Pith. sign in

Paper Citation Record · LEDGER

Connecting substellar and stellar formation. The role of the host star's metallicity

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:1903.01141.

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

pith.paper-citation-record.v1
1903.01141 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 2026-08-15T06:32:42.880941+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T19:34:24.195553Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-03T18:58:50.189491Z

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 227c5baf-b47f-4d5a-a778-ecdba7f36a8f · inbound

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? cites this paper.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? Connecting substellar and stellar formation. The role of the host star's metallicity

Reference 22

Resolution
unresolved
no resolver link, observed 2026-08-11T19:34:24.195553Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T19:34:24.195553Z digest=sha256:b0f541d665ec63846704d53488b3917ac629a487d89b98dea5475b7c60805eeb

Observation 3dc89983-a641-454d-8134-86198453a55c · inbound

CORALIE radial-velocity search for companions around evolved stars (CASCADES) V. Three planetary companions and achievable precision cites this paper.

CORALIE radial-velocity search for companions around evolved stars (CASCADES) V. Three planetary companions and achievable precision Connecting substellar and stellar formation. The role of the host star's metallicity

Reference 142

Resolution
verified exact
local_arxiv, observed 2026-06-27T15:10:59.119292Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:b266c8f3514cfe31370b48d4bb7fa04641a384cb13de6697a7a21789882fb2ef

Observation b1f470e1-c58d-45f7-a010-11bf9acc229e · inbound

Understanding eccentric temperate giants: an in-depth study of the architecture and stellar obliquity of the TOI-2134 system cites this paper.

Understanding eccentric temperate giants: an in-depth study of the architecture and stellar obliquity of the TOI-2134 system Connecting substellar and stellar formation. The role of the host star's metallicity

Reference 168

Resolution
verified exact
local_arxiv, observed 2026-07-02T05:26:39.319355Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:07adffc89474acf5890bfa0626f6caebfb46ed18de469632c25bdfaacf2662e4

Observation 8ef5e5ac-4763-47aa-b4a9-9ba791d117cc · inbound

Understanding eccentric temperate giants: an in-depth study of the architecture and stellar obliquity of the TOI-2134 system cites this paper.

Understanding eccentric temperate giants: an in-depth study of the architecture and stellar obliquity of the TOI-2134 system Connecting substellar and stellar formation. The role of the host star's metallicity

Reference 168

Resolution
verified exact
local_arxiv, observed 2026-07-03T18:58:50.191143Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:42a9e613d046fa894c0c5794a587f9e18ed6ec4fa68b8773cc5c1b442458b8b9

Observation b5e42a6a-2059-4a72-83d2-1aaca0b6ebfb · inbound

Understanding eccentric temperate giants: an in-depth study of the architecture and stellar obliquity of the TOI-2134 system cites this paper.

Understanding eccentric temperate giants: an in-depth study of the architecture and stellar obliquity of the TOI-2134 system Connecting substellar and stellar formation. The role of the host star's metallicity

Reference 168

Resolution
unresolved
no resolver link, observed 2026-07-12T09:03:32.977007Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-12T09:03:32.977007Z digest=sha256:b7637d843a8b0bd4e7390d3590c56b16285e68ecf4b41353c0e60aecb0c2e8be

Observation f6156d2a-51d2-4261-9878-708b8cdfb3e7 · 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 Connecting substellar and stellar formation. The role of the host star's metallicity

Reference 234

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=sha256:5bf49efc639afff48619e99a06c1c6154ad2a9803f8ea0dec24d08d205837628

Observation 6d404ca6-9226-48cd-a9cd-970d33e49905 · 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 Connecting substellar and stellar formation. The role of the host star's metallicity

Reference 234

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=sha256:7d975600cf0985025d4c83bba8cd41ab78dadb6552f576289b29066d0e85ff44