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Paper Citation Record · LEDGER

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

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 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 6 of 6 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 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T19:11:16.313477Z

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

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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 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.

source=arxiv_source observed=2026-08-10T16:29:20.797628Z digest=sha256:c12a8136545e30cb3e7e546abab7d394e8ba2ebaa6c44b3107aaf1a154163f43

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 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-06-27T09:15:19.155163Z digest=sha256:ab54911de8878837844ca7c197e8ee841126aed356173518ec2f3b71326f9480

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.

source=arxiv_source observed=2026-08-02T11:54:24.509923Z digest=sha256:d964b27144b8649af5160c6765bc3e735a8f0dc896bf61fc809542c61c8e5c2c

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.

source=arxiv_source observed=2026-07-12T00:24:01.284884Z digest=sha256:861f91a897699a58f95ea98a3f3672da38ad115f6832856482abd7ffa0714186

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.

source=arxiv_source observed=2026-08-07T20:40:57.664265Z digest=sha256:68cb3e4bd3de14a3eca76d5171992d7d8071d1cac6b0338b9e62b93de1d61c05

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.

source=arxiv_source observed=2026-08-11T19:11:16.313477Z digest=sha256:66ae9ab4dcb257bd49b59321f786549b37f693754a20b72983027fd7444dad9b