Pith. sign in

Paper Citation Record · LEDGER

Timing and spectral study of the Be XRB IGR J11305-6256: Swift discovers the orbital period and a soft X-ray excess

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1305.3916.

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

pith.paper-citation-record.v1
1305.3916 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T05:50:58.522497Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-14T18:16:19.847625Z

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 7cac16b3-a258-4dad-ae3b-f775160590fe · inbound

On Neutron Star Natal Kicks in High-Mass X-Ray Binaries: Insights from Population Synthesis cites this paper.

On Neutron Star Natal Kicks in High-Mass X-Ray Binaries: Insights from Population Synthesis Timing and spectral study of the Be XRB IGR J11305-6256: Swift discovers the orbital period and a soft X-ray excess

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-16T05:50:58.522497Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T05:50:58.522497Z digest=sha256:c1acb4919350d49e5b5453995e3731f8bef93692ac20e7c25124cd49c97fe08a

Observation b63b8bd5-50f8-4371-9b68-77b19a1c1986 · 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 Timing and spectral study of the Be XRB IGR J11305-6256: Swift discovers the orbital period and a soft X-ray excess

Reference 184

Resolution
verified exact
local_arxiv, observed 2026-08-14T15:23:52.563627Z

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.

source=arxiv_source observed=2026-08-14T15:20:02.821147Z digest=sha256:f6360f0cff4ea53dbe8f948375de2dddf0f2ad70ad397b765a4c8ab62962dcdd