Pith. sign in

Paper Citation Record · LEDGER

An Ultraluminous X-ray Source Powered by An Accreting Neutron Star

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 12 inbound Pith citation observations for arXiv:1410.3590.

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

pith.paper-citation-record.v1
1410.3590 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 12 of 12 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-05T06:32:48.257954+00:00

measured 12 of 12 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T18:26:34.955548Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T13:17:05.364651Z

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 2f43ce89-a75c-42f2-8b8c-6ce19cb9eb6a · inbound

High Power Accretion in Massive Binary Systems and the Impact of Metallicity cites this paper.

High Power Accretion in Massive Binary Systems and the Impact of Metallicity An Ultraluminous X-ray Source Powered by An Accreting Neutron Star

Reference 1

Resolution
unresolved
no resolver link, observed 2026-08-04T18:26:34.955548Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T18:26:34.955548Z digest=sha256:214a8593148f5493d9377e3c81525cfe914825d9756f7ca4b90effd73054b19a

Observation 96eabebc-d218-4fd5-aa91-5528fee143a8 · inbound

Revisiting the Reported Period of FRB 20201124A Using MCMC Methods cites this paper.

Revisiting the Reported Period of FRB 20201124A Using MCMC Methods An Ultraluminous X-ray Source Powered by An Accreting Neutron Star

Reference 26

Resolution
malformed identifier
local_arxiv, observed 2026-05-16T19:41:12.333550Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=pdf_text observed=2026-05-16T19:39:51.068922Z digest=sha256:cd67bac751d46c7981c79ec9f0f29937b93edfbaab1904a0a8dcc766eb20d2c8

Observation 304af550-351a-4228-af93-823d1b40db1e · 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 An Ultraluminous X-ray Source Powered by An Accreting Neutron Star

Reference 3

Resolution
unresolved
no resolver link, observed 2026-07-13T14:30:13.573690Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-13T14:30:13.573690Z digest=sha256:2c1a66ee634b09db5edd5af17df0fb5c1d47a33468e5012ceb827a748769317e

Observation f98b5801-5b1a-48fc-b94e-ce233769892f · inbound

Significant or Not? The Impact of Randomisation During Data Reduction on Confirming a New Pulsating Ultraluminous X-ray Source Candidate in Centaurus A cites this paper.

Significant or Not? The Impact of Randomisation During Data Reduction on Confirming a New Pulsating Ultraluminous X-ray Source Candidate in Centaurus A An Ultraluminous X-ray Source Powered by An Accreting Neutron Star

Reference 84

Resolution
verified exact
local_arxiv, observed 2026-05-15T03:09:41.997794Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:691ce949f5477bdf6e68274f7e3561338b63ca896d57994fcc1967b3ad3e6ad1

Observation 536d590a-d156-4e27-9e94-fcfa58d0b240 · inbound

Searching for links between energetic millisecond pulsars and repeating fast radio bursts cites this paper.

Searching for links between energetic millisecond pulsars and repeating fast radio bursts An Ultraluminous X-ray Source Powered by An Accreting Neutron Star

Reference 25

Resolution
verified exact
local_arxiv, observed 2026-05-21T03:34:28.195289Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:b8b4d6e3ce07410213f00133b7c96aca23e7fbef8e02bc43eee8c78304f87665

Observation 0a2de73e-5e0d-41ac-a351-43dc2e3c1be4 · inbound

The role of major mergers in triggering super-Eddington accretion cites this paper.

The role of major mergers in triggering super-Eddington accretion An Ultraluminous X-ray Source Powered by An Accreting Neutron Star

Reference 61

Resolution
verified exact
local_arxiv, observed 2026-06-28T09:01:48.659707Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:d6222c280ad477ecc6ca4681af8b0f8eb5b4e4291b12c2cb1c99f56e371cf956

Observation b13d7c0c-78b3-46a6-b537-384d34f96140 · inbound

Deep optical spectroscopic monitoring of the pulsating ULX NGC 1313 X-2 with longslit Gemini observations cites this paper.

Deep optical spectroscopic monitoring of the pulsating ULX NGC 1313 X-2 with longslit Gemini observations An Ultraluminous X-ray Source Powered by An Accreting Neutron Star

Reference 24

Resolution
verified exact
local_arxiv, observed 2026-06-28T11:32:03.607453Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:1f7f5123d2da837601698e0d738f4332212552aac9648198a2dae8e18cc01eeb

Observation 33d45ce3-8228-4108-ace5-69f76b54f630 · inbound

Exploring Gravitational Wave Signatures Due to Primordial Non-gaussianity and Large Scale Structure Using SKAO cites this paper.

Exploring Gravitational Wave Signatures Due to Primordial Non-gaussianity and Large Scale Structure Using SKAO An Ultraluminous X-ray Source Powered by An Accreting Neutron Star

Reference 294

Resolution
verified exact
local_arxiv, observed 2026-06-27T01:30:20.708019Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:37da8081b6c2b180d600c5c35b2214c412b45dffd29035300d89dfa388220474

Observation bdd85398-0063-48d2-8e3d-ee1eca2c5565 · inbound

Polarimetry of Ultraluminous X-ray sources cites this paper.

Polarimetry of Ultraluminous X-ray sources An Ultraluminous X-ray Source Powered by An Accreting Neutron Star

Reference 24

Resolution
verified exact
local_arxiv, observed 2026-06-29T03:23:04.321144Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:43bed9ac5238e65fb87070a6e20e09b4b56151cad3e8a2c8d5001c8f6638d7ac

Observation 5395377c-5056-4732-b83b-813c006e6961 · inbound

Transient and Variable Ultra-luminous X-ray Sources in NGC 4552 cites this paper.

Transient and Variable Ultra-luminous X-ray Sources in NGC 4552 An Ultraluminous X-ray Source Powered by An Accreting Neutron Star

Reference 64

Resolution
verified exact
local_arxiv, observed 2026-07-09T06:56:03.633534Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:10825017185ba84084832ca052001af5d4c09ca182120441460012a1d7138d3a

Observation 9ad3c8c7-084b-497b-beee-283cc5651ee9 · inbound

Multi-wavelength Constraints on the Transient EP250905a cites this paper.

Multi-wavelength Constraints on the Transient EP250905a An Ultraluminous X-ray Source Powered by An Accreting Neutron Star

Reference 265

Resolution
verified exact
local_arxiv, observed 2026-07-10T13:17:05.366122Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:26077528db40587ee337d73ec002eb58ece6bfaddd04722a33bf9d73ec5e645f

Observation 068077cb-1508-47c2-858d-03beabec783e · inbound

Outflows in super-Eddington quasars drive clumpy circumgalactic medium and extended H$\alpha$ nebulae at $z \gtrsim 6$ cites this paper.

Outflows in super-Eddington quasars drive clumpy circumgalactic medium and extended H$\alpha$ nebulae at $z \gtrsim 6$ An Ultraluminous X-ray Source Powered by An Accreting Neutron Star

Reference 71

Resolution
unresolved
no resolver link, observed 2026-08-01T06:58:38.892215Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T06:58:38.892215Z digest=sha256:2c81e2cc41f29a6601008515612e8857f23abda7f971ff08ee6099cbad0bf2a1