Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 33 inbound Pith citation observations for arXiv:2203.09562.
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 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-11T05:19:24.566435Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
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- unresolved0
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External citation measurements
39
arxiv_reference, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 407177bf-8060-4a20-ad82-c65a732d0fed · inbound
A Tale of Three: Magnetic Fields along the Orion Integral-Shaped Filament as Revealed by JCMT BISTRO survey cites this paper.
A Tale of Three: Magnetic Fields along the Orion Integral-Shaped Filament as Revealed by JCMT BISTRO survey Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM
Reference 23
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T05:19:24.566435Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 00c24179-c422-4f8a-a4c5-db4b53dd5e9c · inbound
3D MC I: X-ray Tomography Begins to Unravel the 3-D Structure of a Molecular Cloud in our Galaxy's Center cites this paper.
3D MC I: X-ray Tomography Begins to Unravel the 3-D Structure of a Molecular Cloud in our Galaxy's Center Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM
Reference 21
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T20:42:45.977225Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ce2066b9-35bc-4b11-81bf-e5261b7c3a50 · inbound
Dense gas tracers in and between spiral arms: from Giant Molecular Filaments to star-forming clumps cites this paper.
Dense gas tracers in and between spiral arms: from Giant Molecular Filaments to star-forming clumps Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM
Reference 18
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T12:35:33.295695Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8d3346e5-d270-49ba-a6c2-af8ddfaa2fde · inbound
The Karl G. Jansky Very Large Array Local Group L-band Survey (LGLBS) cites this paper.
The Karl G. Jansky Very Large Array Local Group L-band Survey (LGLBS) Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM
Reference 64
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T04:09:23.505962Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation fe20cdbc-f53b-483f-a4fe-e520090d251d · inbound
Protostellar disks in their natural habitat -- the formation of protostars and their accretion disks in the turbulent and magnetized interstellar medium cites this paper.
Protostellar disks in their natural habitat -- the formation of protostars and their accretion disks in the turbulent and magnetized interstellar medium Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM
Reference 32
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T00:24:49.181587Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5e2703d1-4126-45d2-8053-9dde93da3d1f · inbound
ALMA-IMF. XXI.: N$_2$H$^+$ kinematics in the G012.80 protocluster: Evidence for filament rotation and evolution cites this paper.
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 cedbbc0a-f8d5-4276-860d-a9759f507b13 · inbound
Revealing the Connection Between the Filamentary Hierarchy and Star Cluster Formation in a Simulated NGC 628 Galaxy cites this paper.
Revealing the Connection Between the Filamentary Hierarchy and Star Cluster Formation in a Simulated NGC 628 Galaxy Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM
Reference 12
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-05-17T22:40:23.596622Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation a57ee145-67b5-4f43-8825-6e022419cf45 · inbound
ALMA Central molecular zone Exploration Survey (ACES) VI: ALMA Large Program Reveals a Highly Filamentary Central Molecular Zone cites this paper.
ALMA Central molecular zone Exploration Survey (ACES) VI: ALMA Large Program Reveals a Highly Filamentary Central Molecular Zone Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM
Reference 2
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T21:26:56.896967Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a8d462a1-5b06-495a-b378-a386ff2e2f33 · inbound
The fragmentation properties of massive star-forming regions in 30Dor-10 at 2000 au resolution cites this paper.
The fragmentation properties of massive star-forming regions in 30Dor-10 at 2000 au resolution Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM
Reference 66
- Resolution
- verified exact
- arxiv_id, observed 2026-05-11T13:21:19.869391Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation bdd4db4b-de20-445b-823a-44948d2559db · inbound
Scale-Aware Adversarial Analysis: A Diagnostic for Generative AI in Multiscale Complex Systems cites this paper.
Scale-Aware Adversarial Analysis: A Diagnostic for Generative AI in Multiscale Complex Systems Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM
Reference 24
- Resolution
- verified exact
- arxiv_id, observed 2026-05-09T19:56:16.549878Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation c5237c22-3d1e-411c-82a1-311ed53c6faa · inbound
The slope of the power spectrum of the density field in isothermal supersonic compressible turbulence cites this paper.
The slope of the power spectrum of the density field in isothermal supersonic compressible turbulence Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM
Reference 73
- Resolution
- verified exact
- arxiv_id, observed 2026-05-12T00:31:19.230952Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 88832007-dc2a-4ea4-9336-0fd26c02f84b · inbound
The slope of the power spectrum of the density field in isothermal supersonic compressible turbulence cites this paper.
The slope of the power spectrum of the density field in isothermal supersonic compressible turbulence Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM
Reference 73
- Resolution
- verified exact
- arxiv_id, observed 2026-05-09T06:25:48.361711Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation c1405d7a-3209-444f-9e0d-72330ca437c1 · inbound
Simulating Star Formation and Star Cluster Assembly in the Aquila Rift Using Archival Observations cites this paper.
Simulating Star Formation and Star Cluster Assembly in the Aquila Rift Using Archival Observations Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM
Reference 92
- Resolution
- verified exact
- arxiv_id, observed 2026-05-12T04:06:21.388027Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation fee08d22-6d4b-462e-a701-8a3a89320c6f · inbound
SIMPLIFI -- Study of Interstellar Magnetic Polarization: a Legacy Investigation of Filaments. I. Magnetically-Guided Accretion onto the DR21 Ridge cites this paper.
SIMPLIFI -- Study of Interstellar Magnetic Polarization: a Legacy Investigation of Filaments. I. Magnetically-Guided Accretion onto the DR21 Ridge Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM
Reference 35
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-05-14T20:27:58.124118Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation ea2d211e-89e7-41b7-ab13-5b685a0096a2 · inbound
The ${}^{13}\mathrm{CO}(2{-}1)/^{12}\mathrm{CO}(2{-}1)$ Line Ratio from 100 Molecular Clouds in the Large Magellanic Cloud cites this paper.
The ${}^{13}\mathrm{CO}(2{-}1)/^{12}\mathrm{CO}(2{-}1)$ Line Ratio from 100 Molecular Clouds in the Large Magellanic Cloud Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM
Reference 170
- Resolution
- verified exact
- arxiv_id, observed 2026-05-19T20:17:45.046281Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 0adb23a8-4c1b-4ff6-b8c5-7dd1c07807ab · inbound
Evolution of compressed clouds formed by filament coalescence. I. Oblique collisions cites this paper.
Evolution of compressed clouds formed by filament coalescence. I. Oblique collisions Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM
Reference 164
- Resolution
- verified exact
- arxiv_id, observed 2026-05-21T03:59:32.167103Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 6c6eea55-c521-413c-bdb5-c279e8848808 · inbound
Interstellar Medium-Driven Orbital Transport -- I. Radial Heating and Migration cites this paper.
Interstellar Medium-Driven Orbital Transport -- I. Radial Heating and Migration Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM
Reference 67
- Resolution
- verified exact
- arxiv_id, observed 2026-05-22T09:36:20.875881Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 1b933c6e-f695-4296-b7f2-f1a9af041d5c · inbound
A nine-member protostellar system forming via filament fragmentation in the high mass protocluster NGC 6334-43 cites this paper.
A nine-member protostellar system forming via filament fragmentation in the high mass protocluster NGC 6334-43 Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM
Reference 119
- Resolution
- verified exact
- arxiv_id, observed 2026-06-28T09:41:50.712999Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 744292da-894a-455b-b8c8-ca0eb6e2bc62 · inbound
Statistical analysis of the relative orientations between filaments and magnetic fields using Herschel and Planck data in star-forming regions cites this paper.
Statistical analysis of the relative orientations between filaments and magnetic fields using Herschel and Planck data in star-forming regions Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM
Reference 31
- Resolution
- verified exact
- arxiv_id, observed 2026-06-28T05:41:41.162046Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 3e0c5d14-b5cc-41e6-9188-d01e17f2613b · inbound
From filaments to clumps: filament properties with synthetic Herschel observations cites this paper.
From filaments to clumps: filament properties with synthetic Herschel observations Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM
Reference 25
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-06-27T18:11:08.528266Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation af995a1d-acda-4d80-a654-2d28fc46eaaa · inbound
Star Formation at the Periphery of a Molecular Superbubble: The Case of G12.79+0.43 cites this paper.
Star Formation at the Periphery of a Molecular Superbubble: The Case of G12.79+0.43 Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM
Reference 105
- Resolution
- verified exact
- arxiv_id, observed 2026-06-26T14:09:31.143798Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 28d5fdda-12cd-4db1-8ec0-a9e073fd2e7f · inbound
Highly filamentary H{\,\small I} gas in the circumgalactic medium and intragalactic medium around NGC 4631 cites this paper.
Highly filamentary H{\,\small I} gas in the circumgalactic medium and intragalactic medium around NGC 4631 Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM
Reference 7
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-06-26T08:39:14.865373Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 575ff8bb-ed38-4a02-97b2-8b6d897dc92e · inbound
Early phases of star formation with SKAO: synchrotron emission from dense starless cores in molecular clouds cites this paper.
Early phases of star formation with SKAO: synchrotron emission from dense starless cores in molecular clouds Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM
Reference 35
- Resolution
- verified exact
- arxiv_id, observed 2026-06-27T01:20:20.680940Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 7774ea62-0624-4955-9efe-ab01fb7a13a9 · inbound
Spectroscopic surveys with the SKA probing the ionized and molecular Milky Way cites this paper.
Spectroscopic surveys with the SKA probing the ionized and molecular Milky Way Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM
Reference 69
- Resolution
- verified exact
- arxiv_id, observed 2026-06-27T04:10:32.574374Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation ca5687d1-788e-43b8-bf2e-2775ee14e84a · inbound
The 10-15 GHz radio continuum survey of the Galactic Plane with SKAO cites this paper.
The 10-15 GHz radio continuum survey of the Galactic Plane with SKAO Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM
Reference 63
- Resolution
- verified exact
- arxiv_id, observed 2026-06-26T02:38:56.460347Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 0f0c17af-b4a5-43f3-bff1-5696ccd8e6d1 · inbound
The 10-15 GHz radio continuum survey of the Galactic Plane with SKAO cites this paper.
The 10-15 GHz radio continuum survey of the Galactic Plane with SKAO Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM
Reference 63
- Resolution
- verified exact
- arxiv_id, observed 2026-06-29T04:43:06.553953Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 44c6591c-5b40-48e9-87b1-edcaa1846595 · inbound
Astrochemical Study of Early Embedded Disks cites this paper.
Astrochemical Study of Early Embedded Disks Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM
Reference 90
- Resolution
- verified exact
- arxiv_id, observed 2026-06-26T02:58:56.470624Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation f4cf2613-7f02-4f50-8274-53600725c1d6 · inbound
3D Magnetic Field Vectors in Space: Bubbles, Clouds, and Filaments cites this paper.
3D Magnetic Field Vectors in Space: Bubbles, Clouds, and Filaments Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM
Reference 34
- Resolution
- verified exact
- arxiv_id, observed 2026-06-26T06:29:04.527710Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation f1b5d9ae-2d93-4555-b7a8-667c56cc002f · inbound
The Milky Way Atlas for Linear Filaments III: Giant filaments and magnetic fields as evidence of a bubbly Galactic disk cites this paper.
The Milky Way Atlas for Linear Filaments III: Giant filaments and magnetic fields as evidence of a bubbly Galactic disk Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM
Reference 27
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-07-02T08:56:49.161170Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 88ba3b1d-5b90-403b-91c0-1e3cdeed7fa9 · inbound
Sutra : An integrated framework for identification and characterization of filaments in the interstellar medium cites this paper.
Sutra : An integrated framework for identification and characterization of filaments in the interstellar medium Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM
Reference 64
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T13:23:11.503279Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d501f3d3-23af-46bb-987c-bb2638d80ba7 · inbound
Emergence of high-mass stars in complex fiber networks (EMERGE) VI. Turbulence dissipation and the formation of dense fibers cites this paper.
Emergence of high-mass stars in complex fiber networks (EMERGE) VI. Turbulence dissipation and the formation of dense fibers Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM
Reference 61
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T07:55:39.166465Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6a36198d-bbaa-4db9-bf11-1dacf848481b · inbound
Bipolar HII regions Produced by Cloud-Cloud Collisions cites this paper.
Bipolar HII regions Produced by Cloud-Cloud Collisions Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM
Reference 45
- Resolution
- unresolved
- no resolver link, observed 2026-07-31T15:39:28.691792Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a7a3a2cf-476e-4055-9b07-b355e943ba39 · inbound
Accretion across scales: streamers, surface-layer transport, and rapid replenishment in young protoplanetary discs cites this paper.
Accretion across scales: streamers, surface-layer transport, and rapid replenishment in young protoplanetary discs Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM
Reference 163
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T11:34:11.863799Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.