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Paper Citation Record · LEDGER

Type Ia Supernova Rate Measurements to Redshift 2.5 from CANDELS : Searching for Prompt Explosions in the Early Universe

As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1401.7978.

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

pith.paper-citation-record.v1
1401.7978 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-20T06:33:59.587034+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T00:12:18.789271Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-27T18:01:08.168381Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
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  • 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 e424a88d-01d6-4d30-9f1a-121c5017201f · inbound

JWST Absorption-Line Analysis of UV-Bright Galaxies at $z=7.2-10.6$: Early Chemical Enrichment Traced by C, O, Mg, Al, Si, and Fe cites this paper.

JWST Absorption-Line Analysis of UV-Bright Galaxies at $z=7.2-10.6$: Early Chemical Enrichment Traced by C, O, Mg, Al, Si, and Fe Type Ia Supernova Rate Measurements to Redshift 2.5 from CANDELS : Searching for Prompt Explosions in the Early Universe

Reference 119

Resolution
verified exact
local_arxiv, observed 2026-06-27T18:01:08.170218Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:d08ebf85b02321859954ce7ead915480129e36f2b6019a9aa4888408797d1a4b

Observation b2ba7236-a905-4d4c-be28-2d433fb51e37 · inbound

ZTF SN Ia DR2 follow-up: early excess in Type Ia supernova light curves cites this paper.

ZTF SN Ia DR2 follow-up: early excess in Type Ia supernova light curves Type Ia Supernova Rate Measurements to Redshift 2.5 from CANDELS : Searching for Prompt Explosions in the Early Universe

Reference 268

Resolution
unresolved
no resolver link, observed 2026-08-01T06:02:17.792869Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T06:02:17.792869Z digest=sha256:c108177b217625859daedca1ffb4e6ec5ed6d14a508371a29b4e899c660a30ea

Observation 7cee9099-2832-4cac-902f-b4b87b5ce46a · inbound

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics cites this paper.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics Type Ia Supernova Rate Measurements to Redshift 2.5 from CANDELS : Searching for Prompt Explosions in the Early Universe

Reference 265

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:18.789271Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:18.789271Z digest=sha256:be459f059d66d45e12c7cffe3eb901abee2a058a8cebb7d435f73856bae8120c