Paper Citation Record · LEDGER

The SPHERE infrared survey for exoplanets (SHINE) V. Full sample characterization

As of 11 August 2026, this Paper Citation Record lists 5 of 5 outbound references and 2 inbound Pith citation observations for arXiv:2605.27247.

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

pith.paper-citation-record.v1
2605.27247 v2

Coverage vector

measured 5 of 5 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-07-01T15:57:40.411744Z

measured 7 of 7 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T04:55:52.327681Z

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

5 of 5 outbound references displayed

verified exact0
verified fuzzy3
unresolved0
parse uncertain0
malformed identifier2
metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation bdfaf3d7-4045-404f-ab02-7ba8bff22ac1 · outbound

This paper cites The star has AstroSpectroSB1 solution in Gaia-NSS, with nominal mass in the substellar regime (Marcussen & Albrecht 2023).

The SPHERE infrared survey for exoplanets (SHINE) V. Full sample characterization The star has AstroSpectroSB1 solution in Gaia-NSS, with nominal mass in the substellar regime (Marcussen & Albrecht 2023)

Reference 1

Resolution: verified fuzzy; raw_fallback, observed 2026-07-06T11:22:20.678848Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation ccdd8768-d750-4219-a1f5-a03abb194f8c · outbound

This paper cites is probable very wide companion (Majidi et al. 2020). HIP 76395.The star is classified as a close, equal-mass binary (ρ=0.2.

The SPHERE infrared survey for exoplanets (SHINE) V. Full sample characterization is probable very wide companion (Majidi et al. 2020). HIP 76395.The star is classified as a close, equal-mass binary (ρ=0.2

Reference 2

Resolution: malformed identifier; raw_fallback, observed 2026-07-06T11:22:20.673605Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 1d263214-3d1e-4f05-ae0e-a7ed730fc77c · outbound

This paper cites (2024) argue instead for membership to the Theia92 group, with an age of 35 Myr.

The SPHERE infrared survey for exoplanets (SHINE) V. Full sample characterization (2024) argue instead for membership to the Theia92 group, with an age of 35 Myr

Reference 3

Resolution: verified fuzzy; raw_fallback, observed 2026-07-06T11:22:20.676186Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 979cd571-3108-4188-8aea-90228b85c4a2 · outbound

This paper cites , 2MASS J05195412-0723359, which is itself a close visual binary. AF Hor=2MASS J02414730-5259306.This star has a close (0.1.

The SPHERE infrared survey for exoplanets (SHINE) V. Full sample characterization , 2MASS J05195412-0723359, which is itself a close visual binary. AF Hor=2MASS J02414730-5259306.This star has a close (0.1

Reference 4

Resolution: verified fuzzy; raw_fallback, observed 2026-07-06T11:22:20.681149Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 3b54e339-585d-4223-944d-11a757dc861b · outbound

This paper cites , with slightly discrepant astrometric parameters likely due to the close companion. If the X-ray source 1RXS J030750.4-275012 is associated with the early type compo- nent (ρ=20.7.

The SPHERE infrared survey for exoplanets (SHINE) V. Full sample characterization , with slightly discrepant astrometric parameters likely due to the close companion. If the X-ray source 1RXS J030750.4-275012 is associated with the early type compo- nent (ρ=20.7

Reference 5

Resolution: malformed identifier; raw_fallback, observed 2026-07-06T11:22:20.683670Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Pith citing papers

Observation 964582ef-62a1-4cac-858b-8526232f19a2 · inbound

SAXO+, the second-stage adaptive optics for SPHERE: NCPA compensation and dark-hole loop with a pyramid wavefront sensor cites this paper.

SAXO+, the second-stage adaptive optics for SPHERE: NCPA compensation and dark-hole loop with a pyramid wavefront sensor The SPHERE infrared survey for exoplanets (SHINE) V. Full sample characterization

Reference 6

Resolution: unresolved; no resolver link, observed 2026-07-14T14:07:35.588680Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2dbb0b12-9981-4638-a5ed-ba6aed6ca9c8 · inbound

SaNDi-SHoP: Searching for Satellites'N'Disks with a Star-Hopping Program II. Spectrophotometric analysis and orbital monitoring of directly imaged companions cites this paper.

SaNDi-SHoP: Searching for Satellites'N'Disks with a Star-Hopping Program II. Spectrophotometric analysis and orbital monitoring of directly imaged companions The SPHERE infrared survey for exoplanets (SHINE) V. Full sample characterization

Reference 130

Resolution: unresolved; no resolver link, observed 2026-08-02T04:55:52.327681Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.