Paper Citation Record · LEDGER

Protoplanetary disk masses from CO isotopologues line emission

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1410.2093.

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

pith.paper-citation-record.v1
1410.2093 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-05T06:32:48.257954+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T22:01:35.545126Z

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

0 of 0 outbound references displayed

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External citation measurements

198
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 5f1642d2-8341-4ab6-8601-3d80265f8cbe · inbound

Chemistry and IR emission of acetylene in planet-forming regions of T Tauri disks. Impact of elemental abundances and dust properties cites this paper.

Chemistry and IR emission of acetylene in planet-forming regions of T Tauri disks. Impact of elemental abundances and dust properties Protoplanetary disk masses from CO isotopologues line emission

Reference 100

Resolution: verified exact; local_arxiv, observed 2026-05-20T00:57:54.032424Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 9aa2f00d-936a-44eb-93d0-79798704838f · inbound

Chemistry and IR emission of acetylene in planet-forming regions of T Tauri disks. Impact of elemental abundances and dust properties cites this paper.

Chemistry and IR emission of acetylene in planet-forming regions of T Tauri disks. Impact of elemental abundances and dust properties Protoplanetary disk masses from CO isotopologues line emission

Reference 100

Resolution: verified exact; local_arxiv, observed 2026-05-20T08:38:09.505335Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 66dc8c1f-b2ab-4276-ab22-3044a05a406a · inbound

CO snow lines are stabilised by the vertical transport of volatiles cites this paper.

CO snow lines are stabilised by the vertical transport of volatiles Protoplanetary disk masses from CO isotopologues line emission

Reference 70

Resolution: verified exact; local_arxiv, observed 2026-06-30T04:04:18.126621Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 8afc22ab-1997-44ea-922b-f0dabba1a471 · inbound

Native-resolution retrievals of VHS 1256-1257 b spanning the JWST/NIRSpec wavelength range: Chemical composition of a partially cloudy atmosphere cites this paper.

Native-resolution retrievals of VHS 1256-1257 b spanning the JWST/NIRSpec wavelength range: Chemical composition of a partially cloudy atmosphere Protoplanetary disk masses from CO isotopologues line emission

Reference 70

Resolution: verified exact; local_arxiv, observed 2026-07-02T05:36:39.245893Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

Observation 2941485d-a4b7-4dcb-9630-9755be30dc16 · inbound

Extending dynamical mass measurements: probing GI as a possible origin of mm-dust spirals cites this paper.

Extending dynamical mass measurements: probing GI as a possible origin of mm-dust spirals Protoplanetary disk masses from CO isotopologues line emission

Reference 191

Resolution: unresolved; no resolver link, observed 2026-08-01T22:01:35.545126Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.