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Paper Citation Record · LEDGER

Modeling the Multi-Wavelength Emission of Shell-Type Supernova Remnant RX J1713.7-3946

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1011.0145.

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

pith.paper-citation-record.v1
1011.0145 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T02:23:17.885949Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-03T12:48:11.884396Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • malformed identifier0
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External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 73089c4a-3e4a-4eed-aa6b-10fb6d483561 · inbound

On The Nonthermal Power Laws In Magnetized Turbulent Plasmas cites this paper.

On The Nonthermal Power Laws In Magnetized Turbulent Plasmas Modeling the Multi-Wavelength Emission of Shell-Type Supernova Remnant RX J1713.7-3946

Reference 260

Resolution
verified exact
arxiv_id, observed 2026-05-11T22:21:41.876547Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-05-08T02:56:31.205859Z digest=sha256:e8ec57b95260d4eb8da32d5f4e557fe8050677b3aca001eb312e235d9e9db247

Observation 85633ea4-ed45-413b-a582-a02fa144ca65 · inbound

SN 1006: A Cosmic Laboratory for Investigating Shock Acceleration Physics cites this paper.

SN 1006: A Cosmic Laboratory for Investigating Shock Acceleration Physics Modeling the Multi-Wavelength Emission of Shell-Type Supernova Remnant RX J1713.7-3946

Reference 275

Resolution
verified exact
local_arxiv, observed 2026-07-03T12:48:11.885592Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-06-27T08:44:08.685220Z digest=sha256:6d6eac9b5892c22dbbbbbc17e2de01cb609325fde0d0a8fd98658f043fc00933

Observation c2254487-22c0-491a-91f3-88a482e92f6a · inbound

Hybrid Simulations of Proton Acceleration at Oblique High-$\beta$ Shocks cites this paper.

Hybrid Simulations of Proton Acceleration at Oblique High-$\beta$ Shocks Modeling the Multi-Wavelength Emission of Shell-Type Supernova Remnant RX J1713.7-3946

Reference 278

Resolution
unresolved
no resolver link, observed 2026-07-13T06:22:12.013309Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-13T06:22:12.013309Z digest=sha256:bb42fdac98b04f1e04adb939174570bc8b1110843c31a8d6ed4b2cea978f40c3

Observation 924bf66a-549a-46c3-84a0-0807833dea05 · inbound

Multiwavelength study of non-thermal emission in the Swift J1834.9-0846/W41 region cites this paper.

Multiwavelength study of non-thermal emission in the Swift J1834.9-0846/W41 region Modeling the Multi-Wavelength Emission of Shell-Type Supernova Remnant RX J1713.7-3946

Reference 66

Resolution
unresolved
no resolver link, observed 2026-08-02T02:23:17.885949Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T02:23:17.885949Z digest=sha256:1201da76f94998b9109c1c9be0efe25c8a7df2a3baacd13d7fa2b080eec4f30c

Observation 79c250ab-2f2f-4d13-b2e0-72b008218bef · inbound

Non-thermal emission from the vicinity of the magnetar CXOU J171405.7-381031 cites this paper.

Non-thermal emission from the vicinity of the magnetar CXOU J171405.7-381031 Modeling the Multi-Wavelength Emission of Shell-Type Supernova Remnant RX J1713.7-3946

Reference 59

Resolution
unresolved
no resolver link, observed 2026-08-01T21:55:38.298760Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T21:55:38.298760Z digest=sha256:abbb675ab1613b6ea3e032de19df0b07b68f3ad8b74fdd0528cb296dba2f1e09