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Paper Citation Record · LEDGER

Marked correlations in galaxy formation models

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:astro-ph/0511773.

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

pith.paper-citation-record.v1
astro-ph/0511773 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 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 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T16:55:30.269135Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-22T18:56:57.994505Z

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 352a23d9-7b7a-4bfe-9042-902838fd38e1 · inbound

Tomographic Alcock-Paczynski Test with Marked Correlation Functions cites this paper.

Tomographic Alcock-Paczynski Test with Marked Correlation Functions Marked correlations in galaxy formation models

Reference 34

Resolution
verified exact
local_arxiv, observed 2026-05-22T18:56:57.997840Z

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=2026-05-22T18:56:46.117021Z digest=sha256:a5c3e5144b82443a6e888927238a7b8aa19c43f439955ee21b3451e106a7b33c

Observation 2eff2671-30c3-4b25-b4e3-f14a169516fc · inbound

First Constraints from Marked Angular Power Spectra with Subaru Hyper Suprime-Cam Survey First-Year Data cites this paper.

First Constraints from Marked Angular Power Spectra with Subaru Hyper Suprime-Cam Survey First-Year Data Marked correlations in galaxy formation models

Reference 60

Resolution
unresolved
no resolver link, observed 2026-08-06T16:55:30.269135Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T16:55:30.269135Z digest=sha256:fbb60c08fd2879a722d4e52bb2d5f30d4d73570463c13470df278bc9d2f90575

Observation 3dda3c80-150f-45c7-89ae-e5e603a8d23c · inbound

Non-conservation and time non-locality of biased tracers cites this paper.

Non-conservation and time non-locality of biased tracers Marked correlations in galaxy formation models

Reference 164

Resolution
metadata mismatch
arxiv_id, observed 2026-05-11T18:11:05.321456Z

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=arxiv_source observed=2026-05-08T16:32:11.394394Z digest=sha256:b8e2561405dad08ffed4ddd8849455a9005054d8fd4230920453f1a3f31c9b7e

Observation 84ba9938-e563-4b32-8362-662382ecd4da · inbound

Probing Reionization up to the Mark: The Marked Power Spectrum to unveil the HI 21-cm signal from the EoR cites this paper.

Probing Reionization up to the Mark: The Marked Power Spectrum to unveil the HI 21-cm signal from the EoR Marked correlations in galaxy formation models

Reference 45

Resolution
verified exact
local_arxiv, observed 2026-05-20T00:22:53.953341Z

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=2026-05-20T00:18:13.785838Z digest=sha256:fcaa761e7e1c7d552cfba4185fdf21f7c26e8fc6a6423c0bdcd92075f275b846

Observation a954d515-9310-4783-b1f2-d63fc0f03163 · inbound

Assembly bias from nuisance to probe I: the relation between galactic conformity and the linear matter clustering cites this paper.

Assembly bias from nuisance to probe I: the relation between galactic conformity and the linear matter clustering Marked correlations in galaxy formation models

Reference 21

Resolution
unresolved
no resolver link, observed 2026-07-11T22:15:18.223338Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-11T22:15:18.223338Z digest=sha256:baa9a36ef564191e6663612c69029b9b48eac7c40c01369ec4f5ed2072a86ec2

Observation f4506b4a-637a-4182-8113-f6689c9c4cf4 · inbound

Assembly bias from nuisance to probe I: the relation between galactic conformity and the linear matter clustering cites this paper.

Assembly bias from nuisance to probe I: the relation between galactic conformity and the linear matter clustering Marked correlations in galaxy formation models

Reference 21

Resolution
unresolved
no resolver link, observed 2026-08-02T08:48:14.634105Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T08:48:14.634105Z digest=sha256:d7c8dfe4cbdd4153ab87a8a4bbf6d609419fed237ad93079c03cb68dd30f27b2