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Paper Citation Record · LEDGER

Is Quasar Optical Variability a Damped Random Walk?

As of 2 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:1202.3783.

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

pith.paper-citation-record.v1
1202.3783 v2

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 2026-08-02T06:30:47.504484+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T21:02:28.437831Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-01T15:35:47.927620Z

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 496af014-2b73-457c-9718-97cb1cf6b3ac · inbound

Constraining Orbital Eccentricity of a Supermassive Black Hole Binary Candidate PKS 2131-0211 cites this paper.

Constraining Orbital Eccentricity of a Supermassive Black Hole Binary Candidate PKS 2131-0211 Is Quasar Optical Variability a Damped Random Walk?

Reference 1

Resolution
verified exact
local_arxiv, observed 2026-06-28T04:41:39.618833Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-02T06:30:47.504484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:9f574e76fa4b113801c140fb06430480ba0435adfaf08c04bab786020e92c051

Observation aca6ec06-9b1f-423f-85cd-2c2ec028f8ac · inbound

A Disappearing Act: Constraints From "Missing" Flares of Repeating Partial TDE Candidates cites this paper.

A Disappearing Act: Constraints From "Missing" Flares of Repeating Partial TDE Candidates Is Quasar Optical Variability a Damped Random Walk?

Reference 298

Resolution
verified exact
local_arxiv, observed 2026-06-28T02:01:29.575322Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-02T06:30:47.504484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:274dbe5ac5c794f330b1c728c42f37d417d8d59404157f82dea9d11f022b79c5

Observation daf31f1b-ea08-4934-b4e6-fe1651e9b4ab · inbound

Reverberation in the Narrow Fe K${\alpha}$ Line in the Seyfert Galaxy NGC 4151 with XRISM cites this paper.

Reverberation in the Narrow Fe K${\alpha}$ Line in the Seyfert Galaxy NGC 4151 with XRISM Is Quasar Optical Variability a Damped Random Walk?

Reference 21

Resolution
verified exact
local_arxiv, observed 2026-06-26T14:59:32.559693Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-02T06:30:47.504484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:88db5a41b79a21cb5ff4cc8b113d7dda9277d81ecf4e9c2a5cd3d04b14effd99

Observation 4c7aabdb-0d11-41b6-8db0-f28e67b5ef97 · inbound

Validating the ICCF-Cut Method with Simultaneous Photometric and Spectroscopic H$\alpha$ Reverberation Mapping of NGC 4151 and UGC 3374 cites this paper.

Validating the ICCF-Cut Method with Simultaneous Photometric and Spectroscopic H$\alpha$ Reverberation Mapping of NGC 4151 and UGC 3374 Is Quasar Optical Variability a Damped Random Walk?

Reference 38

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verified exact
local_arxiv, observed 2026-06-26T05:38:59.760926Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-02T06:30:47.504484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:7d46b86befc3e51692a7cb19e750abaff2ba8a6be31f27185e4d615ae5ee0500

Observation 4da763bb-c4b0-492d-bc41-a291628376b0 · inbound

HALO II: Constraining Hubble constant $H_{0}$ through continuum delay fitting of Fairall 9 cites this paper.

HALO II: Constraining Hubble constant $H_{0}$ through continuum delay fitting of Fairall 9 Is Quasar Optical Variability a Damped Random Walk?

Reference 254

Resolution
verified exact
local_arxiv, observed 2026-06-26T05:59:03.839845Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-02T06:30:47.504484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:3f37c8a4893944369565adff76dff2b6588e7d0b5b3f079c0677af18c7cf3841

Observation 8fd4735d-ddb6-4f00-92bf-bd8a7c54ec8b · inbound

A hierarchical Bayesian framework for cosmology using Type 1 AGN variability cites this paper.

A hierarchical Bayesian framework for cosmology using Type 1 AGN variability Is Quasar Optical Variability a Damped Random Walk?

Reference 45

Resolution
verified exact
local_arxiv, observed 2026-07-01T15:35:47.928939Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-02T06:30:47.504484+00:00.

source=pdf_text observed=2026-06-30T01:21:18.798989Z digest=sha256:3bb79d637454790b3ee6ba01e01ea2acdad4fb6a77e8d1812c08954def8cb8f8

Observation 8485c59d-d249-470b-8ad2-22fb12aa2237 · inbound

VAR-PZnn: A machine-learning framework for AGN photometric redshifts using color and variability-based features cites this paper.

VAR-PZnn: A machine-learning framework for AGN photometric redshifts using color and variability-based features Is Quasar Optical Variability a Damped Random Walk?

Reference 117

Resolution
unresolved
no resolver link, observed 2026-08-01T21:02:28.437831Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T21:02:28.437831Z digest=sha256:f37ee2d17aa274408d91232f103ef6e01746223304996ce163af81fc82bf5b53