Paper Citation Record · LEDGER

An Empirical Background Model for the NICER X-ray Timing Instrument

As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2105.09901.

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

pith.paper-citation-record.v1
2105.09901 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-21T06:32:19.484+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T00:31:23.601127Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T11:58:06.143481Z

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 38ac6a00-6aa8-411e-a42a-1f2e263eab9d · inbound

Spectro-temporal Investigation of Quasi-periodic Oscillations From Black Hole X-ray Binary 4U 1630-472 Using $\textit{NICER}$ cites this paper.

Spectro-temporal Investigation of Quasi-periodic Oscillations From Black Hole X-ray Binary 4U 1630-472 Using $\textit{NICER}$ An Empirical Background Model for the NICER X-ray Timing Instrument

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-10T16:29:20.797628Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d674a2e2-aa79-48b8-a296-23e75266a340 · inbound

Long thermonuclear burst driven thermal-viscous instability of accretion disk: triggering an outburst-like X-ray flare cites this paper.

Long thermonuclear burst driven thermal-viscous instability of accretion disk: triggering an outburst-like X-ray flare An Empirical Background Model for the NICER X-ray Timing Instrument

Reference 50

Resolution: verified exact; arxiv_id, observed 2026-07-03T11:58:06.144863Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation b34d7c1e-27ae-4b84-8033-e2a1492e6c24 · inbound

Long thermonuclear burst driven thermal-viscous instability of accretion disk: triggering an outburst-like X-ray flare cites this paper.

Long thermonuclear burst driven thermal-viscous instability of accretion disk: triggering an outburst-like X-ray flare An Empirical Background Model for the NICER X-ray Timing Instrument

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-02T11:54:24.509923Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f28ac7f9-1749-482e-844b-ecf185ade6c1 · inbound

A NICER view of the millisecond pulsar PSR J2124$-$3358: evidence for a helium atmosphere cites this paper.

A NICER view of the millisecond pulsar PSR J2124$-$3358: evidence for a helium atmosphere An Empirical Background Model for the NICER X-ray Timing Instrument

Reference 99

Resolution: unresolved; no resolver link, observed 2026-07-12T00:24:01.284884Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cb0387b3-fd7a-43ff-bf9c-6b1bae970c88 · inbound

Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry cites this paper.

Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry An Empirical Background Model for the NICER X-ray Timing Instrument

Reference 224

Resolution: unresolved; no resolver link, observed 2026-08-07T20:40:57.664265Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ebdfdce4-330f-495e-84b6-6bdb652dc31e · inbound

Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry cites this paper.

Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry An Empirical Background Model for the NICER X-ray Timing Instrument

Reference 224

Resolution: unresolved; no resolver link, observed 2026-08-15T14:41:14.121957Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 14f33755-9572-49dd-8956-439daa2fd454 · inbound

Rapid Orbital Decay in the Ultracompact Double-degenerate Binary eRASSU J060839.5$-$704014 cites this paper.

Rapid Orbital Decay in the Ultracompact Double-degenerate Binary eRASSU J060839.5$-$704014 An Empirical Background Model for the NICER X-ray Timing Instrument

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-11T19:11:16.313477Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9e76c264-c08f-4413-8ebf-19c0fcf5eaa9 · inbound

Radio flares and X-ray hardening embedded in the long soft state of 4U 1543-475 cites this paper.

Radio flares and X-ray hardening embedded in the long soft state of 4U 1543-475 An Empirical Background Model for the NICER X-ray Timing Instrument

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-16T00:31:23.601127Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.