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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 15 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

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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 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=sha256:1d5d5c4e3ae8adef360e678677a37fd46c54476ff24c806c8e6681faa0443adb

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.

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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.

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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:b1116c5dec180f4c9019a2c619c6a0e51b7e64c8c3063466efb19a7d4d52a13d

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:ba2876ecea423383db1c48e2528cbfccce2abc9d355daf0ed576afb01200166f

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:a4eaf36ba6adf6041c9a2497b2dbe0a5635a9f421cdb4bf6f2257c3b15da3156

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:e8f8140c133e985aa6bd81779f74d327013a2526633c05307d291f3ddc92551c

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=sha256:58301c78e6c4addf7d3a5b0abdbec1630b98159ede7c856606fbc9518e23f42f