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Paper Citation Record · LEDGER

A protostellar system fed by a streamer of 10,500 au length

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2007.13430.

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

pith.paper-citation-record.v1
2007.13430 v1

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 2026-08-19T06:32:44.657259+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T11:33:56.865149Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-15T13:05:38.416241Z

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 04d97b4d-d55c-442f-89d4-2b953a5fb8d8 · inbound

The emerging timescale of young star clusters regulated by cluster stellar mass cites this paper.

The emerging timescale of young star clusters regulated by cluster stellar mass A protostellar system fed by a streamer of 10,500 au length

Reference 55

Resolution
malformed identifier
arxiv_id, observed 2026-05-15T13:05:38.418004Z

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.

source=pdf_text observed=2026-05-15T13:03:52.765706Z digest=sha256:ff8e77891faf54a2ddf093d0e2a64467f9e30d45c13bb9e57a95c127936be70d

Observation af565f31-3917-4667-9d05-68f207d92d35 · inbound

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching cites this paper.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching A protostellar system fed by a streamer of 10,500 au length

Reference 49

Resolution
unresolved
no resolver link, observed 2026-07-14T15:02:03.459139Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T15:02:03.459139Z digest=sha256:0884b2870cfdd11044b8b7d45f23d2428183cd46a1789f7aa6b3d31e1500e74c

Observation 793a63e9-ee59-41cf-b9af-33cbd6ea46e7 · inbound

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching cites this paper.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching A protostellar system fed by a streamer of 10,500 au length

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-02T07:32:02.671277Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T07:32:02.671277Z digest=sha256:1653f7702346ca7729cdb1c009fedf010e1d418c62bdc691d501add9db3cf1a8

Observation 2b7734e6-2502-48e4-9b0e-f4ea03239278 · inbound

Preferential alignment of Class 0, Class I protostellar disks in multiple systems across nine nearby molecular clouds cites this paper.

Preferential alignment of Class 0, Class I protostellar disks in multiple systems across nine nearby molecular clouds A protostellar system fed by a streamer of 10,500 au length

Reference 129

Resolution
unresolved
no resolver link, observed 2026-08-02T02:36:30.159039Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T02:36:30.159039Z digest=sha256:9ba7a1232fb05fdcfce6974d9ae6e4f59b4bf6c820dbe63ac3ec14efea892f67

Observation df772c38-e41e-4b79-a488-153ff2024d45 · inbound

A JWST, ALMA and VLA survey of the Ophiuchus-A star-forming region: Unveiling hidden dust mass and connecting infrared outflows to their radio origins cites this paper.

A JWST, ALMA and VLA survey of the Ophiuchus-A star-forming region: Unveiling hidden dust mass and connecting infrared outflows to their radio origins A protostellar system fed by a streamer of 10,500 au length

Reference 147

Resolution
unresolved
no resolver link, observed 2026-08-01T23:20:56.982899Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T23:20:56.982899Z digest=sha256:70f2421fa4ce888a2eef79ccecc25ae16d74ac5bc30b12e03f555653dd48c2f3

Observation 73ac26f3-46ce-4d49-8c12-f57cda3f8197 · inbound

Angular Momentum of Planet-Forming Disks: Implications for Infall Driven Misalignments cites this paper.

Angular Momentum of Planet-Forming Disks: Implications for Infall Driven Misalignments A protostellar system fed by a streamer of 10,500 au length

Reference 48

Resolution
unresolved
no resolver link, observed 2026-07-30T14:23:16.794661Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-30T14:23:16.794661Z digest=sha256:6406c902662b49528fc80c10144e7e41ee60c00e90ad64bfd1e707a5e1162771

Observation c1a57e40-c8cd-47fa-9401-aa7cada464d3 · inbound

Angular Momentum of Planet-Forming Disks: Implications for Infall Driven Misalignments cites this paper.

Angular Momentum of Planet-Forming Disks: Implications for Infall Driven Misalignments A protostellar system fed by a streamer of 10,500 au length

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-04T01:36:12.374228Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T01:36:12.374228Z digest=sha256:5f79f20881fd3fef61dc59f3f3396dbfa2c2b97855e51a2cbea1a868f1a3247e

Observation 8d5d6f9d-f40f-438c-b299-5b38bbc85853 · inbound

Accretion across scales: streamers, surface-layer transport, and rapid replenishment in young protoplanetary discs cites this paper.

Accretion across scales: streamers, surface-layer transport, and rapid replenishment in young protoplanetary discs A protostellar system fed by a streamer of 10,500 au length

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-04T11:33:56.865149Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:33:56.865149Z digest=sha256:61f835e58cb85a7d27bf0dc93dff1ed0d0bd2c785cc57b9705b03e018393d569