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Paper Citation Record · LEDGER

Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 39 inbound Pith citation observations for arXiv:2203.09562.

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

pith.paper-citation-record.v1
2203.09562 v1

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measured 39 of 39 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-19T06:32:44.657259+00:00

measured 39 of 39 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T12:03:24.697288Z

measured 1 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z

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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 1dad93c6-9c8b-4da8-9d50-dad1d405decb · inbound

Fuzzy Galaxies or Cirrus? Decomposition of Galactic Cirrus in Deep Wide-Field Images cites this paper.

Fuzzy Galaxies or Cirrus? Decomposition of Galactic Cirrus in Deep Wide-Field Images Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM

Reference 51

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Observation 793c5471-1673-4445-83cb-a35eab0b2452 · inbound

Investigations of MWISP Filaments. I. Filament Identification and Analysis Algorithms, and Source Catalogue cites this paper.

Investigations of MWISP Filaments. I. Filament Identification and Analysis Algorithms, and Source Catalogue Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM

Reference 29

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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

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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

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Observation dd726dcc-4b9c-4319-9d18-9d8713042d77 · inbound

Probing the Kinematics of Multiple- and Single-Protostar Systems in Perseus with N2H+ cites this paper.

Probing the Kinematics of Multiple- and Single-Protostar Systems in Perseus with N2H+ Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM

Reference 14

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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

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unresolved
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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

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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

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Observation e575835c-afb4-463f-9605-412d89ce9aeb · inbound

High-resolution APEX/LAsMA $^{12}$CO and $^{13}$CO (3-2) observation of the G333 giant molecular cloud complex : III. Decomposition of molecular clouds into multi-scale hub-filament structures cites this paper.

High-resolution APEX/LAsMA $^{12}$CO and $^{13}$CO (3-2) observation of the G333 giant molecular cloud complex : III. Decomposition of molecular clouds into multi-scale hub-filament structures Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM

Reference 7

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Observation b4f9d1f7-cb15-4e80-8212-ceaef0e1ae7a · inbound

An S-shaped filament formed due to Cloud-Cloud Collision in molecular cloud G178.28-00.61 cites this paper.

An S-shaped filament formed due to Cloud-Cloud Collision in molecular cloud G178.28-00.61 Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM

Reference 28

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Observation 13cb4bfc-03e0-40af-b6f6-df92f5f94430 · inbound

High sensitivity molecular line observations towards the L1544 pre-stellar core challenge current models cites this paper.

High sensitivity molecular line observations towards the L1544 pre-stellar core challenge current models Initial Conditions for Star Formation: A Physical Description of the Filamentary ISM

Reference 24

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unresolved
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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

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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

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arxiv_id, observed 2026-05-17T22:40:23.596622Z

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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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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arxiv_id, observed 2026-05-22T09:36:20.875881Z

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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

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arxiv_id, observed 2026-06-28T09:41:50.712999Z

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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

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arxiv_id, observed 2026-06-28T05:41:41.162046Z

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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

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arxiv_id, observed 2026-06-27T18:11:08.528266Z

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No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

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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

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verified exact
arxiv_id, observed 2026-06-26T14:09:31.143798Z

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No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

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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
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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 2026-08-19T06:32:44.657259+00:00.

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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

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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 2026-08-19T06:32:44.657259+00:00.

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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

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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 2026-08-19T06:32:44.657259+00:00.

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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 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-06-29T04:35:39.162440Z digest=sha256:35b57428615ca482f29c0266f17ae17fd29f32d3d7d443466e2a3fbc89113c8f

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 2026-08-19T06:32:44.657259+00:00.

source=arxiv_source observed=2026-06-26T02:51:59.361331Z digest=sha256:8070124f1eebaa648358f2d301345f774d7f853674fd7833e07f5280d73b965a

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 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-06-26T03:40:21.115655Z digest=sha256:4433fbbeba08aa838d02377f81534c77e48ce9c7f4bd963a36e6ae75f5649300

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 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-07-02T08:49:14.813286Z digest=sha256:f5ec09d4fa70c2a3ee0cee4086a343b2368a86a387e52aa1fa8c602afd4f7083

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.

source=arxiv_source observed=2026-07-11T13:23:11.503279Z digest=sha256:1dfb67645d02749a9b7387e3dbd958cefe6cd40b070359892ddafa22f2162a7c

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.

source=arxiv_source observed=2026-07-11T07:55:39.166465Z digest=sha256:58b83da12bc2a0670b7c580375a7a2314d0343f73a41b68c1efa409371f76f30

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.

source=arxiv_source observed=2026-07-31T15:39:28.691792Z digest=sha256:e385f0dd8207e4a12c2e7fc4e983e965d0b13050b545360ef678bf98586242d2

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.

source=arxiv_source observed=2026-08-04T11:34:11.863799Z digest=sha256:d5758b4fe5382b03d868a7449db1ceee76efd12aface7d4770f0ca8ff97692bb