Pith. sign in

Paper Citation Record · LEDGER

Dynamical Masses of Low Mass Stars in the Taurus and Ophiuchus Star Forming Regions

As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1706.03505.

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

pith.paper-citation-record.v1
1706.03505 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-06T06:34:29.942622+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T22:01:28.613871Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-14T04:00:13.625611Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

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 36cbe564-fdb8-49d6-b998-b2bc5f187a48 · inbound

Unstable magnetospheric accretion on the T Tauri star TW Hya cites this paper.

Unstable magnetospheric accretion on the T Tauri star TW Hya Dynamical Masses of Low Mass Stars in the Taurus and Ophiuchus Star Forming Regions

Reference 278

Resolution
verified exact
local_arxiv, observed 2026-07-14T04:00:13.627325Z

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.

source=arxiv_source observed=2026-07-14T03:58:35.317650Z digest=sha256:c58fb39f9e043ecb5454bf6b1060d4b3d9688507d4e0d5e07f29980a99400522

Observation d93f7f43-3470-443f-960f-81ea6df1ad1e · 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 Dynamical Masses of Low Mass Stars in the Taurus and Ophiuchus Star Forming Regions

Reference 131

Resolution
unresolved
no resolver link, observed 2026-08-01T22:01:28.613871Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T22:01:28.613871Z digest=sha256:07a5e9f0eda0900c20928f86cffb59d4263f44b133fd47d67631799bc94cf9bb