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Paper Citation Record · LEDGER

A Spitzer Infrared Spectrograph (IRS) Spectral Sequence of M, L, and T Dwarfs

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0605639.

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

pith.paper-citation-record.v1
astro-ph/0605639 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 2026-08-18T06:34:40.430872+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-28T08:01:46.706108Z

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 2d07c37c-63dc-47d1-8918-42c1549f346d · 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 A Spitzer Infrared Spectrograph (IRS) Spectral Sequence of M, L, and T Dwarfs

Reference 266

Resolution
verified exact
local_arxiv, observed 2026-06-28T08:01:46.707493Z

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=2026-07-11T11:50:26.030339Z digest=sha256:39a3a378d2df8d450bd8566bd8f02f2db9abb30aae0b8432e36d85e869f34233

Observation 7b5984f8-05d0-4299-830e-1a99e11c8ae9 · inbound

Studying hot evolved stars with ultraviolet spectroscopy cites this paper.

Studying hot evolved stars with ultraviolet spectroscopy A Spitzer Infrared Spectrograph (IRS) Spectral Sequence of M, L, and T Dwarfs

Reference 203

Resolution
verified exact
local_arxiv, observed 2026-06-28T03:11:31.011464Z

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=2026-07-11T11:50:26.030339Z digest=sha256:0b8b129366dba2e0a99e1e66a8664314b1969e928d387363b32a6ec47a743cf4