Paper Citation Record · LEDGER

Exoplanet Occurrence Rates from Microlensing Surveys

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2310.07502.

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

pith.paper-citation-record.v1
2310.07502 v2

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 2026-08-11T06:34:44.6726+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T21:59:47.008958Z

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

3
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 d64af522-5984-4207-bbdf-58743cf0e32f · inbound

Twinkle: A GPU-based binary-lens microlensing code with contour integration method cites this paper.

Twinkle: A GPU-based binary-lens microlensing code with contour integration method Exoplanet Occurrence Rates from Microlensing Surveys

Reference 19

Resolution: malformed identifier; no resolver link, observed 2026-08-10T21:59:47.008958Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ef5e545b-b800-4f86-8e28-eefe4ddd3280 · inbound

Detecting Exomoons in Free-Floating-Planet Events from Space-based Microlensing Surveys cites this paper.

Detecting Exomoons in Free-Floating-Planet Events from Space-based Microlensing Surveys Exoplanet Occurrence Rates from Microlensing Surveys

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-10T21:48:24.626475Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3c9e4d88-e140-4ac3-9b4a-9c4a87809049 · inbound

The SPHERE infrared survey for exoplanets (SHINE). V. Complete observations, data reduction and analysis, detection performances, and final results cites this paper.

The SPHERE infrared survey for exoplanets (SHINE). V. Complete observations, data reduction and analysis, detection performances, and final results Exoplanet Occurrence Rates from Microlensing Surveys

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-10T17:43:18.204041Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a53dc313-bdbb-4625-b5fe-5d90e12908f0 · inbound

Free Floating or Merely Detached? cites this paper.

Free Floating or Merely Detached? Exoplanet Occurrence Rates from Microlensing Surveys

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-06T18:16:28.456654Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2de7f295-f6c7-407a-84e8-b27843801f77 · inbound

Disc Fragmentation. III. The need for a new paradigm for formation of planets within close binary systems cites this paper.

Disc Fragmentation. III. The need for a new paradigm for formation of planets within close binary systems Exoplanet Occurrence Rates from Microlensing Surveys

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-02T19:27:54.442591Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 66d69fac-0b24-46e7-82e0-2172a3aa1294 · inbound

You Shall Not Pass (Without Modeling): High-Resolution Analysis of KMT-2019-BLG-0253 using MORIA cites this paper.

You Shall Not Pass (Without Modeling): High-Resolution Analysis of KMT-2019-BLG-0253 using MORIA Exoplanet Occurrence Rates from Microlensing Surveys

Reference 1

Resolution: metadata mismatch; arxiv_id, observed 2026-05-12T01:16:15.683745Z

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 3278dfea-fdc6-465b-9f1f-72e8fa1ee9ad · inbound

Constraining the Galactic Center Dark Cluster with ELT/MICADO Observations cites this paper.

Constraining the Galactic Center Dark Cluster with ELT/MICADO Observations Exoplanet Occurrence Rates from Microlensing Surveys

Reference 111

Resolution: verified exact; arxiv_id, observed 2026-05-15T02:13:30.508784Z

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.