 10
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T21:42:15.120326Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e6ba869f-92f3-422e-abfd-27110e6cf63b · inbound
Detecting dark matter sub-halos in the Galactic plane with the Cherenkov Telescope Array Observatory cites this paper.
Detecting dark matter sub-halos in the Galactic plane with the Cherenkov Telescope Array Observatory Dark Matter Constraints from Observations of 25 Milky Way Satellite Galaxies with the Fermi Large Area Telescope
Reference 27
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:48:57.216635Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 751119df-ca0a-4df2-8dc8-12f1b4db09cf · inbound
Unveiling the inert Triplet desert region with a pNGB Dark Matter and its Gravitational Wave signatures cites this paper.
Unveiling the inert Triplet desert region with a pNGB Dark Matter and its Gravitational Wave signatures Dark Matter Constraints from Observations of 25 Milky Way Satellite Galaxies with the Fermi Large Area Telescope
Reference 23
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T15:04:38.321051Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation db8d2c87-10d5-4090-ac85-e540bfd8ddaf · inbound
A Tentative Double Excess in the Gamma-Ray Spectrum of the Fermi Blazar 4FGL J0604.9-0000 cites this paper.
A Tentative Double Excess in the Gamma-Ray Spectrum of the Fermi Blazar 4FGL J0604.9-0000 Dark Matter Constraints from Observations of 25 Milky Way Satellite Galaxies with the Fermi Large Area Telescope
Reference 32
- Resolution
- verified exact
- local_arxiv, observed 2026-07-04T11:59:51.380466Z
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.