Pith. sign in

Paper Citation Record · LEDGER

Planet Occurrence within 0.25 AU of Solar-type Stars from Kepler

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:1103.2541.

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

pith.paper-citation-record.v1
1103.2541 v1

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 2026-08-05T06:32:48.257954+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T05:36:56.798482Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-02T05:46:40.545995Z

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 206ffdb7-572f-4f8c-9210-82874c115da4 · inbound

The Maximum Density of a Collisionally-Produced Planet is A Function of its Mass and Orbital Period cites this paper.

The Maximum Density of a Collisionally-Produced Planet is A Function of its Mass and Orbital Period Planet Occurrence within 0.25 AU of Solar-type Stars from Kepler

Reference 25

Resolution
verified exact
local_arxiv, observed 2026-06-26T22:40:09.991749Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:ba96906b39eeed13dafed5774add1ee05cdaa089182521f5a32cba19d648bb9b

Observation c8519a11-88ad-458e-a21e-d7c0ef4ab862 · inbound

Chemical Abundances of the Bioessential Elements C, O and S, and the Refractory Elements Fe and Ni, in Solar-type Exoplanet-hosting Stars from HARPS North and South cites this paper.

Chemical Abundances of the Bioessential Elements C, O and S, and the Refractory Elements Fe and Ni, in Solar-type Exoplanet-hosting Stars from HARPS North and South Planet Occurrence within 0.25 AU of Solar-type Stars from Kepler

Reference 238

Resolution
verified exact
local_arxiv, observed 2026-07-01T01:55:14.372778Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:9a217ca519eda14bc8e50745041a4843903eec56049c589648353c4e58466f48

Observation ed43470a-c303-4d69-806f-18d97aa0f967 · inbound

The Mid-Infrared Transmission Spectrum of the Temperate Sub-Neptune TOI-270 d cites this paper.

The Mid-Infrared Transmission Spectrum of the Temperate Sub-Neptune TOI-270 d Planet Occurrence within 0.25 AU of Solar-type Stars from Kepler

Reference 240

Resolution
verified exact
local_arxiv, observed 2026-07-02T05:46:40.547427Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:99d43f60a0b22258206e5e98b1d33a8f565eef74a33932c739c153ddeb2bd172

Observation 3c3d9cea-ad65-4f9c-b72f-a55049a90907 · inbound

The GAPS Programme with HARPS-N at TNG LXXVII. Occurrence rates of small close-in planets in the presence of cold Jupiters cites this paper.

The GAPS Programme with HARPS-N at TNG LXXVII. Occurrence rates of small close-in planets in the presence of cold Jupiters Planet Occurrence within 0.25 AU of Solar-type Stars from Kepler

Reference 257

Resolution
unresolved
no resolver link, observed 2026-07-13T03:54:36.358098Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-13T03:54:36.358098Z digest=sha256:065b41436b921140cee28be20f488d12180a0cc4befb6fbdc9c3256bc15da6a6

Observation 49d718a2-cd15-47f7-b152-2a1c1e44fc3d · inbound

The GAPS Programme with HARPS-N at TNG LXXVII. Occurrence rates of small close-in planets in the presence of cold Jupiters cites this paper.

The GAPS Programme with HARPS-N at TNG LXXVII. Occurrence rates of small close-in planets in the presence of cold Jupiters Planet Occurrence within 0.25 AU of Solar-type Stars from Kepler

Reference 257

Resolution
unresolved
no resolver link, observed 2026-07-14T15:15:28.911413Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T15:15:28.911413Z digest=sha256:d11344fcd5d66b541c57a9589177e061c20c33c53c7096325c59bfa1adc75a54

Observation 83cfa778-cf18-4565-a271-befcea282460 · inbound

HD 148797: A bright F-type star with two moderate-period low-density sub-Jovian planets. Compact multi-planet architectures are common in the Neptunian savanna cites this paper.

HD 148797: A bright F-type star with two moderate-period low-density sub-Jovian planets. Compact multi-planet architectures are common in the Neptunian savanna Planet Occurrence within 0.25 AU of Solar-type Stars from Kepler

Reference 202

Resolution
unresolved
no resolver link, observed 2026-07-13T01:25:33.763066Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-13T01:25:33.763066Z digest=sha256:e4e478f8cd251d2f875f89b5189dddf19dd22a3de539cb4c7aab395a58de7474

Observation e0084f19-45e6-4868-b78e-829ee6975e48 · inbound

Revisiting TOI-4438 and TOI-442 planetary systems with new observations from SPIRou and TESS cites this paper.

Revisiting TOI-4438 and TOI-442 planetary systems with new observations from SPIRou and TESS Planet Occurrence within 0.25 AU of Solar-type Stars from Kepler

Reference 247

Resolution
unresolved
no resolver link, observed 2026-08-02T05:36:56.798482Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T05:36:56.798482Z digest=sha256:690cff26cd3dd8d2305d2f267198057e29ad709dbd549c83155fb612c5abd6ca