Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Neutron star mass and radius measurements from atmospheric model fits to X-ray burst cooling tail spectra
As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:1709.09120.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-16T05:25:17.239051Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-04T07:49:39.067014Z
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 237199d3-7737-48ec-84d6-084aa37245e5 · inbound
GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral cites this paper.
GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral Neutron star mass and radius measurements from atmospheric model fits to X-ray burst cooling tail spectra
Reference 167
- Resolution
- verified exact
- arxiv_id, observed 2026-05-12T01:58:58.894601Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation 1e919a8c-11ea-49f8-ad8a-4ff1609c3e57 · inbound
Gravitational Waves from Holographic Neutron Star Mergers cites this paper.
Gravitational Waves from Holographic Neutron Star Mergers Neutron star mass and radius measurements from atmospheric model fits to X-ray burst cooling tail spectra
Reference 43
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T14:26:03.946262Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1efe7168-12c8-4ca7-af3c-bfdd5681c065 · inbound
Numerical Relativity Simulations of Dark Matter Admixed Binary Neutron Stars cites this paper.
Numerical Relativity Simulations of Dark Matter Admixed Binary Neutron Stars Neutron star mass and radius measurements from atmospheric model fits to X-ray burst cooling tail spectra
Reference 24
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T05:25:17.239051Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3d8e3e44-b83c-4f22-ae45-1fad754a1826 · inbound
Properties of Stable Massive Quark Stars in Holography cites this paper.
Properties of Stable Massive Quark Stars in Holography Neutron star mass and radius measurements from atmospheric model fits to X-ray burst cooling tail spectra
Reference 16
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T03:08:56.890982Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation 2920aa9b-e1ba-48b2-bcd2-1476205c0d41 · inbound
The compact neutron star in 4U 1746-37 revisited: Reassessing the mass and radius cites this paper.
The compact neutron star in 4U 1746-37 revisited: Reassessing the mass and radius Neutron star mass and radius measurements from atmospheric model fits to X-ray burst cooling tail spectra
Reference 114
- Resolution
- verified exact
- local_arxiv, observed 2026-05-15T02:33:31.652352Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation dc6e63c9-e3ce-4123-bae7-096f70956785 · inbound
Pulse profile modelling of the 2024 outburst of the accreting millisecond pulsar SRGA J144459.2-604207 cites this paper.
Pulse profile modelling of the 2024 outburst of the accreting millisecond pulsar SRGA J144459.2-604207 Neutron star mass and radius measurements from atmospheric model fits to X-ray burst cooling tail spectra
Reference 17
- Resolution
- verified exact
- local_arxiv, observed 2026-05-20T08:58:09.366488Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation 55e8c17e-0861-49f4-b4c8-9025ff45bf24 · inbound
Is the coexistence of strange quark stars and hadronic stars favored by astrophysical data? A Bayesian analysis cites this paper.
Is the coexistence of strange quark stars and hadronic stars favored by astrophysical data? A Bayesian analysis Neutron star mass and radius measurements from atmospheric model fits to X-ray burst cooling tail spectra
Reference 144
- Resolution
- verified exact
- local_arxiv, observed 2026-07-04T07:49:39.068426Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation 0c1cc199-9b63-47f1-b5cd-3dd7355dbd4a · 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 Neutron star mass and radius measurements from atmospheric model fits to X-ray burst cooling tail spectra
Reference 85
- Resolution
- unresolved
- no resolver link, observed 2026-07-12T00:24:01.284884Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.