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Paper Citation Record · LEDGER

Planck intermediate results. XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds

As of 4 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 14 inbound Pith citation observations for arXiv:1502.04123.

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pith.paper-citation-record.v1
1502.04123 v4

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Source: paper_references, paper_reference_links

measured 14 of 14 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-04T06:34:03.388597+00:00

measured 14 of 14 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T10:56:39.701691Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-30T05:14:18.347864Z

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Outbound references

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Pith citing papers

Observation 8952b6cf-c23a-451d-931a-11f3e14277f1 · 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 Planck intermediate results. XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds

Reference 187

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local_arxiv, observed 2026-05-19T20:17:44.918635Z

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Observation fe4fb0d6-3a2c-42e1-8550-20b51fb5773e · 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 Planck intermediate results. XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds

Reference 31

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local_arxiv, observed 2026-05-21T03:59:31.873700Z

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Observation 3b52b9b7-e23e-476b-a3d2-1bf53da4d894 · inbound

B-Fields and Star Formation across Scales with TRAO (B-FROST): CO Abundances, Dynamics and Relative Orientations in the Translucent High Latitude Cloud MBM12 cites this paper.

B-Fields and Star Formation across Scales with TRAO (B-FROST): CO Abundances, Dynamics and Relative Orientations in the Translucent High Latitude Cloud MBM12 Planck intermediate results. XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds

Reference 35

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Observation 5b0f0acd-6702-4ef8-bbe8-3e7d1b4192a7 · inbound

Numerical simulations of shock-driven, supersonic turbulence in colliding three-temperature laboratory plasmas cites this paper.

Numerical simulations of shock-driven, supersonic turbulence in colliding three-temperature laboratory plasmas Planck intermediate results. XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds

Reference 268

Resolution
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local_arxiv, observed 2026-05-22T08:11:15.976282Z

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Observation 6aa05da5-e32b-4eed-a0eb-1506109f989b · inbound

The magnetic field of the Milky Way: an observational perspective cites this paper.

The magnetic field of the Milky Way: an observational perspective Planck intermediate results. XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds

Reference 295

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local_arxiv, observed 2026-06-28T14:02:16.493922Z

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Observation 77f3c08c-dfd0-475c-8585-35b426115a8f · 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 Planck intermediate results. XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds

Reference 81

Resolution
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local_arxiv, observed 2026-06-28T05:41:41.003000Z

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No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

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Observation bd56c492-50bb-4297-826b-869cd8f4b1bc · inbound

Measuring Magnetic Field Strengths in Galactic Star-forming Regions via the Zeeman Effect with the SKA cites this paper.

Measuring Magnetic Field Strengths in Galactic Star-forming Regions via the Zeeman Effect with the SKA Planck intermediate results. XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds

Reference 131

Resolution
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Observation 9f15a4d5-f756-45b2-b10f-01ead40098d4 · inbound

Characterising magnetic fields at the onset of star cluster formation: From giant molecular clouds to infrared dark clumps cites this paper.

Characterising magnetic fields at the onset of star cluster formation: From giant molecular clouds to infrared dark clumps Planck intermediate results. XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds

Reference 58

Resolution
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Observation 39ad4911-a86e-48c5-82f9-7c29f4bd9e5f · inbound

Small-scale Magnetic Fields in the Milky Way and Nearby Galaxies cites this paper.

Small-scale Magnetic Fields in the Milky Way and Nearby Galaxies Planck intermediate results. XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds

Reference 146

Resolution
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local_arxiv, observed 2026-06-26T00:48:45.515283Z

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Observation f4755f75-c914-4cd6-80d3-5032cc88187f · 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 Planck intermediate results. XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds

Reference 33

Resolution
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local_arxiv, observed 2026-06-27T01:20:20.605500Z

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Observation d265ae24-5509-4122-9d1c-7df9d410f72d · inbound

Detectors for CLASS-W2: The second 90 GHz telescope of the Cosmology Large Angular Scale Surveyor cites this paper.

Detectors for CLASS-W2: The second 90 GHz telescope of the Cosmology Large Angular Scale Surveyor Planck intermediate results. XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds

Reference 261

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local_arxiv, observed 2026-06-26T04:28:59.172334Z

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Observation 8766d022-dc25-4c4a-b4dd-258a9ef4a237 · inbound

Projection Is All You Need: Interpreting Polarization Measurements in the Orion Clouds with Sub-Alfv\'enic MHD Simulations cites this paper.

Projection Is All You Need: Interpreting Polarization Measurements in the Orion Clouds with Sub-Alfv\'enic MHD Simulations Planck intermediate results. XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds

Reference 22

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Observation baac3d50-c0e8-4b7b-958c-fa43a47e9bb9 · inbound

ALMA observations of Magnetic Fields in the Massive Star-forming Region IRAS 18360-0537 cites this paper.

ALMA observations of Magnetic Fields in the Massive Star-forming Region IRAS 18360-0537 Planck intermediate results. XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds

Reference 126

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Observation 2b6c6747-783c-4f6b-8619-388742312c91 · inbound

Galactic Science with the LiteBIRD satellite: Spectral characterization of diffuse Galactic polarized emission at the angular power spectrum level cites this paper.

Galactic Science with the LiteBIRD satellite: Spectral characterization of diffuse Galactic polarized emission at the angular power spectrum level Planck intermediate results. XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds

Reference 43

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