Pith. sign in

Paper Citation Record · LEDGER

Introducing the BRAHMA simulation suite: Signatures of low mass black hole seeding models in cosmological simulations

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2402.03626.

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

pith.paper-citation-record.v1
2402.03626 v1

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 2026-08-09T06:31:02.800959+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T20:32:19.053888Z

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

2
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 0fdbb190-b8eb-41d7-b08f-c51671d6c169 · inbound

A prevalent population of normal-mass central black holes in high-redshift massive galaxies cites this paper.

A prevalent population of normal-mass central black holes in high-redshift massive galaxies Introducing the BRAHMA simulation suite: Signatures of low mass black hole seeding models in cosmological simulations

Reference 20

Resolution
unresolved
no resolver link, observed 2026-08-08T20:32:19.053888Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T20:32:19.053888Z digest=sha256:f2e614bd93b245488ef8d06e7f88a897a95b4aeb14062e440a190f1ae436743a

Observation 39a83a12-5b75-4084-a525-69c2fe559da3 · inbound

Black Hole Binary Detection Landscape for the Laser Interferometer Lunar Antenna (LILA): Signal-to-Noise Calculations & Science Cases cites this paper.

Black Hole Binary Detection Landscape for the Laser Interferometer Lunar Antenna (LILA): Signal-to-Noise Calculations & Science Cases Introducing the BRAHMA simulation suite: Signatures of low mass black hole seeding models in cosmological simulations

Reference 38

Resolution
verified exact
arxiv_id, observed 2026-05-13T01:37:02.328884Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-05-13T01:34:08.111553Z digest=sha256:201e58d3df5b86624da41faf446874b66e68cb44d4ed6eecd89fb7041a5b656d