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Paper Citation Record · LEDGER

Variations of the initial mass function in semi-analytical models: implications for the mass assembly and the chemical enrichment of galaxies in the GAEA model

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1606.01908.

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

pith.paper-citation-record.v1
1606.01908 v2

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

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T13:44:39.937530Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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External citation measurements

70
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 6c900fff-689d-470e-82f0-f58522314c4a · inbound

Dark-matter-induced transients over cosmic time: The role of star formation history profiles cites this paper.

Dark-matter-induced transients over cosmic time: The role of star formation history profiles Variations of the initial mass function in semi-analytical models: implications for the mass assembly and the chemical enrichment of galaxies in the GAEA model

Reference 61

Resolution
unresolved
no resolver link, observed 2026-08-07T13:44:39.937530Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T13:44:39.937530Z digest=sha256:79b74ce1ad556f572b957c3603786d72833492ebdc197f8885d3fe515389f94b

Observation 3fdf63c6-217e-42f7-98e4-dc0c66213910 · inbound

MEGA and SMILES Find Fewer Dusty Galaxies than Expected at Cosmic Noon cites this paper.

MEGA and SMILES Find Fewer Dusty Galaxies than Expected at Cosmic Noon Variations of the initial mass function in semi-analytical models: implications for the mass assembly and the chemical enrichment of galaxies in the GAEA model

Reference 124

Resolution
verified exact
local_arxiv, observed 2026-06-27T03:30:27.428528Z

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.

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Observation 1685c15f-458c-4c4c-88c7-1218f77a13ad · 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 Variations of the initial mass function in semi-analytical models: implications for the mass assembly and the chemical enrichment of galaxies in the GAEA model

Reference 165

Resolution
verified exact
local_arxiv, observed 2026-06-30T05:14:17.603150Z

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:fee9f2811e7f30d56b7f5c5d3ef2f29610b4806c5ad36e8ef0b003a9027a6257

Reference 75

Resolution
unresolved
no resolver link, observed 2026-08-01T22:19:57.473898Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T22:19:57.473898Z digest=sha256:9aa88c849968b660186b3dc748d2c088501e5a25f019425ca45a3bfbc9bd8109

Observation 8b14c54d-b231-41d8-950f-57ce39b5d6a0 · inbound

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity cites this paper.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Variations of the initial mass function in semi-analytical models: implications for the mass assembly and the chemical enrichment of galaxies in the GAEA model

Reference 117

Resolution
unresolved
no resolver link, observed 2026-08-01T14:10:56.523303Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T14:10:56.523303Z digest=sha256:0159c44a7c903d53318d8187f5ebb538b9b3781f2062705e32b3d64c932d2bab