Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Metallicity Gradients in Modern Cosmological Simulations I: Tension Between Smooth Stellar Feedback Models and Observations
As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2503.03804.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-19T06:32:44.657259+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-09T22:56:06.996320Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z
Reference resolution
0 of 0 outbound references displayed
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External citation measurements
1
arxiv_reference, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation d5becdcf-371a-4148-8e7c-d9f329053694 · inbound
Star Formation Rates, Metallicities, and Stellar Masses on kpc-scales in TNG50 cites this paper.
Star Formation Rates, Metallicities, and Stellar Masses on kpc-scales in TNG50 Metallicity Gradients in Modern Cosmological Simulations I: Tension Between Smooth Stellar Feedback Models and Observations
Reference 43
- Resolution
- unresolved
- no resolver link, observed 2026-08-09T22:56:06.996320Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3b97d23b-2c45-4a42-b663-10b633d29c79 · inbound
The survey of planetary nebulae in Andromeda (M31) VII. Predictions of a major merger simulation model compared with chemodynamical data of the disc and inner halo substructures cites this paper.
The survey of planetary nebulae in Andromeda (M31) VII. Predictions of a major merger simulation model compared with chemodynamical data of the disc and inner halo substructures Metallicity Gradients in Modern Cosmological Simulations I: Tension Between Smooth Stellar Feedback Models and Observations
Reference 43
- Resolution
- unresolved
- no resolver link, observed 2026-08-09T17:25:48.006814Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1be6d64e-0720-40f0-9068-8af8e9123f68 · inbound
Insight into the physical processes that shape the metallicity profiles in galaxies cites this paper.
Insight into the physical processes that shape the metallicity profiles in galaxies Metallicity Gradients in Modern Cosmological Simulations I: Tension Between Smooth Stellar Feedback Models and Observations
Reference 29
- Resolution
- unresolved
- no resolver link, observed 2026-08-09T13:30:01.777476Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7f5c806d-9e7c-433a-ac23-ad2cb313cd1e · inbound
Galaxy Metallicity Gradients in the Reionization Epoch from the FIRE-2 Simulations cites this paper.
Galaxy Metallicity Gradients in the Reionization Epoch from the FIRE-2 Simulations Metallicity Gradients in Modern Cosmological Simulations I: Tension Between Smooth Stellar Feedback Models and Observations
Reference 23
- Resolution
- verified exact
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.
Observation c40f37f8-afdd-4e7a-91ff-fd7106cc87fd · inbound
The DREAMS Project: Disentangling the Impact of Halo-to-Halo Variance and Baryonic Feedback on Milky Way Dark Matter Density Profiles cites this paper.
The DREAMS Project: Disentangling the Impact of Halo-to-Halo Variance and Baryonic Feedback on Milky Way Dark Matter Density Profiles Metallicity Gradients in Modern Cosmological Simulations I: Tension Between Smooth Stellar Feedback Models and Observations
Reference 30
- Resolution
- verified exact
- arxiv_id, observed 2026-05-17T01:58:51.025281Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.
Observation d72a332d-df4e-4630-9008-10f7d45e6187 · inbound
MSA-3D: Connecting the Chemical and Kinematic Structures of Galaxies at $z \sim 1$ cites this paper.
MSA-3D: Connecting the Chemical and Kinematic Structures of Galaxies at $z \sim 1$ Metallicity Gradients in Modern Cosmological Simulations I: Tension Between Smooth Stellar Feedback Models and Observations
Reference 12
- Resolution
- verified exact
- arxiv_id, observed 2026-05-16T12:22:52.041295Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.
Observation aba2d656-59ec-422e-9ccd-249f1da18c63 · inbound
MSA-3D: Connecting the Chemical and Kinematic Structures of Galaxies at $z \sim 1$ cites this paper.
MSA-3D: Connecting the Chemical and Kinematic Structures of Galaxies at $z \sim 1$ Metallicity Gradients in Modern Cosmological Simulations I: Tension Between Smooth Stellar Feedback Models and Observations
Reference 12
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T09:04:23.249681Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.