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Paper Citation Record · LEDGER

The infrared-radio correlation of star-forming galaxies is strongly M$_{\star}$-dependent but nearly redshift-invariant since z$\sim$4

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2010.05510.

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

pith.paper-citation-record.v1
2010.05510 v2

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 2026-08-18T06:34:40.430872+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-14T16:07:11.412748Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T17:27:26.410724Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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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 2264661f-3dc3-4201-80f5-f1b6eb3243d4 · inbound

A MIGHTEE robust measurement of the star formation rate-radio correlation cites this paper.

A MIGHTEE robust measurement of the star formation rate-radio correlation The infrared-radio correlation of star-forming galaxies is strongly M$_{\star}$-dependent but nearly redshift-invariant since z$\sim$4

Reference 59

Resolution
unresolved
no resolver link, observed 2026-07-12T01:44:24.704352Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-12T01:44:24.704352Z digest=sha256:683a58c4b264a930f2537ebf3173e7b1e7d7418cc9307156d0aa96e2788cfbf6

Observation 1ec6360c-1fec-4e2d-9e1f-3695c7e3898f · inbound

Deep far-UV observations of the ELAIS N1 field using AstroSat: Source catalogue, spectral energy distribution modelling and star formation cites this paper.

Deep far-UV observations of the ELAIS N1 field using AstroSat: Source catalogue, spectral energy distribution modelling and star formation The infrared-radio correlation of star-forming galaxies is strongly M$_{\star}$-dependent but nearly redshift-invariant since z$\sim$4

Reference 205

Resolution
verified exact
local_arxiv, observed 2026-07-08T15:35:06.887663Z

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=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:7642456724fc52650675270d0cb02b09aeea9ef42f04d48d891d46f53cfa3aee

Observation 01366495-8969-4029-a503-cead2fccd60e · inbound

Deep far-UV observations of the ELAIS N1 field using AstroSat: Source catalogue, spectral energy distribution modelling and star formation cites this paper.

Deep far-UV observations of the ELAIS N1 field using AstroSat: Source catalogue, spectral energy distribution modelling and star formation The infrared-radio correlation of star-forming galaxies is strongly M$_{\star}$-dependent but nearly redshift-invariant since z$\sim$4

Reference 205

Resolution
unresolved
no resolver link, observed 2026-07-14T16:07:11.412748Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T16:07:11.412748Z digest=sha256:89880cd887407032614189f4ac71f0c34d2b066cea340e1427a00390d3d5b4eb

Observation 7eca1cd4-14ba-451c-bc45-928c6258ce6a · inbound

The DESI View of the Faint Radio Source Population in LoTSS DR2 cites this paper.

The DESI View of the Faint Radio Source Population in LoTSS DR2 The infrared-radio correlation of star-forming galaxies is strongly M$_{\star}$-dependent but nearly redshift-invariant since z$\sim$4

Reference 65

Resolution
verified exact
local_arxiv, observed 2026-07-10T17:27:26.412055Z

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=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:3e5f6ab7b014e7e2a8e75c09e1b200df83045a1e4e75c59f6cebd85dfb885249