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Paper Citation Record · LEDGER

The specific star formation rate function at different mass scales and quenching: A comparison between cosmological models and SDSS

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2010.08173.

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

pith.paper-citation-record.v1
2010.08173 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-05T06:32:48.257954+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T08:26:15.634877Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T00:46:39.931815Z

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 c4c08805-b46d-4d7b-984a-956808b9e63b · inbound

First detection of ultra-fast outflows in a quiescent galaxy cites this paper.

First detection of ultra-fast outflows in a quiescent galaxy The specific star formation rate function at different mass scales and quenching: A comparison between cosmological models and SDSS

Reference 198

Resolution
verified exact
local_arxiv, observed 2026-07-10T00:46:39.933202Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:d7ec73c82387f9f009d8edff7839f287486a58849b63c0972c29449bb2a6879a

Observation fde08267-125d-4e81-b6cf-b3c9a52d47a5 · inbound

What's Missing in AGN Feedback? Lessons learnt from Magneticum, IllustrisTNG and Simba cites this paper.

What's Missing in AGN Feedback? Lessons learnt from Magneticum, IllustrisTNG and Simba The specific star formation rate function at different mass scales and quenching: A comparison between cosmological models and SDSS

Reference 182

Resolution
unresolved
no resolver link, observed 2026-08-01T08:26:15.634877Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T08:26:15.634877Z digest=sha256:25f3c3af3cce44bb5652800aac8cb5eff4174d9051a39b8e362c252de7deb583