Paper Citation Record · LEDGER

From filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey

As of 17 July 2026, this Paper Citation Record lists 0 of 0 outbound references and 15 inbound Pith citation observations for arXiv:1005.2618.

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pith.paper-citation-record.v1
1005.2618 v2

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measured 15 of 15 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-07-17T06:31:00.352745+00:00

measured 15 of 15 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-14T15:02:03.459139Z

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

Source: pith, observed 2026-07-10T11:37:02.967207Z

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Outbound references

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Pith citing papers

Observation 3181e8c5-bf03-43bd-bd0c-766a339ad97b · 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 From filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey

Reference 33

Resolution: verified exact; local_arxiv, observed 2026-05-21T03:59:32.322657Z

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Observation 7fdd460c-944e-4fb1-afe0-9549e27feda0 · 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 From filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey

Reference 22

Resolution: verified exact; local_arxiv, observed 2026-05-21T03:29:29.018445Z

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Observation 3761b21b-62a4-4672-97e4-90eacec6e220 · 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 From filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey

Reference 4

Resolution: verified exact; local_arxiv, observed 2026-06-28T05:41:40.958228Z

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Observation 308dccb1-42f4-4582-878c-3ad032e7841d · inbound

Grain Alignment and Dust Evolution Physics with Polarisation (GRADE-POL). II. On the physical basis of Serkowski and super-Serkowski polarisation spectra cites this paper.

Grain Alignment and Dust Evolution Physics with Polarisation (GRADE-POL). II. On the physical basis of Serkowski and super-Serkowski polarisation spectra From filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey

Reference 49

Resolution: verified exact; local_arxiv, observed 2026-06-27T06:50:39.932157Z

Source-reported events for the cited work

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Observation 67e676e3-271f-4d16-b7ff-120cc6139556 · inbound

A HINSA view of cosmic-ray ionization in IC 348 and NGC 1333: evidence for a strong low-energy cosmic-ray disparity cites this paper.

A HINSA view of cosmic-ray ionization in IC 348 and NGC 1333: evidence for a strong low-energy cosmic-ray disparity From filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey

Reference 141

Resolution: verified exact; local_arxiv, observed 2026-06-27T03:50:28.348084Z

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Observation c03a397a-c226-44a0-9513-1374f5a23bba · inbound

PMO Polaris CO survey. II. Where is the dust? cites this paper.

PMO Polaris CO survey. II. Where is the dust? From filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey

Reference 68

Resolution: verified exact; local_arxiv, observed 2026-06-26T17:19:35.805876Z

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Observation 8d1e6e44-051a-4e8b-90ee-ab7b438fc6d9 · 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 From filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey

Reference 42

Resolution: verified exact; local_arxiv, observed 2026-06-27T01:20:20.617253Z

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Observation 0343dfd4-4ebb-4343-9ba1-8c438c09d3c2 · inbound

Formation of a Protostellar Multiple System via Rotational Fragmentation cites this paper.

Formation of a Protostellar Multiple System via Rotational Fragmentation From filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey

Reference 22

Resolution: verified exact; local_arxiv, observed 2026-06-25T20:58:21.401273Z

Source-reported events for the cited work

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Observation 5ef939fc-9d0d-48a6-8e79-37daec4a60d0 · inbound

Kolmogorov turbulence across multi-fractal gas in Polaris Flare cites this paper.

Kolmogorov turbulence across multi-fractal gas in Polaris Flare From filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey

Reference 18

Resolution: verified exact; local_arxiv, observed 2026-07-02T09:06:48.291827Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-17T06:31:00.352745+00:00.

Observation 02e41e26-a850-43be-813d-87fb82fab019 · inbound

Tracing grain growth in the forming prestellar core L1506C with 3D modeling of Herschel, IRAM, and CFHT observations cites this paper.

Tracing grain growth in the forming prestellar core L1506C with 3D modeling of Herschel, IRAM, and CFHT observations From filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey

Reference 21

Resolution: verified exact; local_arxiv, observed 2026-07-03T09:27:47.948348Z

Source-reported events for the cited work

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Observation b147b128-dbc1-484f-a67b-16995855be3b · 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 From filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey

Reference 46

Resolution: unresolved; no resolver link, observed 2026-07-11T13:23:11.503279Z

Source-reported events for the cited work

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Observation a9c2f07b-83fd-41ba-809e-ea25ad8f293d · 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 From filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey

Reference 5

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 ea2b6727-0723-431f-9169-acc1b7d5a12f · inbound

Chemical diversity of dense cores in Orion B: The role of the environment cites this paper.

Chemical diversity of dense cores in Orion B: The role of the environment From filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey

Reference 7

Resolution: verified exact; local_arxiv, observed 2026-07-09T09:26:08.530602Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-17T06:31:00.352745+00:00.

Observation 13c35a88-ebda-49e9-ba57-a5b83fe6346c · inbound

CARPP: Parametric Radiative-Transfer Fitting of Molecular Cores from Dust Continuum Data cites this paper.

CARPP: Parametric Radiative-Transfer Fitting of Molecular Cores from Dust Continuum Data From filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey

Reference 26

Resolution: verified exact; local_arxiv, observed 2026-07-10T11:37:02.970084Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-17T06:31:00.352745+00:00.

Observation c9f5f3c6-91d3-478d-b012-ec4ea533c866 · 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 From filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey

Reference 12

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.