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Paper Citation Record · LEDGER

Impact of initial mass function on the chemical evolution of high-redshift galaxies

As of 20 August 2026, this Paper Citation Record lists 12 of 12 outbound references and 2 inbound Pith citation observations for arXiv:2506.06139.

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

pith.paper-citation-record.v1
2506.06139 v3

Coverage vector

measured 12 of 12 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-05-19T10:48:01.438891Z

measured 14 of 14 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-20T06:33:59.587034+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-02T17:57:57.440482Z

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

12 of 12 outbound references displayed

  • verified exact0
  • verified fuzzy6
  • unresolved2
  • parse uncertain0
  • malformed identifier3
  • metadata mismatch1

External citation measurements

0
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

Observation ce43f095-f8e1-404a-b14f-21a900cb431c · outbound

This paper cites The Science of the Einstein Telescope.

Impact of initial mass function on the chemical evolution of high-redshift galaxies The Science of the Einstein Telescope

Reference 1

Resolution
metadata mismatch
local_arxiv, observed 2026-05-19T10:52:15.319146Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation 8d3a0ba1-07cc-4177-9ee1-31002afef32b · outbound

This paper cites an unresolved cited work.

Impact of initial mass function on the chemical evolution of high-redshift galaxies Unresolved cited work

Reference 2

Resolution
unresolved
raw_fallback, observed 2026-05-19T10:57:18.844089Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation c143b728-9846-4824-b750-4519913b1e97 · outbound

This paper cites Similar to the case of the old prescription, the sim- ulated SFMS is generally in agreement with that from Rinaldi et al.

Impact of initial mass function on the chemical evolution of high-redshift galaxies Similar to the case of the old prescription, the sim- ulated SFMS is generally in agreement with that from Rinaldi et al

Reference 3

Resolution
verified fuzzy
raw_fallback, observed 2026-05-19T10:57:18.874202Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation 68315a14-d157-4b27-814a-0e422b485b93 · outbound

This paper cites an unresolved cited work.

Impact of initial mass function on the chemical evolution of high-redshift galaxies Unresolved cited work

Reference 4

Resolution
malformed identifier
raw_fallback, observed 2026-05-19T10:57:18.870699Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation 94217f2f-928d-4493-8a21-0ea3606c22fe · outbound

This paper cites The long dashed curve shows the total SFRD measured in simulation timesteps.

Impact of initial mass function on the chemical evolution of high-redshift galaxies The long dashed curve shows the total SFRD measured in simulation timesteps

Reference 5

Resolution
verified fuzzy
raw_fallback, observed 2026-05-19T10:57:18.868556Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation eeee9ffb-af94-4f1f-8d31-16684ee45c73 · outbound

This paper cites (2023) and Curti et al.

Impact of initial mass function on the chemical evolution of high-redshift galaxies (2023) and Curti et al

Reference 6

Resolution
verified fuzzy
raw_fallback, observed 2026-05-19T10:57:18.865980Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation c4426c7a-8168-4403-87b9-2f601a3d10d2 · outbound

This paper cites Each data point involves three diamonds color-coded by the mean and 1 σ upper and lower limits of metallicity.

Impact of initial mass function on the chemical evolution of high-redshift galaxies Each data point involves three diamonds color-coded by the mean and 1 σ upper and lower limits of metallicity

Reference 7

Resolution
verified fuzzy
raw_fallback, observed 2026-05-19T10:57:18.862479Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation 07133042-aa01-49d1-8627-7f7adaa16b1b · outbound

This paper cites an unresolved cited work.

Impact of initial mass function on the chemical evolution of high-redshift galaxies Unresolved cited work

Reference 8

Resolution
unresolved
raw_fallback, observed 2026-05-19T10:57:18.859495Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation 9151b071-b18e-46b8-b856-3f817d2ed739 · outbound

This paper cites (2012); V ogelsberger et al.

Impact of initial mass function on the chemical evolution of high-redshift galaxies (2012); V ogelsberger et al

Reference 9

Resolution
verified fuzzy
raw_fallback, observed 2026-05-19T10:57:18.856028Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation 41f46072-1e9a-4f20-b177-f4f14c022e34 · outbound

This paper cites At each star for- mation timestep i, we first estimate the number of SN Ia pro- genitors expected to form as Ni Ia,P,est = NIaδM⋆ given the mass δMi ⋆ of stars formed in this step.

Impact of initial mass function on the chemical evolution of high-redshift galaxies At each star for- mation timestep i, we first estimate the number of SN Ia pro- genitors expected to form as Ni Ia,P,est = NIaδM⋆ given the mass δMi ⋆ of stars formed in this step

Reference 10

Resolution
verified fuzzy
raw_fallback, observed 2026-05-19T10:57:18.841685Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation 266a8c68-5f1c-47e0-bf83-7cf7a1d9b93d · outbound

This paper cites an unresolved cited work.

Impact of initial mass function on the chemical evolution of high-redshift galaxies Unresolved cited work

Reference 11

Resolution
malformed identifier
raw_fallback, observed 2026-05-19T10:57:18.846330Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Observation 9063d504-af2c-40ac-9e8d-12ad1569126c · outbound

This paper cites an unresolved cited work.

Impact of initial mass function on the chemical evolution of high-redshift galaxies Unresolved cited work

Reference 12

Resolution
malformed identifier
raw_fallback, observed 2026-05-19T10:57:18.849182Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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Pith citing papers

Observation c14ccfa7-f9bd-430f-9118-9f18feebd302 · inbound

JADES: the mass-metallicity relation at $z=1-10$. New calibrations, extremely metal-poor galaxies, and chemical diversity cites this paper.

JADES: the mass-metallicity relation at $z=1-10$. New calibrations, extremely metal-poor galaxies, and chemical diversity Impact of initial mass function on the chemical evolution of high-redshift galaxies

Reference 123

Resolution
verified exact
local_arxiv, observed 2026-06-27T12:20:54.762424Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-06-27T12:17:35.420949Z digest=sha256:9b81e59630adf787cd697601baccd497a6a6c591586a59dd878166de9c3fc420

Observation 4332b2c4-bfd2-4fbf-95e2-f7f537b0b4bf · inbound

How can we finally see the first light? Status and perspective in the search for Population III stars cites this paper.

How can we finally see the first light? Status and perspective in the search for Population III stars Impact of initial mass function on the chemical evolution of high-redshift galaxies

Reference 213

Resolution
metadata mismatch
local_arxiv, observed 2026-07-02T18:17:16.997804Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

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