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Paper Citation Record · LEDGER

Dependence of Planet populations on Stellar Mass and Metallicity: A Pebble Accretion-based Planet Population Synthesis

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2504.00296.

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

pith.paper-citation-record.v1
2504.00296 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-13T06:32:02.005865+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T20:02:12.462724Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-12T06:48:34.072727Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • 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 ddeb2cc5-08d5-4a5f-ad97-7262ad954fc5 · inbound

Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods cites this paper.

Metallicities of M Dwarf Planet Host Stars from Kepler, K2, and TESS observed by APOGEE: Trends with Exoplanetary Radii and Orbital Periods Dependence of Planet populations on Stellar Mass and Metallicity: A Pebble Accretion-based Planet Population Synthesis

Reference 56

Resolution
unresolved
no resolver link, observed 2026-08-06T20:02:12.462724Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T20:02:12.462724Z digest=sha256:b5c0cde6809f74c1a6ad654fea6459b43c40ae7e108d7ef9de18ac5e44426e15

Observation 9f18c6d7-f30e-4ad0-bc16-48827dfff437 · inbound

Uniform Metallicity Measurements of M Dwarf Planet Hosts Support Metallicity-Dependent Sub-Neptune Formation cites this paper.

Uniform Metallicity Measurements of M Dwarf Planet Hosts Support Metallicity-Dependent Sub-Neptune Formation Dependence of Planet populations on Stellar Mass and Metallicity: A Pebble Accretion-based Planet Population Synthesis

Reference 256

Resolution
verified exact
local_arxiv, observed 2026-07-12T06:48:34.074454Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=arxiv_source observed=2026-07-12T06:44:30.209178Z digest=sha256:7c53b5eb25fbe8afdc47bfdfbc6779d3c7e4f71d5020a308efa0a5d53440693e

Observation 400f2453-b0bd-4b4e-8ff5-51ffe057abdd · inbound

The Influence of Dust Composition on Accretion Outbursts cites this paper.

The Influence of Dust Composition on Accretion Outbursts Dependence of Planet populations on Stellar Mass and Metallicity: A Pebble Accretion-based Planet Population Synthesis

Reference 202

Resolution
unresolved
no resolver link, observed 2026-08-01T02:12:13.133780Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T02:12:13.133780Z digest=sha256:03b21d9d2a9e1eb6f8ac8256c4b680023c0ca8407e90e041eac9c78268377b85