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Paper Citation Record · LEDGER

Measurement of \Omega_m, \Omega_{\Lambda} from a blind analysis of Type Ia supernovae with CMAGIC: Using color information to verify the acceleration of the Universe

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0602411.

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

pith.paper-citation-record.v1
astro-ph/0602411 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 2026-08-07T06:34:17.273281+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 2026-05-25T03:05:16.597767Z

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 9dcf8516-ebad-424a-a701-2375d74b45e7 · inbound

cloelib: A Flexible Python Library for Computing Cosmological Observables in the Euclid Era cites this paper.

cloelib: A Flexible Python Library for Computing Cosmological Observables in the Euclid Era Measurement of \Omega_m, \Omega_{\Lambda} from a blind analysis of Type Ia supernovae with CMAGIC: Using color information to verify the acceleration of the Universe

Reference 14

Resolution
verified exact
local_arxiv, observed 2026-05-25T03:05:16.600624Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:1f49ee6059d52c851b7514087ca881211b2a323b4ab7f9af79ca4567e6792cee

Observation 6861a0f9-2ff5-43a0-aa20-7469f49b5f92 · inbound

cloelike: A Python Library for Cosmological Likelihood Inference in the Euclid Era cites this paper.

cloelike: A Python Library for Cosmological Likelihood Inference in the Euclid Era Measurement of \Omega_m, \Omega_{\Lambda} from a blind analysis of Type Ia supernovae with CMAGIC: Using color information to verify the acceleration of the Universe

Reference 17

Resolution
verified exact
local_arxiv, observed 2026-05-25T03:00:15.153562Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:c8f45e43819ff9604162c20625d61d575dfb8bd4c33c766250574190ba4e2710