Paper Citation Record · LEDGER

Resonant structures in exozodiacal clouds created by exo-Earths in the habitable zone of late-type stars

As of 7 August 2026, this Paper Citation Record lists 10 of 10 outbound references and 0 inbound Pith citation observations for arXiv:2511.17872.

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

pith.paper-citation-record.v1
2511.17872 v1

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measured 10 of 10 reference resolution

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Source: paper_references, paper_reference_links, observed 2026-08-03T20:56:03.878267Z

measured 10 of 10 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 0 of 0 inbound itemization

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measured 0 of 1 external citation measurements

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Source: cited_works

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10 of 10 outbound references displayed

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Outbound references

Observation b444a9e6-5088-46dc-a3c5-dd291b9b98af · outbound

This paper cites 2006, PhD thesis, University of Liege, Belgium Baraffe, I., Homeier, D., Allard, F., & Chabrier, G.

Resonant structures in exozodiacal clouds created by exo-Earths in the habitable zone of late-type stars 2006, PhD thesis, University of Liege, Belgium Baraffe, I., Homeier, D., Allard, F., & Chabrier, G

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-03T20:56:02.263726Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 526020f4-b8a6-435a-99db-481adc6dbb7a · outbound

This paper cites K4 (yellow) and M4 (red) appear to have one fewer point because their 0.3µm and 1µm data replace the 0.1µm points respectively, causing overlap (see Section 2.2.2).

Resonant structures in exozodiacal clouds created by exo-Earths in the habitable zone of late-type stars K4 (yellow) and M4 (red) appear to have one fewer point because their 0.3µm and 1µm data replace the 0.1µm points respectively, causing overlap (see Section 2.2.2)

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-03T20:56:03.708992Z

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Observation a6562918-29f5-4f2a-882f-46876f2afd93 · outbound

This paper cites an unresolved cited work.

Resonant structures in exozodiacal clouds created by exo-Earths in the habitable zone of late-type stars Unresolved cited work

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-03T20:56:02.839097Z

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Observation 8c33bcf3-e0b3-4f9e-8b8d-d920e16c0a8f · outbound

This paper cites Nev- ertheless, the semi-analytical⟨C τ⟩values can be used to approx- imately estimateτ BG·⟨Cτ⟩when the background level of dust is given.

Resonant structures in exozodiacal clouds created by exo-Earths in the habitable zone of late-type stars Nev- ertheless, the semi-analytical⟨C τ⟩values can be used to approx- imately estimateτ BG·⟨Cτ⟩when the background level of dust is given

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-03T20:56:03.332423Z

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Observation 27e68963-67a7-4220-863d-d021b6c7680d · outbound

This paper cites See the caption of Fig.

Resonant structures in exozodiacal clouds created by exo-Earths in the habitable zone of late-type stars See the caption of Fig

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-03T20:56:03.596135Z

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Observation 592a51e9-0a99-40c1-a82a-46421a05d0d6 · outbound

This paper cites In this scenario, exozodi resonant structures in M-type systems would clearly pose the least hindrance on MIR interferometric detection of exo-Earths.

Resonant structures in exozodiacal clouds created by exo-Earths in the habitable zone of late-type stars In this scenario, exozodi resonant structures in M-type systems would clearly pose the least hindrance on MIR interferometric detection of exo-Earths

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-03T20:56:03.878267Z

Source-reported events for the cited work

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Observation 5728980d-b23a-443c-ae7f-34740f861176 · outbound

This paper cites Dynamics of Exozodiacal Clouds.

Resonant structures in exozodiacal clouds created by exo-Earths in the habitable zone of late-type stars Dynamics of Exozodiacal Clouds

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-03T20:56:02.371594Z

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Observation 08cb548a-1be9-4881-b849-cc7045829e74 · outbound

This paper cites an unresolved cited work.

Resonant structures in exozodiacal clouds created by exo-Earths in the habitable zone of late-type stars Unresolved cited work

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-03T20:56:03.083621Z

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Observation 66803501-e344-4d00-8055-b7a494e2f475 · outbound

This paper cites (2005) on a young M0 dwarf AU Mic of∼15 Myr age withM ∗ =0.5M ⊙,L ∗ =1.3L ⊙, assuming vSW ∼400 km/s and ˙M∗ ∼1000 ˙M⊙.

Resonant structures in exozodiacal clouds created by exo-Earths in the habitable zone of late-type stars (2005) on a young M0 dwarf AU Mic of∼15 Myr age withM ∗ =0.5M ⊙,L ∗ =1.3L ⊙, assuming vSW ∼400 km/s and ˙M∗ ∼1000 ˙M⊙

Reference 2015

Resolution: unresolved; no resolver link, observed 2026-08-03T20:56:02.667291Z

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Observation 3ca6cab2-3202-4593-a8b8-59285238ab7e · outbound

This paper cites This value is derived from observations (e.g., Metchev et al.

Resonant structures in exozodiacal clouds created by exo-Earths in the habitable zone of late-type stars This value is derived from observations (e.g., Metchev et al

Reference 2024

Resolution: unresolved; no resolver link, observed 2026-08-03T20:56:02.540862Z

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Pith citing papers

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