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 23 August 2026, this Paper Citation Record lists 31 of 31 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 31 of 31 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-10T20:16:55.533782Z

measured 34 of 34 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-23T06:30:58.430688+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

31 of 31 outbound references displayed

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External citation measurements

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

Outbound references

Observation 410852fe-9903-477e-8ee3-07945cfc80c0 · outbound

This paper cites The ALMA Development Program: Roadmap to 2030.

REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths The ALMA Development Program: Roadmap to 2030

Reference 1

Resolution: malformed identifier; no resolver link, observed 2026-08-10T20:16:55.399591Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 13d701e1-984d-421e-871d-d130ba41c49b · outbound

This paper cites 2018), or moving group age also from Gagné et al.

REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths 2018), or moving group age also from Gagné et al

Reference 2

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T20:16:55.993211Z

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Observation ed7a01c8-c3f8-45ae-bb9d-c406a8dc2f05 · outbound

This paper cites 2018), but moving group age from Zuckerman (2019) -.

REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths 2018), but moving group age from Zuckerman (2019) -

Reference 3

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T20:16:55.979604Z

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Observation 418bf59e-f8ea-415a-8ef5-fed0cd17d61b · outbound

This paper cites References.

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

Reference 4

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T20:16:55.965001Z

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Observation a8da65cf-6d4f-4180-b0be-0001c9822c0b · outbound

This paper cites (2014) -.

REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths (2014) -

Reference 5

Resolution: parse uncertain; raw_fallback, observed 2026-08-10T20:16:55.951197Z

Source-reported events for the cited work

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Observation 71e6e97d-7ffb-44ee-b8ba-ac94e1a5ed3b · outbound

This paper cites (2007) -.

REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths (2007) -

Reference 6

Resolution: parse uncertain; raw_fallback, observed 2026-08-10T20:16:55.937158Z

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Observation 6e20753f-9c6b-4900-9cc6-c5ddb340dc8d · outbound

This paper cites (2022, and refs.

REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths (2022, and refs

Reference 7

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T20:16:55.923605Z

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Observation cd65675e-116d-4a92-8f7b-4d6170b8f788 · outbound

This paper cites an unresolved cited work.

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

Reference 8

Resolution: parse uncertain; raw_fallback, observed 2026-08-10T20:16:55.910607Z

Source-reported events for the cited work

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Observation d6c26f14-fd3e-4b59-8712-71d2e504eae8 · outbound

This paper cites (2005) -.

REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths (2005) -

Reference 9

Resolution: parse uncertain; raw_fallback, observed 2026-08-10T20:16:55.896467Z

Source-reported events for the cited work

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Observation 6c794671-b756-41d1-85af-9264df9c7606 · outbound

This paper cites (2015) -.

REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths (2015) -

Reference 10

Resolution: parse uncertain; raw_fallback, observed 2026-08-10T20:16:55.882695Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 8716a765-eebe-4314-a455-1fe9517fc9e0 · outbound

This paper cites (2013) -.

REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths (2013) -

Reference 11

Resolution: parse uncertain; raw_fallback, observed 2026-08-10T20:16:55.868116Z

Source-reported events for the cited work

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Observation 0c80e3a7-b6b7-4b13-9412-0f23f7e0e9c3 · outbound

This paper cites (2016) -.

REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths (2016) -

Reference 12

Resolution: parse uncertain; raw_fallback, observed 2026-08-10T20:16:55.854650Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 917625b3-a12c-4a29-b335-cc43649320ce · outbound

This paper cites (2016) -.

REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths (2016) -

Reference 13

Resolution: parse uncertain; raw_fallback, observed 2026-08-10T20:16:55.841062Z

Source-reported events for the cited work

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Observation 01239136-8966-454d-b2d2-dc64734c801d · outbound

This paper cites (2014) -.

REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths (2014) -

Reference 14

Resolution: parse uncertain; raw_fallback, observed 2026-08-10T20:16:55.827253Z

Source-reported events for the cited work

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Observation b5e85bf8-96ec-423a-b05d-2e6a15d85427 · outbound

This paper cites (2016) -.

REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths (2016) -

Reference 15

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T20:16:55.813542Z

Source-reported events for the cited work

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Observation 9222a4cf-a0aa-443c-a8d9-613bcf287601 · outbound

This paper cites (2010) -.

REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths (2010) -

Reference 16

Resolution: parse uncertain; raw_fallback, observed 2026-08-10T20:16:55.799870Z

Source-reported events for the cited work

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Observation 55d46b3c-a6d5-4c79-93a4-b44291ae1438 · outbound

This paper cites (2006) -.

REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths (2006) -

Reference 17

Resolution: parse uncertain; raw_fallback, observed 2026-08-10T20:16:55.785369Z

Source-reported events for the cited work

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Observation dd15a050-46ef-4817-bb81-9448a2b44bc8 · outbound

This paper cites (2019) -.

REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths (2019) -

Reference 18

Resolution: parse uncertain; raw_fallback, observed 2026-08-10T20:16:55.771872Z

Source-reported events for the cited work

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Observation 2719ab1a-8b6e-4027-aaf6-7a10b37468c1 · outbound

This paper cites (2011) -.

REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths (2011) -

Reference 19

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T20:16:55.757830Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 95abfccd-b06e-4362-a37d-ecfc3f358385 · outbound

This paper cites (2012) -.

REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths (2012) -

Reference 20

Resolution: parse uncertain; raw_fallback, observed 2026-08-10T20:16:55.743807Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 9e280644-f811-4ae1-95fa-55f2b2b29cb7 · outbound

This paper cites (2017) -.

REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths (2017) -

Reference 21

Resolution: parse uncertain; raw_fallback, observed 2026-08-10T20:16:55.730149Z

Source-reported events for the cited work

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Observation fa366e30-b84c-4416-a512-204799882adb · outbound

This paper cites (2008) -.

REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths (2008) -

Reference 22

Resolution: parse uncertain; raw_fallback, observed 2026-08-10T20:16:55.716059Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 193074d9-306d-4fb6-b402-9190cd051bf1 · outbound

This paper cites (2011) -.

REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths (2011) -

Reference 23

Resolution: parse uncertain; raw_fallback, observed 2026-08-10T20:16:55.702163Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation f4e16c9f-aab2-4583-8d81-04fb181cb4c3 · outbound

This paper cites (2000) -.

REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths (2000) -

Reference 24

Resolution: parse uncertain; raw_fallback, observed 2026-08-10T20:16:55.687258Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation e974a5fd-71f6-4f43-b006-b7da5d9722c0 · outbound

This paper cites (2015) -.

REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths (2015) -

Reference 25

Resolution: parse uncertain; raw_fallback, observed 2026-08-10T20:16:55.673001Z

Source-reported events for the cited work

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Observation 91663a66-b9bd-4eb3-8299-ed00d6d6be8b · outbound

This paper cites (2023) Article number, page 22 of 27 L.

REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths (2023) Article number, page 22 of 27 L

Reference 26

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T20:16:55.658419Z

Source-reported events for the cited work

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Observation 1fc6df54-cdeb-4989-ba5a-a6096adae21a · outbound

This paper cites ) 20 10 0 10 20 North offset (.

REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths ) 20 10 0 10 20 North offset (

Reference 27

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T20:16:55.643162Z

Source-reported events for the cited work

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Observation 52333299-789d-46a2-8d75-e674e15dbeeb · outbound

This paper cites an unresolved cited work.

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

Reference 28

Resolution: unresolved; raw_fallback, observed 2026-08-10T20:16:55.628230Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 1d816789-154b-4fb2-a85d-190028f07596 · outbound

This paper cites 32 of Holland et al.

REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths 32 of Holland et al

Reference 29

Resolution: verified fuzzy; raw_fallback, observed 2026-08-10T20:16:55.613484Z

Source-reported events for the cited work

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Observation 9019d484-48c2-4873-9320-3958f37d41f1 · outbound

This paper cites ) 20 10 0 10 20 North offset (.

REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A population of 74 resolved planetesimal belts at millimetre wavelengths ) 20 10 0 10 20 North offset (

Reference 30

Resolution: malformed identifier; raw_fallback, observed 2026-08-10T20:16:55.599413Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 6a69aa38-0db8-4dd9-b5fd-8c3a01c3f153 · outbound

This paper cites an unresolved cited work.

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

Reference 31

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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

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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

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.

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 2026-08-23T06:30:58.430688+00:00.