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Paper Citation Record · LEDGER

The R136 star cluster dissected with Hubble Space Telescope/STIS. I. Far-ultraviolet spectroscopic census and the origin of HeII 1640 in young star clusters

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1603.04994.

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

pith.paper-citation-record.v1
1603.04994 v1

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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 2026-08-05T06:32:48.257954+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-01T05:05:24.413305Z

Reference resolution

0 of 0 outbound references displayed

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Outbound references

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Pith citing papers

Observation 1d6f0cd5-dbe0-402e-8fdf-534ced375920 · inbound

Quenching of X-ray emission in little red dots by both Compton-thick gas and high accretion rates cites this paper.

Quenching of X-ray emission in little red dots by both Compton-thick gas and high accretion rates The R136 star cluster dissected with Hubble Space Telescope/STIS. I. Far-ultraviolet spectroscopic census and the origin of HeII 1640 in young star clusters

Reference 105

Resolution
verified exact
local_arxiv, observed 2026-05-19T16:17:39.809413Z

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=sha256:1ed3d468d5583fba7b770bfe5e48e8e07fa119fa0de8d2bb96216fb1f479f2bf

Observation 6d54a977-2195-4199-a6d2-9ff3ec9fc8fa · inbound

The metallicities of little red dot host galaxies: LRDs are metal poor, but not pristine cites this paper.

The metallicities of little red dot host galaxies: LRDs are metal poor, but not pristine The R136 star cluster dissected with Hubble Space Telescope/STIS. I. Far-ultraviolet spectroscopic census and the origin of HeII 1640 in young star clusters

Reference 239

Resolution
verified exact
local_arxiv, observed 2026-07-01T05:05:24.415477Z

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:cb3cc1cb5331b440bdb69bc81195cebe066f5dcfd31a32202d95e02c74fee1ef