Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-05-14T20:16:12.975192Z
Paper Citation Record · LEDGER
Ariel stellar characterisation IV. Fundamental parameters of 18 hot stars in the Ariel mission candidate sample
As of 6 August 2026, this Paper Citation Record lists 16 of 16 outbound references and 0 inbound Pith citation observations for arXiv:2605.12644.
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 2026-08-06T06:34:29.942622+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
16 of 16 outbound references displayed
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- verified fuzzy14
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- malformed identifier1
- metadata mismatch1
External citation measurements
No source-named external measurement is stored.
Outbound references
Observation f03310ef-bc2b-498b-b2b6-82598003a78d · outbound
This paper cites WASP-189b: an ultra-hot Jupiter transiting the bright A star HR 5599 in a polar orbit.
Ariel stellar characterisation IV. Fundamental parameters of 18 hot stars in the Ariel mission candidate sample WASP-189b: an ultra-hot Jupiter transiting the bright A star HR 5599 in a polar orbit
Reference 1
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-05-14T20:19:28.055324Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 00240082-ea1e-4b9f-9ef4-5b69ee8c0952 · outbound
This paper cites A dominant subsolar–antisolar wind circula- tion pattern has been suggested.
Ariel stellar characterisation IV. Fundamental parameters of 18 hot stars in the Ariel mission candidate sample A dominant subsolar–antisolar wind circula- tion pattern has been suggested
Reference 2
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-15T16:26:18.886931Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 2ce6ad06-7df1-4f26-a964-30843c41b134 · outbound
This paper cites (Zhou et al.
Reference 3
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-15T16:26:18.908612Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 496fce15-c44b-4dc5-9127-8a20c5dd9520 · outbound
This paper cites The planetary orbit is strongly misaligned (projected spin–orbit angleλ∼84 ◦).
Ariel stellar characterisation IV. Fundamental parameters of 18 hot stars in the Ariel mission candidate sample The planetary orbit is strongly misaligned (projected spin–orbit angleλ∼84 ◦)
Reference 4
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-15T16:26:18.912407Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation da232162-a7bf-4687-8dac-a6b245ea3f5c · outbound
This paper cites The system exhibits a near-perfect spin–orbit alignment (3.4◦ ±2.1 ◦).
Ariel stellar characterisation IV. Fundamental parameters of 18 hot stars in the Ariel mission candidate sample The system exhibits a near-perfect spin–orbit alignment (3.4◦ ±2.1 ◦)
Reference 5
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-15T16:26:18.904477Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 93584c1f-6462-429a-9add-732cdfbefcc7 · outbound
This paper cites KELT-21 A b has a well-aligned orbit; Kozai–Lidov oscilla- tions are therefore unlikely to have driven the migration.
Ariel stellar characterisation IV. Fundamental parameters of 18 hot stars in the Ariel mission candidate sample KELT-21 A b has a well-aligned orbit; Kozai–Lidov oscilla- tions are therefore unlikely to have driven the migration
Reference 6
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-15T16:26:18.891657Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 86ad3478-8e73-40a6-a395-e92b0f47e0be · outbound
This paper cites The mass-loss rate is approximately 10 12.8±0.3 g s −1; the planet could lose its atmosphere within∼600 Myr.
Ariel stellar characterisation IV. Fundamental parameters of 18 hot stars in the Ariel mission candidate sample The mass-loss rate is approximately 10 12.8±0.3 g s −1; the planet could lose its atmosphere within∼600 Myr
Reference 7
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-15T16:26:18.896244Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 8b0b2c0f-a022-4d02-a1ad-50d641d1b936 · outbound
This paper cites The planet has an oblique orbit.
Ariel stellar characterisation IV. Fundamental parameters of 18 hot stars in the Ariel mission candidate sample The planet has an oblique orbit
Reference 8
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-15T16:26:18.900527Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation eade8454-67c5-4393-8b93-ea3bc4b89c4c · outbound
This paper cites (Hooton et al.
Ariel stellar characterisation IV. Fundamental parameters of 18 hot stars in the Ariel mission candidate sample (Hooton et al
Reference 9
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-15T16:26:18.878376Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 2dfebd3e-4c9e-4077-9509-fa1861152a59 · outbound
This paper cites The planet has very highly misaligned, retrograde orbit (λ= 250.34◦ ±0.14◦).
Ariel stellar characterisation IV. Fundamental parameters of 18 hot stars in the Ariel mission candidate sample The planet has very highly misaligned, retrograde orbit (λ= 250.34◦ ±0.14◦)
Reference 10
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-15T16:26:18.882449Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation cede83ab-ed1c-4c6a-aa5a-c8a88022f0bc · outbound
This paper cites No atmosphere has yet been detected for the planet.
Ariel stellar characterisation IV. Fundamental parameters of 18 hot stars in the Ariel mission candidate sample No atmosphere has yet been detected for the planet
Reference 11
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-15T16:26:18.866187Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation c9200bbd-cb78-4150-bf67-10173d107bed · outbound
This paper cites (Cabot et al.
Ariel stellar characterisation IV. Fundamental parameters of 18 hot stars in the Ariel mission candidate sample (Cabot et al
Reference 12
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-15T16:26:18.874719Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 4d2855ba-fdd2-415a-a51d-298736cc6691 · outbound
This paper cites The planet’s atmosphere appears carbon-depleted and shows titanium de- pletion.
Ariel stellar characterisation IV. Fundamental parameters of 18 hot stars in the Ariel mission candidate sample The planet’s atmosphere appears carbon-depleted and shows titanium de- pletion
Reference 13
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-15T16:26:18.856997Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 0bffdb8f-92e0-4bc1-b477-4cee55deec51 · outbound
This paper cites Upper-atmosphere studies indicate Mg II and possibly Fe II, with evidence for escaping magnesium and temperatures around 1.5×10 4 K.
Ariel stellar characterisation IV. Fundamental parameters of 18 hot stars in the Ariel mission candidate sample Upper-atmosphere studies indicate Mg II and possibly Fe II, with evidence for escaping magnesium and temperatures around 1.5×10 4 K
Reference 14
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-15T16:26:18.916737Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 97940340-50d5-4d12-a01f-44ec0b45253e · outbound
This paper cites W ASP-33 A is a non-radialδScuti pulsator (a γDoradus–δScuti hybrid candidate).
Ariel stellar characterisation IV. Fundamental parameters of 18 hot stars in the Ariel mission candidate sample W ASP-33 A is a non-radialδScuti pulsator (a γDoradus–δScuti hybrid candidate)
Reference 15
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-05-15T16:26:18.862605Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation eb45e092-0dad-444c-920a-0a26a8c1b4af · outbound
This paper cites Stellar and planetary parameters are adopted from the cited discovery and follow-up papers.
Ariel stellar characterisation IV. Fundamental parameters of 18 hot stars in the Ariel mission candidate sample Stellar and planetary parameters are adopted from the cited discovery and follow-up papers
Reference 16
- Resolution
- malformed identifier
- raw_fallback, observed 2026-05-15T16:26:18.870972Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Pith citing papers
No inbound Pith citation observations are available.