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Paper Citation Record · LEDGER

Evolution of Stellar-to-Halo Mass Ratio at z=0-7 Identified by Clustering Analysis with the Hubble Legacy Imaging and Early Subaru/Hyper Suprime-Cam Survey Data

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1511.07873.

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

pith.paper-citation-record.v1
1511.07873 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-05T06:32:48.257954+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-04T20:10:08.611559Z

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 62c0f801-ac9a-4c26-9c98-5e0058d66009 · inbound

Introducing the Lumina project: large-volume radiation-hydrodynamic simulations of the epochs of hydrogen and helium reionization cites this paper.

Introducing the Lumina project: large-volume radiation-hydrodynamic simulations of the epochs of hydrogen and helium reionization Evolution of Stellar-to-Halo Mass Ratio at z=0-7 Identified by Clustering Analysis with the Hubble Legacy Imaging and Early Subaru/Hyper Suprime-Cam Survey Data

Reference 13

Resolution
verified exact
local_arxiv, observed 2026-05-19T16:17:38.568908Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:f2978fc7c36f541b86b14c48ef2e046289c59e2c6dce8a548608ab338683f2ba

Observation 8dc30a53-15ec-4926-b979-88e24230eec2 · inbound

On the later evolution of observationally selected protocluster candidates at $z\,{\gtrsim}\,5$ cites this paper.

On the later evolution of observationally selected protocluster candidates at $z\,{\gtrsim}\,5$ Evolution of Stellar-to-Halo Mass Ratio at z=0-7 Identified by Clustering Analysis with the Hubble Legacy Imaging and Early Subaru/Hyper Suprime-Cam Survey Data

Reference 288

Resolution
verified exact
local_arxiv, observed 2026-06-26T20:09:57.429174Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:04eb85e74956b2a5dc0b493310fcc1de1fdb0874653ac35d8f28083da88dc842

Observation dae77baf-d648-4e54-8026-f08fe6723fd5 · inbound

Constraining supermassive primordial black hole clustering with the angular auto-correlation of $z\simeq 6$ quasars cites this paper.

Constraining supermassive primordial black hole clustering with the angular auto-correlation of $z\simeq 6$ quasars Evolution of Stellar-to-Halo Mass Ratio at z=0-7 Identified by Clustering Analysis with the Hubble Legacy Imaging and Early Subaru/Hyper Suprime-Cam Survey Data

Reference 88

Resolution
verified exact
local_arxiv, observed 2026-07-04T20:10:08.612989Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=pdf_text observed=2026-06-25T20:34:51.027882Z digest=sha256:9e5f02bb4344f3cd8da8e21fa920a9bce7d4418c3b47a200d66248179ba83a81

Observation d008b99d-97ac-4b7f-ae75-b0c7dac6ac29 · inbound

Tilting at the Turnover: Modeling the Faint-End of the UV Luminosity Function Behind Abell s1063 with JWST cites this paper.

Tilting at the Turnover: Modeling the Faint-End of the UV Luminosity Function Behind Abell s1063 with JWST Evolution of Stellar-to-Halo Mass Ratio at z=0-7 Identified by Clustering Analysis with the Hubble Legacy Imaging and Early Subaru/Hyper Suprime-Cam Survey Data

Reference 196

Resolution
verified exact
local_arxiv, observed 2026-07-02T08:46:48.337565Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:5bedc5b048b992099d1773768410f95b989f88431917846e1cd243173acea318