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Paper Citation Record · LEDGER

Milky Way Satellite Census. I. The Observational Selection Function for Milky Way Satellites in DES Y3 and Pan-STARRS DR1

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1912.03302.

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

pith.paper-citation-record.v1
1912.03302 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 2026-08-04T06:34:03.388597+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T09:11:22.400584Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-19T04:32:03.273499Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • parse uncertain0
  • malformed identifier0
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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 e28ffdd5-b52a-4f22-95c5-14cfa6d92769 · inbound

GeV-scale thermal dark matter from dark photons: tightly constrained, yet allowed cites this paper.

GeV-scale thermal dark matter from dark photons: tightly constrained, yet allowed Milky Way Satellite Census. I. The Observational Selection Function for Milky Way Satellites in DES Y3 and Pan-STARRS DR1

Reference 102

Resolution
verified exact
arxiv_id, observed 2026-05-19T04:32:03.275466Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=pdf_text observed=2026-05-19T04:31:05.784625Z digest=sha256:7e3f7a40961292a5260f59b7d6fa7a169a2d0bcf0f3325c5ac3c1e62ee9e5667

Observation 0a9935fe-22c7-4428-bc60-5c384e504b2f · inbound

A lower bound on primordial power spectrum from halo substructure cites this paper.

A lower bound on primordial power spectrum from halo substructure Milky Way Satellite Census. I. The Observational Selection Function for Milky Way Satellites in DES Y3 and Pan-STARRS DR1

Reference 1

Resolution
unresolved
no resolver link, observed 2026-08-01T09:11:22.400584Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T09:11:22.400584Z digest=sha256:2e5c5fa426ba5370be3d2dbc0e132248ca589438fe09e57a687d4b22cf7fd2de