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Paper Citation Record · LEDGER

Study of the Balmer decrements for Galactic classical Be stars using the Himalayan Chandra Telescope of India

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2404.10339.

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

pith.paper-citation-record.v1
2404.10339 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 2026-08-08T06:32:00.761636+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T18:31:30.115048Z

measured 1 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

0
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 3dece069-8133-4d62-905c-0cb066581437 · inbound

On-axis afocal telescopes as framework for Cubesat based astronomical imagers and slit-less spectrographs cites this paper.

On-axis afocal telescopes as framework for Cubesat based astronomical imagers and slit-less spectrographs Study of the Balmer decrements for Galactic classical Be stars using the Himalayan Chandra Telescope of India

Reference 7

Resolution
unresolved
no resolver link, observed 2026-08-06T18:31:30.115048Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T18:31:30.115048Z digest=sha256:6ef20fadbd02586495e52565a37a1a1e5c6836ce0ba0e6115301d3681b2c9515

Observation cadf89b6-83f3-4203-a49d-bbaa6dc21d81 · inbound

Non-LTE atmosphere models of very luminous sources and their applicability to Little Red Dots, quasi-stars, and similar objects cites this paper.

Non-LTE atmosphere models of very luminous sources and their applicability to Little Red Dots, quasi-stars, and similar objects Study of the Balmer decrements for Galactic classical Be stars using the Himalayan Chandra Telescope of India

Reference 4

Resolution
verified exact
arxiv_id, observed 2026-05-13T04:47:16.386972Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-05-13T04:45:42.351293Z digest=sha256:7fbeaa020813c73897c1e9955d03021c48c498733a98d20fa22dd730d4cf89da