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Paper Citation Record · LEDGER

A Turnover in the Galaxy Main Sequence of Star Formation at $M_{*} \sim 10^{10} M_{\odot}$ for Redshifts $z < 1.3$

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1501.01080.

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

pith.paper-citation-record.v1
1501.01080 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 2026-08-16T06:30:59.297886+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-09T05:26:01.576658Z

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 8d3d9304-123d-4b0c-9b68-c4edc7b65e79 · inbound

Empirical estimates of how massive galaxies can be in {\Lambda}CDM cites this paper.

Empirical estimates of how massive galaxies can be in {\Lambda}CDM A Turnover in the Galaxy Main Sequence of Star Formation at $M_{*} \sim 10^{10} M_{\odot}$ for Redshifts $z < 1.3$

Reference 157

Resolution
verified exact
local_arxiv, observed 2026-05-14T21:09:27.922361Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:6b076ed390bcd68213b5a6732e409ce76b4a624618f9a21586f9f16a35b82471

Observation 653864d1-ec6b-4b01-9e72-b9d4187ca30f · inbound

Gamma-ray bursts reveal the history and faint contributors of cosmic reionization cites this paper.

Gamma-ray bursts reveal the history and faint contributors of cosmic reionization A Turnover in the Galaxy Main Sequence of Star Formation at $M_{*} \sim 10^{10} M_{\odot}$ for Redshifts $z < 1.3$

Reference 54

Resolution
verified exact
local_arxiv, observed 2026-07-09T05:26:01.578659Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

source=arxiv_source observed=2026-07-09T05:25:12.742172Z digest=sha256:400501c4e44cc5c3d6d134fcb6d23e353652defe328a75b9e240e76eb1a6c274