Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Properties of galaxies reproduced by a hydrodynamic simulation
As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 13 inbound Pith citation observations for arXiv:1405.1418.
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 2026-08-06T06:34:29.942622+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-03T22:28:31.352939Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-03T09:57:55.471657Z
Reference resolution
0 of 0 outbound references displayed
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- malformed identifier0
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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 1f89b9f4-efb5-4e3c-b74b-05ecfb884467 · inbound
Realistic simulations of galaxy formation in f(R) modified gravity cites this paper.
Realistic simulations of galaxy formation in f(R) modified gravity Properties of galaxies reproduced by a hydrodynamic simulation
Reference 55
- Resolution
- verified exact
- local_arxiv, observed 2026-05-25T02:00:12.443821Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 5fe52943-b13a-49f0-9784-193117970009 · inbound
Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum cites this paper.
Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum Properties of galaxies reproduced by a hydrodynamic simulation
Reference 40
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T22:28:31.352939Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d88e1d3d-fda1-4ed1-84dd-c5604dcc0511 · inbound
Cosmological analysis of the DESI DR1 Lyman alpha 1D power spectrum cites this paper.
Cosmological analysis of the DESI DR1 Lyman alpha 1D power spectrum Properties of galaxies reproduced by a hydrodynamic simulation
Reference 114
- Resolution
- verified exact
- local_arxiv, observed 2026-05-16T10:07:44.119253Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 0561f0be-a734-4d18-ac47-9a26f930fef6 · inbound
First Light And Reionization Epoch Simulations (FLARES) XXI: The UV Indices of Galaxies in the Early Universe cites this paper.
First Light And Reionization Epoch Simulations (FLARES) XXI: The UV Indices of Galaxies in the Early Universe Properties of galaxies reproduced by a hydrodynamic simulation
Reference 296
- Resolution
- verified exact
- local_arxiv, observed 2026-05-14T18:19:22.758524Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 41ec28e1-0009-49d3-97ed-7cbb22d786b3 · inbound
Introducing the Lumina project: large-volume radiation-hydrodynamic simulations of the epochs of hydrogen and helium reionization cites this paper.
Introducing the Lumina project: large-volume radiation-hydrodynamic simulations of the epochs of hydrogen and helium reionization Properties of galaxies reproduced by a hydrodynamic simulation
Reference 260
- Resolution
- verified exact
- local_arxiv, observed 2026-05-19T16:17:38.588264Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 716f7ba3-0272-4900-a67d-471b8f839572 · inbound
The Lumina Project: CMB Optical Depth Fluctuations from Patchy Reionization cites this paper.
The Lumina Project: CMB Optical Depth Fluctuations from Patchy Reionization Properties of galaxies reproduced by a hydrodynamic simulation
Reference 97
- Resolution
- verified exact
- local_arxiv, observed 2026-05-20T08:43:09.142296Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 749acec1-dafa-476a-895a-dfe3ade57946 · inbound
Bulk vs. turbulent motions at the centres of galaxy clusters: AGN-driven turbulence according to TNG-Cluster cites this paper.
Bulk vs. turbulent motions at the centres of galaxy clusters: AGN-driven turbulence according to TNG-Cluster Properties of galaxies reproduced by a hydrodynamic simulation
Reference 129
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T05:01:39.545784Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 751f9419-0890-4de7-99c1-5c3c921614c3 · inbound
The Lumina Project: Intergalactic Clumping and Recombination Sinks cites this paper.
The Lumina Project: Intergalactic Clumping and Recombination Sinks Properties of galaxies reproduced by a hydrodynamic simulation
Reference 84
- Resolution
- verified exact
- local_arxiv, observed 2026-06-26T23:40:14.812430Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation a3294cda-1844-4206-8325-5bfc8115dd2c · inbound
The Large-Scale Structure of the Universe through the SKA lenses cites this paper.
The Large-Scale Structure of the Universe through the SKA lenses Properties of galaxies reproduced by a hydrodynamic simulation
Reference 217
- Resolution
- verified exact
- local_arxiv, observed 2026-07-01T04:25:21.896666Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation b1281af9-7751-46eb-9f46-a5070733a77d · inbound
Resolved HI and Environmental Dynamics cites this paper.
Resolved HI and Environmental Dynamics Properties of galaxies reproduced by a hydrodynamic simulation
Reference 91
- Resolution
- verified exact
- local_arxiv, observed 2026-07-03T09:57:55.473121Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 19e18182-1f60-443c-8fe1-6d41fdf4d475 · inbound
Performance of morphological classifiers for galaxy mergers compared to current machine learning methods cites this paper.
Performance of morphological classifiers for galaxy mergers compared to current machine learning methods Properties of galaxies reproduced by a hydrodynamic simulation
Reference 13
- Resolution
- unresolved
- no resolver link, observed 2026-07-13T04:41:12.165957Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9d204f12-f0ba-4365-90c0-ac9153071e79 · inbound
Magnesium isotope ratios in Milky Way and dwarf galaxy stars cites this paper.
Magnesium isotope ratios in Milky Way and dwarf galaxy stars Properties of galaxies reproduced by a hydrodynamic simulation
Reference 14
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T02:55:51.536555Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation afbb9e3b-f93e-40fc-82df-fbc6377144a7 · inbound
Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters cites this paper.
Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters Properties of galaxies reproduced by a hydrodynamic simulation
Reference 16
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T23:43:56.435000Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.