Paper Citation Record · LEDGER

Ingredients for 21cm intensity mapping

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 14 inbound Pith citation observations for arXiv:1804.09180.

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

pith.paper-citation-record.v1
1804.09180 v1

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measured 0 of 0 reference resolution

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measured 14 of 14 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00

measured 14 of 14 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T20:15:39.596818Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T17:37:25.968182Z

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 545b95c3-0ba2-49c7-8bde-598f8f50aad8 · inbound

Realistic simulations of galaxy formation in f(R) modified gravity cites this paper.

Realistic simulations of galaxy formation in f(R) modified gravity Ingredients for 21cm intensity mapping

Reference 45

Resolution: verified exact; local_arxiv, observed 2026-05-25T02:00:12.378703Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation bd580b08-b21e-48ef-a602-609abc3da737 · inbound

Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies cites this paper.

Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies Ingredients for 21cm intensity mapping

Reference 188

Resolution: verified exact; local_arxiv, observed 2026-05-14T19:42:53.421180Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation bd2f2197-b52c-4596-abdd-ff4b869f5308 · inbound

JERALD: high-fidelity dark matter, stellar mass and neutral hydrogen maps from fast N-body simulations cites this paper.

JERALD: high-fidelity dark matter, stellar mass and neutral hydrogen maps from fast N-body simulations Ingredients for 21cm intensity mapping

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-10T20:15:39.596818Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2b5a1eba-424d-4fdf-b424-b752bb6dba12 · inbound

Seeing Wiggles without Seeing Wiggles: BAO Recovery in 21 cm Intensity Mapping with Deep Learning cites this paper.

Seeing Wiggles without Seeing Wiggles: BAO Recovery in 21 cm Intensity Mapping with Deep Learning Ingredients for 21cm intensity mapping

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-03T05:10:22.514133Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8d44db70-2b90-405a-93d6-d7dc4845a448 · inbound

Using SKAO to Understand the Clustering of Gravitational Wave Sources cites this paper.

Using SKAO to Understand the Clustering of Gravitational Wave Sources Ingredients for 21cm intensity mapping

Reference 34

Resolution: metadata mismatch; local_arxiv, observed 2026-06-25T23:08:41.248789Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation ef20f847-7c6a-42da-b531-c1db12552ed3 · inbound

Cosmological Galaxy Formation Modelling in the Era of the Square Kilometre Array cites this paper.

Cosmological Galaxy Formation Modelling in the Era of the Square Kilometre Array Ingredients for 21cm intensity mapping

Reference 56

Resolution: verified exact; local_arxiv, observed 2026-06-25T21:38:29.108045Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 527e839c-9e3c-40ea-951f-317e8b0e7fea · inbound

HI Simulations for Cosmology with the SKA Observatory cites this paper.

HI Simulations for Cosmology with the SKA Observatory Ingredients for 21cm intensity mapping

Reference 127

Resolution: verified exact; local_arxiv, observed 2026-06-25T19:58:18.127115Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 817ca8d8-be03-4347-abfa-6e4c31647fac · inbound

Cosmology with Multi-Wavelength Line Intensity Mapping Synergies in the SKAO Era cites this paper.

Cosmology with Multi-Wavelength Line Intensity Mapping Synergies in the SKAO Era Ingredients for 21cm intensity mapping

Reference 7

Resolution: verified exact; local_arxiv, observed 2026-06-30T05:14:18.011287Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 462bb594-71b7-47d5-9044-5a961878005c · inbound

Cosmology with HI Intensity Mapping cites this paper.

Cosmology with HI Intensity Mapping Ingredients for 21cm intensity mapping

Reference 31

Resolution: unresolved; no resolver link, observed 2026-07-12T03:43:52.393274Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 84120805-890d-40d8-aef0-a4eca7825c23 · inbound

Weak Evolution of Cosmic Atomic Hydrogen over the Past 4.5 Billion Years cites this paper.

Weak Evolution of Cosmic Atomic Hydrogen over the Past 4.5 Billion Years Ingredients for 21cm intensity mapping

Reference 37

Resolution: metadata mismatch; local_arxiv, observed 2026-07-07T17:24:00.718450Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 95d22434-3e28-4230-bf32-54b4fcdba2a4 · inbound

Intensity fluctuations of radio halo in galaxy cluster: Insights from power spectrum estimation cites this paper.

Intensity fluctuations of radio halo in galaxy cluster: Insights from power spectrum estimation Ingredients for 21cm intensity mapping

Reference 262

Resolution: verified exact; local_arxiv, observed 2026-07-10T17:37:25.969755Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation a2e6ed0d-0763-4091-8b58-83aa5b63f6cb · inbound

Fast(er)PM and Moving Mesh: JAX-native Geometric Multigrid Methods cites this paper.

Fast(er)PM and Moving Mesh: JAX-native Geometric Multigrid Methods Ingredients for 21cm intensity mapping

Reference 187

Resolution: unresolved; no resolver link, observed 2026-07-14T07:52:28.510358Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cbce1319-303d-43ef-ab88-0d4bf1add9ad · inbound

Simulation-Based Priors for HI Bias from Halo Occupation Physics cites this paper.

Simulation-Based Priors for HI Bias from Halo Occupation Physics Ingredients for 21cm intensity mapping

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-02T02:52:37.926234Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7fce7317-5902-48f0-a84d-2e57df4116ad · inbound

Modeling the HI-Halo Connection: Evolution, Scatter, and a Halo-based Prescription for 21-cm Mock Catalogs cites this paper.

Modeling the HI-Halo Connection: Evolution, Scatter, and a Halo-based Prescription for 21-cm Mock Catalogs Ingredients for 21cm intensity mapping

Reference 128

Resolution: unresolved; no resolver link, observed 2026-08-01T10:48:44.863947Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.