Paper Citation Record · LEDGER

The orbital period of the nova V1674 Her as observed with TESS

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2310.02220.

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

pith.paper-citation-record.v1
2310.02220 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T00:49:45.448718Z

measured 1 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

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External citation measurements

3
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation f74f7a94-9d4e-4fb8-8212-5b95fedbc5e1 · inbound

Optical observations of the fast nova V1674 Herculis cites this paper.

Optical observations of the fast nova V1674 Herculis The orbital period of the nova V1674 Her as observed with TESS

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-02T21:32:12.514505Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8c838e5a-37d3-41a3-8234-0a7c79262177 · inbound

X-ray spectroscopy mass constraints on V1674 Her: the fastest nova does not have a near-Chandrasekhar white dwarf cites this paper.

X-ray spectroscopy mass constraints on V1674 Her: the fastest nova does not have a near-Chandrasekhar white dwarf The orbital period of the nova V1674 Her as observed with TESS

Reference 31

Resolution: verified exact; arxiv_id, observed 2026-05-11T00:55:50.939977Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 358e3279-7d75-4b5b-9e64-b3c3fcdee4cc · inbound

TESS detection of periodic brightness variations during the rise of classical nova PGIR22akgylf cites this paper.

TESS detection of periodic brightness variations during the rise of classical nova PGIR22akgylf The orbital period of the nova V1674 Her as observed with TESS

Reference 68

Resolution: verified exact; arxiv_id, observed 2026-06-27T08:10:45.435147Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 806453b9-d4b1-4311-b5b4-64e7c525314a · inbound

An Optically Motivated Gamma-ray Study of Fermi-LAT Novae cites this paper.

An Optically Motivated Gamma-ray Study of Fermi-LAT Novae The orbital period of the nova V1674 Her as observed with TESS

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-12T00:49:45.448718Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.