Paper Citation Record · LEDGER

How Do Disks Survive Mergers?

As of 4 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:0806.1739.

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

pith.paper-citation-record.v1
0806.1739 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 9 of 9 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-03T06:30:56.289259+00:00

measured 9 of 9 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-31T15:28:44.435273Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-03T08:37:46.178289Z

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 72223eab-e1b8-4cdc-8bae-1035e6dc41b2 · inbound

One Merge to Rule Them All: From Galaxy Interactions to Black Hole Mergers Using Horizon-AGN cites this paper.

One Merge to Rule Them All: From Galaxy Interactions to Black Hole Mergers Using Horizon-AGN How Do Disks Survive Mergers?

Reference 48

Resolution: verified exact; local_arxiv, observed 2026-05-14T20:47:57.043291Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-03T06:30:56.289259+00:00.

Observation b4627853-f039-49ab-b18a-77669a3939c3 · inbound

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies cites this paper.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies How Do Disks Survive Mergers?

Reference 30

Resolution: verified exact; local_arxiv, observed 2026-05-20T08:58:09.878249Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-03T06:30:56.289259+00:00.

Observation 8336f315-1b4c-43f5-8781-f0bca5130a8f · inbound

Dust destruction signals shock-accelerated outflows in the nearby active galaxy NGC 1068 cites this paper.

Dust destruction signals shock-accelerated outflows in the nearby active galaxy NGC 1068 How Do Disks Survive Mergers?

Reference 264

Resolution: verified exact; local_arxiv, observed 2026-06-25T22:58:40.773923Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-03T06:30:56.289259+00:00.

Observation dadc5197-31d3-40cd-949e-1acc82001aa0 · inbound

Dust destruction signals shock-accelerated outflows in the nearby active galaxy NGC 1068 cites this paper.

Dust destruction signals shock-accelerated outflows in the nearby active galaxy NGC 1068 How Do Disks Survive Mergers?

Reference 264

Resolution: verified exact; local_arxiv, observed 2026-06-26T05:28:59.844919Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-03T06:30:56.289259+00:00.

Observation ba9d00a2-6b59-4bbf-97eb-9a9f3efb75c8 · inbound

Tidal origin of dark-matter free dwarf galaxies in the NGC 1052 group cites this paper.

Tidal origin of dark-matter free dwarf galaxies in the NGC 1052 group How Do Disks Survive Mergers?

Reference 56

Resolution: verified exact; local_arxiv, observed 2026-07-01T02:15:15.070609Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-03T06:30:56.289259+00:00.

Observation 531f5baf-8ce9-44d9-9f63-b9ef8d6dc2ba · inbound

Tidal origin of dark-matter free dwarf galaxies in the NGC 1052 group cites this paper.

Tidal origin of dark-matter free dwarf galaxies in the NGC 1052 group How Do Disks Survive Mergers?

Reference 56

Resolution: verified exact; local_arxiv, observed 2026-07-02T20:27:21.598792Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-03T06:30:56.289259+00:00.

Observation 4e1c7d5f-e239-4bd4-a9b8-b81746020b60 · inbound

Optically Selected Superthin Galaxies Remain Thin in the Near-infrared cites this paper.

Optically Selected Superthin Galaxies Remain Thin in the Near-infrared How Do Disks Survive Mergers?

Reference 76

Resolution: verified exact; local_arxiv, observed 2026-07-02T09:36:49.025744Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-03T06:30:56.289259+00:00.

Observation 45f838b0-678e-4cc6-a0fe-291d8a394761 · inbound

The Merger-Driven Origin of the Vast Extended Stellar Disc Around the Andromeda Galaxy cites this paper.

The Merger-Driven Origin of the Vast Extended Stellar Disc Around the Andromeda Galaxy How Do Disks Survive Mergers?

Reference 43

Resolution: verified exact; local_arxiv, observed 2026-07-03T08:37:46.179770Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-03T06:30:56.289259+00:00.

Observation a2a6c00a-e911-42ec-89b9-dbadf4c952dd · inbound

Searching in HI for Massive Low Surface Brightness Galaxies: II. Completing the UGC Sample cites this paper.

Searching in HI for Massive Low Surface Brightness Galaxies: II. Completing the UGC Sample How Do Disks Survive Mergers?

Reference 228

Resolution: unresolved; no resolver link, observed 2026-07-31T15:28:44.435273Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.