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Paper Citation Record · LEDGER

CosmoFlow: Using Deep Learning to Learn the Universe at Scale

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1808.04728.

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

pith.paper-citation-record.v1
1808.04728 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T10:47:27.807503Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-30T15:14:47.283433Z

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 9b68fffb-7c57-4caf-8e9a-4f04dc7583be · inbound

Cosmological parameter estimation from large-scale structure deep learning cites this paper.

Cosmological parameter estimation from large-scale structure deep learning CosmoFlow: Using Deep Learning to Learn the Universe at Scale

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-14T10:47:27.807503Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:47:27.807503Z digest=sha256:d2b02a2c6843c05fab5f3ecbb33f7cd9dca3f07f81abe4d6116b7cd1c386a09b

Observation 1d9f0527-73fc-4a19-9a9a-c88766d20f1b · inbound

Cosmological constraints from neighbor-density-weighted marked correlation functions cites this paper.

Cosmological constraints from neighbor-density-weighted marked correlation functions CosmoFlow: Using Deep Learning to Learn the Universe at Scale

Reference 48

Resolution
verified exact
local_arxiv, observed 2026-05-25T03:30:17.320062Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-05-25T03:27:13.896349Z digest=sha256:1718f24b4a5d75db63f7ef6175e95e884738bbdbdb6d02a18fbc6b20d5454fbc

Observation 4d301c29-360b-4f99-9e69-abc9c0aefb7c · inbound

Cosmological constraints from neighbor-density-weighted marked correlation functions cites this paper.

Cosmological constraints from neighbor-density-weighted marked correlation functions CosmoFlow: Using Deep Learning to Learn the Universe at Scale

Reference 48

Resolution
verified exact
local_arxiv, observed 2026-06-30T15:14:47.284582Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-06-30T15:08:32.960489Z digest=sha256:fd4c80b01306968ad84be8fb28d83e24671755f95869fd38662174c46be1545e