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Paper Citation Record · LEDGER

A distance to the Large Magellanic Cloud that is precise to one per cent

As of 14 July 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:1903.08096.

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

pith.paper-citation-record.v1
1903.08096 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 9 of 9 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-07-13T06:30:06.624239+00:00

measured 9 of 9 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 2026-06-28T10:12:02.276230Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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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 a0a6a831-67fd-4469-ab14-68e2f3a2425d · inbound

Stellar microlensing surveys as a probe of Primordial Black Holes: status and prospects cites this paper.

Stellar microlensing surveys as a probe of Primordial Black Holes: status and prospects A distance to the Large Magellanic Cloud that is precise to one per cent

Reference 34

Resolution
verified exact
local_arxiv, observed 2026-05-15T21:26:38.976943Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.

source=pdf_text observed=2026-07-11T11:50:26.030339Z digest=sha256:c2bf04333a5c765b38f475ee247e6271357a53b60297579c40e974117f21810e

Observation 1ae6c9c1-16e2-44e2-80e6-617b2d38380a · inbound

Scylla VI: Parsec-Scale Dust Extinction Maps in the SMC and LMC cites this paper.

Scylla VI: Parsec-Scale Dust Extinction Maps in the SMC and LMC A distance to the Large Magellanic Cloud that is precise to one per cent

Reference 70

Resolution
metadata mismatch
arxiv_id, observed 2026-05-11T04:50:58.719792Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.

source=pdf_text observed=2026-05-11T01:00:40.787267Z digest=sha256:b74e4ef40ba5af1b983727c9ce7d051a3d52d50f1f73726d735d3069fa83d4e8

Observation f2299d70-1409-4fb8-b9a8-7822cb2d941f · inbound

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion cites this paper.

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion A distance to the Large Magellanic Cloud that is precise to one per cent

Reference 38

Resolution
verified exact
local_arxiv, observed 2026-05-19T16:12:39.061673Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.

source=pdf_text observed=2026-05-19T16:10:46.102334Z digest=sha256:99f81a4f17831335872a528f7428e31d23804785690daf8e90ca9701e121e8b4

Observation a33fc74a-b953-40a6-ad25-125148f0ce51 · inbound

The VMC survey -- LV. The coherent expansion of the SMC cites this paper.

The VMC survey -- LV. The coherent expansion of the SMC A distance to the Large Magellanic Cloud that is precise to one per cent

Reference 126

Resolution
verified exact
local_arxiv, observed 2026-06-28T10:12:02.277486Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:989ec0e8ac0cba107f70bb5d523a18bd7be4431c0e990fa875de2f85e59dd626

Observation 81acb5dd-5354-4a7a-9e48-e0f0374137bf · inbound

Milky Way's warped disc traced by AGB stars cites this paper.

Milky Way's warped disc traced by AGB stars A distance to the Large Magellanic Cloud that is precise to one per cent

Reference 74

Resolution
verified exact
local_arxiv, observed 2026-06-27T18:51:08.918288Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:255b03196735fb791400afd7e4822ce3bef4c3198c1b8ee7bd3b719854c1ef62

Observation 18c32ed8-08dc-4fdf-8502-083ff943994c · inbound

Rogue Ones: Orbital census of Galactic Cepheids and their Anomalies cites this paper.

Rogue Ones: Orbital census of Galactic Cepheids and their Anomalies A distance to the Large Magellanic Cloud that is precise to one per cent

Reference 58

Resolution
verified exact
local_arxiv, observed 2026-06-27T13:10:56.456787Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:a92eb902686cf603abbd937ca6942495707ef7f3e6984e6c931f9271e234d4a3

Observation a2146bdb-c99c-4189-a318-7e6b6f4a13fe · inbound

Variables in S-PLUS: I. Multiband period-luminosity relations and reddening maps of the Magellanic Clouds using classical Cepheids cites this paper.

Variables in S-PLUS: I. Multiband period-luminosity relations and reddening maps of the Magellanic Clouds using classical Cepheids A distance to the Large Magellanic Cloud that is precise to one per cent

Reference 60

Resolution
verified exact
local_arxiv, observed 2026-06-26T16:49:36.596919Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:42a007d8ac9a6a918fcb5635bbca77d95b50e382ecc453a0fb5fe1533b0257bf

Observation 766c5f20-5ba4-43c9-926e-096a783ff970 · inbound

Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI cites this paper.

Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI A distance to the Large Magellanic Cloud that is precise to one per cent

Reference 184

Resolution
verified exact
local_arxiv, observed 2026-06-26T18:09:41.416446Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:40f463103aec2ce4441b356dc5725f4c45c72914c98089a966383599143561b4

Observation f4d88f91-d240-4066-a533-1befcbfeecc8 · inbound

Cepheids with giant companions III. Evolutionary modeling of nine binary double Cepheids from the Milky Way and Magellanic Clouds cites this paper.

Cepheids with giant companions III. Evolutionary modeling of nine binary double Cepheids from the Milky Way and Magellanic Clouds A distance to the Large Magellanic Cloud that is precise to one per cent

Reference 20

Resolution
verified exact
local_arxiv, observed 2026-06-26T02:48:56.558683Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:2bcd52c2f0c20c18f31536aeac93f5c13fd9a6fab17db2a3771e883ef97acf3f