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Paper Citation Record · LEDGER

The evolution of star formation histories of quiescent galaxies

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1609.03572.

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

pith.paper-citation-record.v1
1609.03572 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 5 of 5 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 2026-07-10T10:27:02.188010Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • 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 c9e00d95-d1a3-4f94-8dd4-2e9ef70a5264 · inbound

Strong Progenitor Age Bias in Supernova Cosmology. III. Progenitor Age as the Physical Origin of the Type Ia Supernova Magnitude Steps with Host Properties cites this paper.

Strong Progenitor Age Bias in Supernova Cosmology. III. Progenitor Age as the Physical Origin of the Type Ia Supernova Magnitude Steps with Host Properties The evolution of star formation histories of quiescent galaxies

Reference 74

Resolution
verified exact
local_arxiv, observed 2026-05-14T20:52:57.045580Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:5637ecbc91bd17710e015e802cd149ef78a0c4fe0089f516b3cce3efc1dbb14d

Observation b9b432dc-d6fe-437f-924d-c01b14e55be0 · inbound

On the later evolution of observationally selected protocluster candidates at $z\,{\gtrsim}\,5$ cites this paper.

On the later evolution of observationally selected protocluster candidates at $z\,{\gtrsim}\,5$ The evolution of star formation histories of quiescent galaxies

Reference 216

Resolution
verified exact
local_arxiv, observed 2026-06-26T20:09:57.473361Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:5ad3db42c0efd049e61f382fc48ef88cac985b9d25baa683526ec07fcea6acb5

Observation 63f5f706-15e9-4c6f-99da-e8c1bf0404aa · inbound

LEGGOS I: The JWST LEGGOS Survey -- LEnsing and Galaxy Growth: Observing Substructures -- Unpacks the Nature of Clumpy Star Formation and Quenching in Gravitationally Lensed Galaxies beyond Cosmic Noon cites this paper.

LEGGOS I: The JWST LEGGOS Survey -- LEnsing and Galaxy Growth: Observing Substructures -- Unpacks the Nature of Clumpy Star Formation and Quenching in Gravitationally Lensed Galaxies beyond Cosmic Noon The evolution of star formation histories of quiescent galaxies

Reference 119

Resolution
verified exact
local_arxiv, observed 2026-06-26T16:19:35.510160Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:4110b7e8e1a8249a779953d7b17d6f775b906169b1c82cfb5cd4feec5bb83dab

Observation 29e8201e-0355-4140-9935-474589fcbea0 · inbound

COSMOS-Web: does halo mass alone shape the clustering of star-forming and quiescent galaxies? cites this paper.

COSMOS-Web: does halo mass alone shape the clustering of star-forming and quiescent galaxies? The evolution of star formation histories of quiescent galaxies

Reference 156

Resolution
verified exact
local_arxiv, observed 2026-07-01T04:05:20.562466Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:e0e5c48d8e8111b03ef5f69ec1317bb6233aefc7ea2ec02e55742210247f5da0

Observation e10663f9-bc25-442a-808e-733f9dbcf266 · inbound

Subaru meets JWST: A Direct Measurement of Ly$\boldsymbol{\alpha}$ Escape Fraction at $\boldsymbol{z\simeq6.2}$ with Dual Narrow-Band Imaging cites this paper.

Subaru meets JWST: A Direct Measurement of Ly$\boldsymbol{\alpha}$ Escape Fraction at $\boldsymbol{z\simeq6.2}$ with Dual Narrow-Band Imaging The evolution of star formation histories of quiescent galaxies

Reference 169

Resolution
verified exact
local_arxiv, observed 2026-07-10T10:27:02.189347Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:546616b3eff7ebf868a0d6da5ad55ab26d82b2c70b1632647d07dea0a2f6bb66