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Paper Citation Record · LEDGER

What is the hard spectral state in X-ray binaries? Insights from GRRMHD accretion flows simulations and polarization of their X-ray emission

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2309.09087.

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

pith.paper-citation-record.v1
2309.09087 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T19:33:25.101812Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-19T22:37:49.776667Z

Reference resolution

0 of 0 outbound references displayed

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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 2508c2b2-5c1f-48f4-aafe-b3a7b98fd7db · inbound

Bulk Motions in the Black Hole Jet Sheath as a Candidate for the Comptonizing Corona cites this paper.

Bulk Motions in the Black Hole Jet Sheath as a Candidate for the Comptonizing Corona What is the hard spectral state in X-ray binaries? Insights from GRRMHD accretion flows simulations and polarization of their X-ray emission

Reference 72

Resolution
unresolved
no resolver link, observed 2026-08-12T19:33:25.101812Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T19:33:25.101812Z digest=sha256:ce40424e21f8c68bb1aaf274cad21c28c3caeac581e5d3fee41c8a48792d3819

Observation 73b3d2b5-7b32-4cc2-9faf-96f1110e1bb6 · inbound

Polarization Signatures from GRMHD Simulations of Black Hole Accretion cites this paper.

Polarization Signatures from GRMHD Simulations of Black Hole Accretion What is the hard spectral state in X-ray binaries? Insights from GRRMHD accretion flows simulations and polarization of their X-ray emission

Reference 62

Resolution
verified exact
arxiv_id, observed 2026-05-15T03:08:59.004254Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

source=pdf_text observed=2026-05-15T03:06:24.087052Z digest=sha256:d4363d50de9484cca2d5a24478382154040b036f1ddeba8cd81f5dc68a512851

Observation 7e729a77-b82f-47de-9c6d-2acf270efc8e · inbound

GRMHD Simulations of Magnetized Accretion Disk/Jet: Variabilities of Black Holes and Spectral Energy Distributions in Magnetic States cites this paper.

GRMHD Simulations of Magnetized Accretion Disk/Jet: Variabilities of Black Holes and Spectral Energy Distributions in Magnetic States What is the hard spectral state in X-ray binaries? Insights from GRRMHD accretion flows simulations and polarization of their X-ray emission

Reference 57

Resolution
verified exact
arxiv_id, observed 2026-05-19T22:37:49.778671Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

source=pdf_text observed=2026-05-19T22:37:39.928169Z digest=sha256:02207812910c9b4dd59ce27bc22f38b24ecb96c2a4308870b465daf29081cd01