Paper Citation Record · LEDGER

Improved Distances to Type Ia Supernovae with Multicolor Light Curve Shapes: MLCS2k2

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:astro-ph/0612666.

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pith.paper-citation-record.v1
astro-ph/0612666 v1

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measured 0 of 0 reference resolution

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measured 6 of 6 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 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T13:54:40.952501Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-29T15:13:32.165022Z

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation a160b769-b751-4b1a-83ef-065156da278e · inbound

On the cosmological performance of photometrically classified supernovae with machine learning cites this paper.

On the cosmological performance of photometrically classified supernovae with machine learning Improved Distances to Type Ia Supernovae with Multicolor Light Curve Shapes: MLCS2k2

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-14T13:54:40.952501Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 09dee29d-82e7-4c08-b59f-3fde1c6aca26 · inbound

Cosmology-Independent Constraints on the Etherington Relation and SNeIa Absolute Magnitude Evolution from DESI-DR2 cites this paper.

Cosmology-Independent Constraints on the Etherington Relation and SNeIa Absolute Magnitude Evolution from DESI-DR2 Improved Distances to Type Ia Supernovae with Multicolor Light Curve Shapes: MLCS2k2

Reference 7

Resolution: verified exact; local_arxiv, observed 2026-05-13T20:23:13.835538Z

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.

Observation 529cd872-305f-47d2-8369-8c088831a881 · inbound

Modeling the probability distribution for cosmological analysis with photometrically classified samples cites this paper.

Modeling the probability distribution for cosmological analysis with photometrically classified samples Improved Distances to Type Ia Supernovae with Multicolor Light Curve Shapes: MLCS2k2

Reference 6

Resolution: verified exact; local_arxiv, observed 2026-05-20T15:43:26.978469Z

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.

Observation f4fd6a74-16be-4159-870e-c7fe7cc63256 · inbound

Mapping the Universe as a Bianchi I cosmology with Gaia data cites this paper.

Mapping the Universe as a Bianchi I cosmology with Gaia data Improved Distances to Type Ia Supernovae with Multicolor Light Curve Shapes: MLCS2k2

Reference 128

Resolution: verified exact; local_arxiv, observed 2026-06-29T15:13:32.166280Z

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.

Observation ea0f1818-7de8-425f-991a-aff9c84b6a49 · inbound

The colour variability of low-z SNe Ia is entirely explained by dust cites this paper.

The colour variability of low-z SNe Ia is entirely explained by dust Improved Distances to Type Ia Supernovae with Multicolor Light Curve Shapes: MLCS2k2

Reference 7

Resolution: verified exact; local_arxiv, observed 2026-06-27T23:51:25.146397Z

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.

Observation 71aeddfa-75ac-450b-a41f-8db35297d2cb · inbound

Can cosmic voids ease the Hubble tension? Local expansion in $w_0w_a$CDM cites this paper.

Can cosmic voids ease the Hubble tension? Local expansion in $w_0w_a$CDM Improved Distances to Type Ia Supernovae with Multicolor Light Curve Shapes: MLCS2k2

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-01T10:23:40.060520Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.