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Paper Citation Record · LEDGER

WISE Y Dwarfs As Probes of the Brown Dwarf-Exoplanet Connection

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1401.1194.

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

pith.paper-citation-record.v1
1401.1194 v2

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 2026-08-18T06:34:40.430872+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T04:20:27.552111Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-02T05:56:40.252719Z

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 f568bbcd-4cfb-4950-9623-261ac11f7252 · inbound

Characterizing Transiting Exoplanet Atmospheres in the 2030s with the Hubble Space Telescope cites this paper.

Characterizing Transiting Exoplanet Atmospheres in the 2030s with the Hubble Space Telescope WISE Y Dwarfs As Probes of the Brown Dwarf-Exoplanet Connection

Reference 90

Resolution
metadata mismatch
local_arxiv, observed 2026-07-02T05:56:40.253998Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-06-28T07:59:01.949070Z digest=sha256:e96ea0ce657ed6aefe8be690853b2d73b39a83324e00ab543cf6be15ca49c800

Observation 29752af6-ba17-495b-873a-7cc6d8cfb5d8 · inbound

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf cites this paper.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf WISE Y Dwarfs As Probes of the Brown Dwarf-Exoplanet Connection

Reference 77

Resolution
unresolved
no resolver link, observed 2026-08-10T04:20:27.552111Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T04:20:27.552111Z digest=sha256:b8315eeb54596e81dc5e2f979c41c547b3be131b0d860fa3b9e93a6ba7f6ef66