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Paper Citation Record · LEDGER

MINDS: Intertwined evolution of dust and gas in large planet-forming disks. A diversity driven by halted pebble drift?

As of 4 August 2026, this Paper Citation Record lists 6 of 6 outbound references and 4 inbound Pith citation observations for arXiv:2604.21803.

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

pith.paper-citation-record.v1
2604.21803 v1

Coverage vector

measured 6 of 6 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-05-08T13:37:06.235546Z

measured 10 of 10 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-03T06:30:56.289259+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T04:27:12.862141Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T12:15:01.137692Z

Reference resolution

6 of 6 outbound references displayed

  • verified exact1
  • verified fuzzy4
  • unresolved1
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation c0317b09-4cf4-4245-830a-ac0581f97b34 · outbound

This paper cites MINDS: The very low-mass star and brown dwarf sample. Detections and trends in the inner disk gas.

MINDS: Intertwined evolution of dust and gas in large planet-forming disks. A diversity driven by halted pebble drift? MINDS: The very low-mass star and brown dwarf sample. Detections and trends in the inner disk gas

Reference 1

Resolution
verified exact
arxiv_id, observed 2026-05-11T18:51:08.019277Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-03T06:30:56.289259+00:00.

source=pdf_text observed=2026-05-08T13:37:06.235546Z digest=sha256:b5d0e99ab2b7d947354a61f3ecfae10e1f0d737a27cc4d84d20d6e30c06ca8ff

Observation e9af4c30-4ad8-43a5-98b6-9cb5f5b04506 · outbound

This paper cites 2017; Kalyaan et al.

MINDS: Intertwined evolution of dust and gas in large planet-forming disks. A diversity driven by halted pebble drift? 2017; Kalyaan et al

Reference 2

Resolution
verified fuzzy
raw_fallback, observed 2026-05-26T12:17:19.864607Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-03T06:30:56.289259+00:00.

source=pdf_text observed=2026-05-08T13:37:06.235546Z digest=sha256:c00447b9f44823dd4acf5548f9df34be2207cddc67102dbb334385f7413482d0

Observation 8aa33efc-3c4a-4a63-86a6-08215f595d88 · outbound

This paper cites an unresolved cited work.

MINDS: Intertwined evolution of dust and gas in large planet-forming disks. A diversity driven by halted pebble drift? Unresolved cited work

Reference 3

Resolution
unresolved
raw_fallback, observed 2026-05-26T12:17:19.851331Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-03T06:30:56.289259+00:00.

source=pdf_text observed=2026-05-08T13:37:06.235546Z digest=sha256:4c2cdf1fd003001b17094ef4048eafee10601152d0599d2ad3661b0770f12b3b

Observation bc7e98e5-29f6-4a1a-ba74-db5a4d2888a6 · outbound

This paper cites Italic values correspond to optically thin emission where column density and emitting area are degenerate; uncertainties are therefore not provided.

MINDS: Intertwined evolution of dust and gas in large planet-forming disks. A diversity driven by halted pebble drift? Italic values correspond to optically thin emission where column density and emitting area are degenerate; uncertainties are therefore not provided

Reference 4

Resolution
verified fuzzy
raw_fallback, observed 2026-05-26T12:17:19.846934Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-03T06:30:56.289259+00:00.

source=pdf_text observed=2026-05-08T13:37:06.235546Z digest=sha256:4456971c50f30a7515a44ff7291e5fefbb6812bd31a99fd09320f92b115a35eb

Observation 33fc1fc0-2a00-41c1-9ebd-a644b92266cd · outbound

This paper cites C.2 the (C/O) adv ratio of the advected material for various amount of icy grains assuming a gas with high C/O and various values of O/H.

MINDS: Intertwined evolution of dust and gas in large planet-forming disks. A diversity driven by halted pebble drift? C.2 the (C/O) adv ratio of the advected material for various amount of icy grains assuming a gas with high C/O and various values of O/H

Reference 5

Resolution
verified fuzzy
raw_fallback, observed 2026-05-26T12:17:19.856177Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-03T06:30:56.289259+00:00.

source=pdf_text observed=2026-05-08T13:37:06.235546Z digest=sha256:7d7af2d62dc6ff558f4d141167ba26754d006a0bac8d2d2b80a52c0801403cb9

Observation 27612100-6856-4d26-a1d9-9167121d4cdc · outbound

This paper cites C 2H(3-2) flux Ref.

MINDS: Intertwined evolution of dust and gas in large planet-forming disks. A diversity driven by halted pebble drift? C 2H(3-2) flux Ref

Reference 6

Resolution
verified fuzzy
raw_fallback, observed 2026-05-26T12:17:19.860641Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-03T06:30:56.289259+00:00.

source=pdf_text observed=2026-05-08T13:37:06.235546Z digest=sha256:19b0eefde1a7f15cd7a3d5ff92b9a69134e4bcd4745680bbcb9b529fb69b8ec9

Pith citing papers

Observation d95538bc-e8a7-4ad1-ba81-c079927c00a9 · inbound

Chemistry and IR emission of acetylene in planet-forming regions of T Tauri disks. Impact of elemental abundances and dust properties cites this paper.

Chemistry and IR emission of acetylene in planet-forming regions of T Tauri disks. Impact of elemental abundances and dust properties MINDS: Intertwined evolution of dust and gas in large planet-forming disks. A diversity driven by halted pebble drift?

Reference 2

Resolution
verified exact
local_arxiv, observed 2026-05-20T00:57:53.732096Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-03T06:30:56.289259+00:00.

source=arxiv_source observed=2026-05-20T00:56:12.739349Z digest=sha256:b5fd56a42c46e320f97369c72e2add6b0e31cbc51fa25f44d8d9fc4e438a4d21

Observation ec6ec60a-8f58-4673-8d10-24f0932c2834 · inbound

Chemistry and IR emission of acetylene in planet-forming regions of T Tauri disks. Impact of elemental abundances and dust properties cites this paper.

Chemistry and IR emission of acetylene in planet-forming regions of T Tauri disks. Impact of elemental abundances and dust properties MINDS: Intertwined evolution of dust and gas in large planet-forming disks. A diversity driven by halted pebble drift?

Reference 2

Resolution
verified exact
local_arxiv, observed 2026-05-20T08:38:09.746921Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-03T06:30:56.289259+00:00.

source=arxiv_source observed=2026-05-20T08:33:54.153755Z digest=sha256:37f3df3e8a945ff22aa47a2f0919df80a7e2f08c41f432c8c6323263f63eaff2

Observation dd0a1ef4-d245-4d4a-a20f-48a90ddc6456 · inbound

Molecular Similarity and Water Diversity in Coeval Binary Disks: JWST/MIRI Observations of Sz 65 and Sz 66 cites this paper.

Molecular Similarity and Water Diversity in Coeval Binary Disks: JWST/MIRI Observations of Sz 65 and Sz 66 MINDS: Intertwined evolution of dust and gas in large planet-forming disks. A diversity driven by halted pebble drift?

Reference 77

Resolution
verified exact
local_arxiv, observed 2026-06-29T10:23:17.153175Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-03T06:30:56.289259+00:00.

source=pdf_text observed=2026-06-29T10:20:14.797938Z digest=sha256:55fa1cc5eec08e73636487a79eede1a673ddfe9b134eac0ad79d4af7b0cc3c5f

Observation c13935b0-ea3f-4a8e-9bcd-59f8d53d2f5e · inbound

The JDISC Survey: Inner Disk Chemistry of Class I/FS Disks and Tentative Evidence for Early Pebble Drift cites this paper.

The JDISC Survey: Inner Disk Chemistry of Class I/FS Disks and Tentative Evidence for Early Pebble Drift MINDS: Intertwined evolution of dust and gas in large planet-forming disks. A diversity driven by halted pebble drift?

Reference 105

Resolution
unresolved
no resolver link, observed 2026-08-01T04:27:12.862141Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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