Paper Citation Record · LEDGER

X-ray emission from magnetized neutron star atmospheres at low mass accretion rates. I. Phase-averaged spectrum

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2104.06802.

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

pith.paper-citation-record.v1
2104.06802 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

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

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T15:20:03.151930Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-13T14:39:39.616184Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

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 d9062d61-22f6-4558-8825-3f611b81737e · inbound

X-Ray Views of Galactic Accreting Pulsars in High-Mass X-Ray Binaries cites this paper.

X-Ray Views of Galactic Accreting Pulsars in High-Mass X-Ray Binaries X-ray emission from magnetized neutron star atmospheres at low mass accretion rates. I. Phase-averaged spectrum

Reference 107

Resolution: unresolved; no resolver link, observed 2026-08-11T05:41:09.093958Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f257ee41-0103-4292-bb1e-37c1460f3845 · inbound

Physics of Strong Magnetism with eXTP cites this paper.

Physics of Strong Magnetism with eXTP X-ray emission from magnetized neutron star atmospheres at low mass accretion rates. I. Phase-averaged spectrum

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-07T05:18:38.533074Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e40f2caf-7aee-4156-85b4-8792d85776fc · inbound

Information content of JWST transmission spectroscopy of the exoplanet HAT-P-12b from the optical to the mid-infrared cites this paper.

Information content of JWST transmission spectroscopy of the exoplanet HAT-P-12b from the optical to the mid-infrared X-ray emission from magnetized neutron star atmospheres at low mass accretion rates. I. Phase-averaged spectrum

Reference 21

Resolution: verified exact; local_arxiv, observed 2026-07-13T14:39:39.617987Z

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.

Observation ceb70be5-c232-427b-a263-1b548c34378f · inbound

Magnetospheric flows in X-ray pulsars II: Heating, cooling and ionization degree at sub-critical accretion cites this paper.

Magnetospheric flows in X-ray pulsars II: Heating, cooling and ionization degree at sub-critical accretion X-ray emission from magnetized neutron star atmospheres at low mass accretion rates. I. Phase-averaged spectrum

Reference 26

Resolution: unresolved; no resolver link, observed 2026-07-14T12:29:39.967082Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fd6b26c4-0733-4660-9c88-456453106a38 · inbound

Real-time observations of the transition to the quiescent state in an accreting magnetised neutron star: No propeller required? cites this paper.

Real-time observations of the transition to the quiescent state in an accreting magnetised neutron star: No propeller required? X-ray emission from magnetized neutron star atmospheres at low mass accretion rates. I. Phase-averaged spectrum

Reference 128

Resolution: unresolved; no resolver link, observed 2026-08-12T18:32:11.220584Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 85b3ca2f-e27f-4cfb-8a3e-401c662048fe · inbound

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs cites this paper.

The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs X-ray emission from magnetized neutron star atmospheres at low mass accretion rates. I. Phase-averaged spectrum

Reference 249

Resolution: unresolved; no resolver link, observed 2026-08-14T15:20:03.151930Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.