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Paper Citation Record · LEDGER

Modeling Asteroseismic Yields for the Roman Galactic Bulge Time-Domain Survey

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2503.04999.

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

pith.paper-citation-record.v1
2503.04999 v3

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 2026-07-31T16:17:45.563384Z

measured 1 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

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

External citation measurements

0
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 4e99506e-267f-4264-84ab-6801dd88095f · inbound

Evaluating the Sensitivity of the Age Inferences of Red Giant Stars to Machine Learning Methodology cites this paper.

Evaluating the Sensitivity of the Age Inferences of Red Giant Stars to Machine Learning Methodology Modeling Asteroseismic Yields for the Roman Galactic Bulge Time-Domain Survey

Reference 129

Resolution
verified exact
arxiv_id, observed 2026-06-25T22:48:38.628841Z

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=2026-06-25T22:44:31.023366Z digest=sha256:79e12bcfb4bc54d2a9e4839250f441b7bb75cded1275f9d23f74647ddf73fd76

Observation 57f41376-7cd4-44e6-bc0d-0cf5f5a6f87c · inbound

Detecting Solar-Like Oscillations in the Highest Mass TESS Giants cites this paper.

Detecting Solar-Like Oscillations in the Highest Mass TESS Giants Modeling Asteroseismic Yields for the Roman Galactic Bulge Time-Domain Survey

Reference 67

Resolution
unresolved
no resolver link, observed 2026-07-31T16:17:45.563384Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-31T16:17:45.563384Z digest=sha256:7cd697f59276a59e241d1af76be2f905d3bf6f9b554b78900a1ff672dde5a398