Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-07-01T15:57:40.411744Z
Paper Citation Record · LEDGER
The SPHERE infrared survey for exoplanets (SHINE) V. Full sample characterization
As of 6 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.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-05T06:32:48.257954+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-02T04:55:52.327681Z
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 2026-08-05T06:32:48.257954+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 2026-08-05T06:32:48.257954+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 2026-08-05T06:32:48.257954+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 2026-08-05T06:32:48.257954+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 2026-08-05T06:32:48.257954+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.