Paper Citation Record · LEDGER

ALMA-IMF. XXI.: N$_2$H$^+$ kinematics in the G012.80 protocluster: Evidence for filament rotation and evolution

As of 21 August 2026, this Paper Citation Record lists 26 of 26 outbound references and 2 inbound Pith citation observations for arXiv:2510.03447.

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

pith.paper-citation-record.v1
2510.03447 v2

Coverage vector

measured 26 of 26 reference resolution

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measured 28 of 28 standing notices

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Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T07:32:02.299613Z

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

Source: pith, observed 2026-08-02T12:16:14.744948Z

Reference resolution

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External citation measurements

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Outbound references

Observation 9d8c8997-16f8-4344-a288-6826f8e8e255 · outbound

This paper cites an unresolved cited work.

ALMA-IMF. XXI.: N$_2$H$^+$ kinematics in the G012.80 protocluster: Evidence for filament rotation and evolution Unresolved cited work

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-04T12:27:29.185521Z

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Unavailable: canonical work link unavailable.

Observation b83425c1-2b0b-4604-948c-8d81fe8d2d52 · outbound

This paper cites an unresolved cited work.

ALMA-IMF. XXI.: N$_2$H$^+$ kinematics in the G012.80 protocluster: Evidence for filament rotation and evolution Unresolved cited work

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-04T12:27:29.193518Z

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Unavailable: canonical work link unavailable.

Observation f51e0b85-0956-489b-af96-1bad4cf1ccaa · outbound

This paper cites an unresolved cited work.

ALMA-IMF. XXI.: N$_2$H$^+$ kinematics in the G012.80 protocluster: Evidence for filament rotation and evolution Unresolved cited work

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-04T12:27:29.210925Z

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Observation 723223cc-cd9e-4105-9340-b817c455825f · outbound

This paper cites Andrews, North Haugh, St.

ALMA-IMF. XXI.: N$_2$H$^+$ kinematics in the G012.80 protocluster: Evidence for filament rotation and evolution Andrews, North Haugh, St

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-04T12:27:29.223027Z

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Observation 446d16b2-d9f1-4fe1-bfb6-d4005ea40428 · outbound

This paper cites Grenoble Alpes, CNRS, IPAG, 38000 Grenoble, France.

ALMA-IMF. XXI.: N$_2$H$^+$ kinematics in the G012.80 protocluster: Evidence for filament rotation and evolution Grenoble Alpes, CNRS, IPAG, 38000 Grenoble, France

Reference 5

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Observation 95c17f34-0ee6-4cf5-b540-1f748ba015b7 · outbound

This paper cites Fermi 5, I-50125 Firenze, Italy.

ALMA-IMF. XXI.: N$_2$H$^+$ kinematics in the G012.80 protocluster: Evidence for filament rotation and evolution Fermi 5, I-50125 Firenze, Italy

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-04T12:27:29.237877Z

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Observation 712128a3-85e5-4f91-8780-7dbc3af4737f · outbound

This paper cites Bordeaux, CNRS, B18N, allée Geoffroy Saint-Hilaire, 33615 Pessac, France.

ALMA-IMF. XXI.: N$_2$H$^+$ kinematics in the G012.80 protocluster: Evidence for filament rotation and evolution Bordeaux, CNRS, B18N, allée Geoffroy Saint-Hilaire, 33615 Pessac, France

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-04T12:27:29.253292Z

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Observation 936f6c3c-a449-4e30-a23b-27fe21458c0a · outbound

This paper cites an unresolved cited work.

ALMA-IMF. XXI.: N$_2$H$^+$ kinematics in the G012.80 protocluster: Evidence for filament rotation and evolution Unresolved cited work

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-04T12:27:29.266423Z

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Observation 8da46211-11f7-46d7-902c-5c6be4ad8d4a · outbound

This paper cites an unresolved cited work.

ALMA-IMF. XXI.: N$_2$H$^+$ kinematics in the G012.80 protocluster: Evidence for filament rotation and evolution Unresolved cited work

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-04T12:27:29.272044Z

Source-reported events for the cited work

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Observation 5c80184d-c6f9-48ad-bef2-879d1dc972e7 · outbound

This paper cites an unresolved cited work.

ALMA-IMF. XXI.: N$_2$H$^+$ kinematics in the G012.80 protocluster: Evidence for filament rotation and evolution Unresolved cited work

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-04T12:27:29.278462Z

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Observation 8662ebff-d299-4d34-bc73-6f381ac63aa1 · outbound

This paper cites an unresolved cited work.

ALMA-IMF. XXI.: N$_2$H$^+$ kinematics in the G012.80 protocluster: Evidence for filament rotation and evolution Unresolved cited work

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-04T12:27:29.288863Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 48300b5d-cf67-48bb-abdf-12d14df3b3ed · outbound

This paper cites an unresolved cited work.

ALMA-IMF. XXI.: N$_2$H$^+$ kinematics in the G012.80 protocluster: Evidence for filament rotation and evolution Unresolved cited work

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-04T12:27:29.296476Z

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Observation 99e5c8ae-60ee-4360-85f7-cd5612407ad1 · outbound

This paper cites an unresolved cited work.

ALMA-IMF. XXI.: N$_2$H$^+$ kinematics in the G012.80 protocluster: Evidence for filament rotation and evolution Unresolved cited work

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-04T12:27:29.313100Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 66ba8c27-14ad-40c2-afe3-d0a92627a4c4 · outbound

This paper cites an unresolved cited work.

ALMA-IMF. XXI.: N$_2$H$^+$ kinematics in the G012.80 protocluster: Evidence for filament rotation and evolution Unresolved cited work

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-04T12:27:29.328076Z

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Observation d0da72a9-10d3-40c4-b5e9-e03cddb0c66e · outbound

This paper cites 2010, ApJ, 725, 17.

ALMA-IMF. XXI.: N$_2$H$^+$ kinematics in the G012.80 protocluster: Evidence for filament rotation and evolution 2010, ApJ, 725, 17

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-04T12:27:29.152285Z

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Observation a2801958-ebc5-4826-a060-93a2c30925b6 · outbound

This paper cites an unresolved cited work.

ALMA-IMF. XXI.: N$_2$H$^+$ kinematics in the G012.80 protocluster: Evidence for filament rotation and evolution Unresolved cited work

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-04T12:27:29.344739Z

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Observation a517090e-665f-404e-b873-5eb8f3e2cfee · outbound

This paper cites an unresolved cited work.

ALMA-IMF. XXI.: N$_2$H$^+$ kinematics in the G012.80 protocluster: Evidence for filament rotation and evolution Unresolved cited work

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-04T12:27:29.338987Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5a16a5ae-7334-4ccd-b1f8-0117fd47ec44 · outbound

This paper cites an unresolved cited work.

ALMA-IMF. XXI.: N$_2$H$^+$ kinematics in the G012.80 protocluster: Evidence for filament rotation and evolution Unresolved cited work

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-04T12:27:29.358008Z

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Unavailable: canonical work link unavailable.

Observation 2374d7f4-7ce5-487a-b9d0-7c0d99d425dc · outbound

This paper cites an unresolved cited work.

ALMA-IMF. XXI.: N$_2$H$^+$ kinematics in the G012.80 protocluster: Evidence for filament rotation and evolution Unresolved cited work

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-04T12:27:29.376462Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ebcc2415-13b1-4d19-8c64-c21b60677aee · outbound

This paper cites Specifically, we smooth the x-axis of the ridgeline, us- ing a window size of 1 pixel (the same window size was used to align filaments with respect to the column density).

ALMA-IMF. XXI.: N$_2$H$^+$ kinematics in the G012.80 protocluster: Evidence for filament rotation and evolution Specifically, we smooth the x-axis of the ridgeline, us- ing a window size of 1 pixel (the same window size was used to align filaments with respect to the column density)

Reference 22

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Observation ffb24228-d675-4ef5-bff9-ab6167105b9a · outbound

This paper cites an unresolved cited work.

ALMA-IMF. XXI.: N$_2$H$^+$ kinematics in the G012.80 protocluster: Evidence for filament rotation and evolution Unresolved cited work

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-04T12:27:29.397303Z

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Observation 483031ac-a913-453a-bd40-7f1c24ee2cf1 · outbound

This paper cites an unresolved cited work.

ALMA-IMF. XXI.: N$_2$H$^+$ kinematics in the G012.80 protocluster: Evidence for filament rotation and evolution Unresolved cited work

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-04T12:27:29.407727Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d8032cf0-4eae-4303-93e2-5dbc108957df · outbound

This paper cites (2024) H 2 pixel scale.

ALMA-IMF. XXI.: N$_2$H$^+$ kinematics in the G012.80 protocluster: Evidence for filament rotation and evolution (2024) H 2 pixel scale

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-04T12:27:29.416208Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b06827ac-1b9d-40dd-9d43-dbdaeedca576 · outbound

This paper cites That is, all pixels with values<1 in the binary mask are ex- cluded from the regridded N2H+ column density map.

ALMA-IMF. XXI.: N$_2$H$^+$ kinematics in the G012.80 protocluster: Evidence for filament rotation and evolution That is, all pixels with values<1 in the binary mask are ex- cluded from the regridded N2H+ column density map

Reference 26

Resolution: malformed identifier; no resolver link, observed 2026-08-04T12:27:29.427692Z

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Unavailable: canonical work link unavailable.

Observation 5e2703d1-4126-45d2-8053-9dde93da3d1f · outbound

This paper cites Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM.

ALMA-IMF. XXI.: N$_2$H$^+$ kinematics in the G012.80 protocluster: Evidence for filament rotation and evolution Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM

Reference 153

Resolution: unresolved; no resolver link, observed 2026-08-04T12:27:29.167221Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a74061c7-6207-4834-8b59-1405d9c7006c · outbound

This paper cites Gaia: Orion's Integral Shaped Filament is a Standing Wave.

ALMA-IMF. XXI.: N$_2$H$^+$ kinematics in the G012.80 protocluster: Evidence for filament rotation and evolution Gaia: Orion's Integral Shaped Filament is a Standing Wave

Reference 2220

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Pith citing papers

Observation 06e87d6f-9a8e-4f7d-8ba2-1634d9f03c5a · inbound

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching cites this paper.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching ALMA-IMF. XXI.: N$_2$H$^+$ kinematics in the G012.80 protocluster: Evidence for filament rotation and evolution

Reference 46

Resolution: unresolved; no resolver link, observed 2026-07-14T15:02:03.459139Z

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Observation b34ba670-a4b7-4961-a8d9-0a1a5b91125c · inbound

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching cites this paper.

Reference 46

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