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Paper Citation Record · LEDGER

What Shapes the Luminosity Function of Galaxies?

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:astro-ph/0302450.

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

pith.paper-citation-record.v1
astro-ph/0302450 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T00:16:27.364744Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-27T16:11:02.309347Z

Reference resolution

0 of 0 outbound references displayed

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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 a5e8187a-7b37-468b-9b29-9f0288016008 · inbound

JWST Advanced Deep Extragalactic Survey (JADES) Data Release 5: stellar population catalogue for galaxies in GOODS-N and GOODS-S cites this paper.

JWST Advanced Deep Extragalactic Survey (JADES) Data Release 5: stellar population catalogue for galaxies in GOODS-N and GOODS-S What Shapes the Luminosity Function of Galaxies?

Reference 60

Resolution
verified exact
local_arxiv, observed 2026-05-22T09:06:18.957130Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:dd09f3f2435c3a1d101295595f7aa8a78bc865402a8b6557c6c0738526325f94

Observation 7b6a737e-0652-4e33-b2ed-8994a135c413 · inbound

Satellite compaction pathways: environmental drivers shaping dwarf galaxy corpulence in the TNG50 simulation cites this paper.

Satellite compaction pathways: environmental drivers shaping dwarf galaxy corpulence in the TNG50 simulation What Shapes the Luminosity Function of Galaxies?

Reference 57

Resolution
verified exact
local_arxiv, observed 2026-06-27T16:11:02.310491Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:47c0f234f1d7797a513f0a27c4778457611bcdf4e9d92cc23c69727363b43035

Observation a7a9e5e3-342a-4e5e-b023-dc2a2dd85be4 · inbound

Multiphase images of a powerful supernova-driven wind in the early Universe cites this paper.

Multiphase images of a powerful supernova-driven wind in the early Universe What Shapes the Luminosity Function of Galaxies?

Reference 105

Resolution
verified exact
local_arxiv, observed 2026-06-27T13:00:56.624340Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:a9c989b7123b324c2683e963b5067712472c4976d189438287dbf7b874cbe560

Observation 5c0b4664-b8f2-4145-9e9d-f2eac5f3d211 · inbound

Cosmological Galaxy Formation Modelling in the Era of the Square Kilometre Array cites this paper.

Cosmological Galaxy Formation Modelling in the Era of the Square Kilometre Array What Shapes the Luminosity Function of Galaxies?

Reference 158

Resolution
verified exact
local_arxiv, observed 2026-06-25T21:38:29.144658Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:0451b69c963140d8d08ae09888895cc0d36e3bfbba16f26f09cad00e9b07a289

Observation 860c7f73-dbfc-414a-b886-c8c3aa3d217a · inbound

Exploring the physics of ram pressure stripping with radio continuum observations in the SKA era cites this paper.

Exploring the physics of ram pressure stripping with radio continuum observations in the SKA era What Shapes the Luminosity Function of Galaxies?

Reference 60

Resolution
verified exact
local_arxiv, observed 2026-06-25T21:28:28.446755Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:51411590b2abfb005160ebed69da6631ee50621d02a389bbcd544b1707542ce8

Observation 447a84b9-4b20-44c1-8a74-7780377cb0ab · inbound

Satellite quenching by radio jets of central galaxies in galaxy groups cites this paper.

Satellite quenching by radio jets of central galaxies in galaxy groups What Shapes the Luminosity Function of Galaxies?

Reference 86

Resolution
unresolved
no resolver link, observed 2026-07-12T06:58:22.474180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-12T06:58:22.474180Z digest=sha256:1ae7f21494675c0cf781cf3b5d044712f209fcbdfcacd1e7727f12bcf32716be

Observation 1d7ce425-735d-4977-ad1e-0c7819c98d6d · inbound

First Light and Assembly of GalaxieS (FLAGS) I: The JWST/NIRCam Number Counts and IGL as Constraints on Galaxy Formation Models cites this paper.

First Light and Assembly of GalaxieS (FLAGS) I: The JWST/NIRCam Number Counts and IGL as Constraints on Galaxy Formation Models What Shapes the Luminosity Function of Galaxies?

Reference 11

Resolution
unresolved
no resolver link, observed 2026-08-11T00:30:25.367869Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T00:30:25.367869Z digest=sha256:5834d6c9136779d7549a0042f9b230bb246e2f70666a3731120514aa183b5b34

Observation 71908dfe-7cd8-4963-a0d1-9c8e40c0c9c0 · inbound

The Quasar Feedback Survey: Ionised Outflows in type 2 QSOs with MUSE data cites this paper.

The Quasar Feedback Survey: Ionised Outflows in type 2 QSOs with MUSE data What Shapes the Luminosity Function of Galaxies?

Reference 212

Resolution
unresolved
no resolver link, observed 2026-08-12T00:16:27.364744Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T00:16:27.364744Z digest=sha256:1968ddd6fb7ddaebe54566d52346baa30d6537af374ca457e4b8689293e044aa