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Paper Citation Record · LEDGER

REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2501.09058.

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

pith.paper-citation-record.v1
2501.09058 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 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 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-12T07:44:24.116339Z

measured 1 of 1 external citation measurements

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

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

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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External citation measurements

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

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 644a21d4-e927-4869-a540-fd98cc5034b2 · inbound

$\alpha\beta q_\mathrm{th}$-mapping of planet-induced density wave damping in protoplanetary discs cites this paper.

$\alpha\beta q_\mathrm{th}$-mapping of planet-induced density wave damping in protoplanetary discs REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths

Reference 282

Resolution
verified exact
arxiv_id, observed 2026-05-14T20:27:56.754575Z

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=2026-05-14T20:25:56.002658Z digest=sha256:e953474de06cd37bcf9f1c66db2022e64b9204cc195f163e5b2633e2944c1456

Observation 7c92e7aa-1dc9-4b15-975c-96551b42c6a9 · inbound

The Longest-period Young Transiting Exoplanets. A Duo of Puffy Giants inside a Debris Disk cites this paper.

The Longest-period Young Transiting Exoplanets. A Duo of Puffy Giants inside a Debris Disk REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths

Reference 48

Resolution
unresolved
no resolver link, observed 2026-07-12T07:44:24.116339Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-12T07:44:24.116339Z digest=sha256:318a05806ca1951f61da765fba187666ab97066400b3e7e515c5e94f9a85bd9d

Observation 544c456e-6f2b-49f0-b4dd-e05de6728974 · inbound

A search for circumstellar gas in pre-main-sequence debris discs using absorption spectroscopy cites this paper.

A search for circumstellar gas in pre-main-sequence debris discs using absorption spectroscopy REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths

Reference 74

Resolution
metadata mismatch
local_arxiv, observed 2026-07-10T10:27:01.468486Z

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=sha256:1951f0c4f3bbcd2cb865d56ebc50a21169b3f427cee72572124f9daf09c64fcc