Pith. sign in

Paper Citation Record · LEDGER

The dependence of dark matter profiles on the stellar to halo mass ratio: a prediction for cusps vs cores

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:1306.0898.

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

pith.paper-citation-record.v1
1306.0898 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T22:14:25.482998Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-01T02:45:18.196955Z

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 621b7e36-76a6-4943-aee0-34f5c9a23239 · inbound

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps cites this paper.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps The dependence of dark matter profiles on the stellar to halo mass ratio: a prediction for cusps vs cores

Reference 39

Resolution
unresolved
no resolver link, observed 2026-08-04T22:14:25.482998Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T22:14:25.482998Z digest=sha256:35a68394944a73ffd388ce70d3754db3f66b422c225f46cf6321aa69b21e270a

Observation c11e4b63-a276-4a6f-964b-97435f15410f · inbound

It's Not Just Star Formation: A trend of low dark matter densities in the Andromeda dwarf galaxy system cites this paper.

It's Not Just Star Formation: A trend of low dark matter densities in the Andromeda dwarf galaxy system The dependence of dark matter profiles on the stellar to halo mass ratio: a prediction for cusps vs cores

Reference 122

Resolution
verified exact
local_arxiv, observed 2026-06-28T21:32:38.621618Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:266f77184fef87808a16a869a52659da4361ef26c13e9af2430d94ac2ac96738

Observation 30531ebc-dc69-4a16-815d-929b080f0e9b · inbound

Dark Matter in Draco and Bo\"otes I: Hints of a Core in an Ultra-Faint Dwarf from Simulation-Based Inference cites this paper.

Dark Matter in Draco and Bo\"otes I: Hints of a Core in an Ultra-Faint Dwarf from Simulation-Based Inference The dependence of dark matter profiles on the stellar to halo mass ratio: a prediction for cusps vs cores

Reference 180

Resolution
verified exact
local_arxiv, observed 2026-06-26T02:08:55.071299Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:832911f77d8b46aaedb1b7150ca74f6a60ad9d39faa96f7e778dae1c1c80c97c

Observation 35c12de0-8cd3-4424-8071-b419380e284e · inbound

The Bright Future of the Dark and Dim Universe cites this paper.

The Bright Future of the Dark and Dim Universe The dependence of dark matter profiles on the stellar to halo mass ratio: a prediction for cusps vs cores

Reference 141

Resolution
verified exact
local_arxiv, observed 2026-06-29T01:52:58.582347Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:f652c7ba78a586d544bdf19bc093855b7bc8629c190e06d87e9207ec5d7a452d

Observation 95a503fb-6a01-4778-906b-2bcd98a89179 · inbound

Global trends in morphology from massive to dwarf galaxies cites this paper.

Global trends in morphology from massive to dwarf galaxies The dependence of dark matter profiles on the stellar to halo mass ratio: a prediction for cusps vs cores

Reference 297

Resolution
verified exact
local_arxiv, observed 2026-07-01T02:45:18.199969Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:6f5906069fe73683045c24e5572eafa707c6b155ff93bfb266ba74ac8fee64ab

Observation b594c65d-7bde-4cba-887c-5eaebfd65b6a · inbound

Constraints on the population level distribution of nearby Dark Matter halo shapes with extragalactic streams cites this paper.

Constraints on the population level distribution of nearby Dark Matter halo shapes with extragalactic streams The dependence of dark matter profiles on the stellar to halo mass ratio: a prediction for cusps vs cores

Reference 119

Resolution
unresolved
no resolver link, observed 2026-07-11T06:35:48.157333Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T06:35:48.157333Z digest=sha256:b7a925c9199076e912e8d216900e286a1e487a2f8bf1d9c96d8c9636c54f189f

Observation b11c3b18-3160-4f37-95eb-6dbef3747fbf · inbound

Dark matter density profiles of the Milky Way satellite population: reconciling simulations and observations cites this paper.

Dark matter density profiles of the Milky Way satellite population: reconciling simulations and observations The dependence of dark matter profiles on the stellar to halo mass ratio: a prediction for cusps vs cores

Reference 6

Resolution
unresolved
no resolver link, observed 2026-07-13T06:28:17.325404Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-13T06:28:17.325404Z digest=sha256:614d68981bdeacefcdbad5c7d04a516a04c275eb575aa00061769c0068a6290e

Observation abad568f-841f-4dc4-bd18-95ec9b0b3861 · inbound

Dynamical flattening of halo density cusps by Q-ball dark matter cites this paper.

Dynamical flattening of halo density cusps by Q-ball dark matter The dependence of dark matter profiles on the stellar to halo mass ratio: a prediction for cusps vs cores

Reference 15

Resolution
unresolved
no resolver link, observed 2026-07-31T04:54:06.761605Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-31T04:54:06.761605Z digest=sha256:a93d0f99af9165de0b40cab52daf82c36abdd10d07f3b0bd293d09a533b23118