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Paper Citation Record · LEDGER

Gaia Early Data Release 3: Parallax bias versus magnitude, colour, and position

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 16 inbound Pith citation observations for arXiv:2012.01742.

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

pith.paper-citation-record.v1
2012.01742 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 16 of 16 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-21T06:32:19.484+00:00

measured 16 of 16 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T00:46:38.391148Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T23:07:44.515739Z

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 a1098f24-f095-4473-9c97-4af3dae63ed2 · inbound

Estimating distances from parallaxes. V: Geometric and photogeometric distances to 1.47 billion stars in Gaia Early Data Release 3 cites this paper.

Estimating distances from parallaxes. V: Geometric and photogeometric distances to 1.47 billion stars in Gaia Early Data Release 3 Gaia Early Data Release 3: Parallax bias versus magnitude, colour, and position

Reference 93

Resolution
metadata mismatch
arxiv_id, observed 2026-05-15T04:32:55.526333Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-05-15T04:32:54.967863Z digest=sha256:c28067c3abcbe8316a04a6cbfbd3b63bf2e369211bf0ab533a28a2165feacc27

Observation 602c6709-ef30-4640-ba46-330bdfac5416 · inbound

Basic stellar observables cites this paper.

Basic stellar observables Gaia Early Data Release 3: Parallax bias versus magnitude, colour, and position

Reference 24

Resolution
unresolved
no resolver link, observed 2026-08-11T20:31:57.334173Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T20:31:57.334173Z digest=sha256:7e6bf5a6816e40486c9c8cf92989ea52d1883583c02840d03d66a69abca37944

Observation 7e22b07f-889c-4597-aa3c-8b78729ec807 · inbound

Disruption of a Giant: Spectroscopic Identification of Members in the Periphery and Tidal Tails of $\omega$ Centauri cites this paper.

Disruption of a Giant: Spectroscopic Identification of Members in the Periphery and Tidal Tails of $\omega$ Centauri Gaia Early Data Release 3: Parallax bias versus magnitude, colour, and position

Reference 136

Resolution
verified exact
arxiv_id, observed 2026-05-25T04:00:18.786862Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

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Observation f74381fe-3070-45bf-a9a1-3170ddc6c844 · inbound

Mitigating Charge Migration in JWST NIRISS Reveals That KELT-7 b is a Metal-enriched Ultra-hot Jupiter Orbiting a Young Metal-rich Star cites this paper.

Mitigating Charge Migration in JWST NIRISS Reveals That KELT-7 b is a Metal-enriched Ultra-hot Jupiter Orbiting a Young Metal-rich Star Gaia Early Data Release 3: Parallax bias versus magnitude, colour, and position

Reference 58

Resolution
metadata mismatch
local_arxiv, observed 2026-07-10T23:07:44.530257Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:ecbfb06178ecbfade0e60992778461fcb3eb924d969c7eae5e9661ce2ef24ed5

Observation 50a1e106-5b01-440e-a73d-94382f2e1676 · inbound

Probing the origins. III. Exoplanet demographics across Galactic birth radii cites this paper.

Probing the origins. III. Exoplanet demographics across Galactic birth radii Gaia Early Data Release 3: Parallax bias versus magnitude, colour, and position

Reference 108

Resolution
metadata mismatch
local_arxiv, observed 2026-07-10T18:17:33.139687Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:24ff1ccccc54e9938e6ca00ac782efaf269736d5a3768ed2ed811faef0db59d9

Observation 113e9b03-b316-4f54-9028-0dadecce9b5e · inbound

The potential broader complex linked to the key Cepheid SV Vul cites this paper.

The potential broader complex linked to the key Cepheid SV Vul Gaia Early Data Release 3: Parallax bias versus magnitude, colour, and position

Reference 147

Resolution
unresolved
no resolver link, observed 2026-08-02T03:06:04.624910Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T03:06:04.624910Z digest=sha256:efa0c156372d2f64eac9917e61e9d8f457b983a18ffa1b2d1b2314b8d83c8b53

Observation 6b5d4494-1226-4a55-a41a-e99bf5071b07 · inbound

Effective temperatures estimation of low-mass stars and identification of T Tauri stars in LAMOST DR10 using machine learning cites this paper.

Effective temperatures estimation of low-mass stars and identification of T Tauri stars in LAMOST DR10 using machine learning Gaia Early Data Release 3: Parallax bias versus magnitude, colour, and position

Reference 63

Resolution
unresolved
no resolver link, observed 2026-08-01T20:35:53.334229Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T20:35:53.334229Z digest=sha256:8d4e2f70863d9419b3216462654b40ad41f9511ad408bb1ceecf13a7ad667c31

Observation aa7f30bd-5dc8-4861-a91b-fd76965d27e1 · inbound

Systematic Effects in Gaia CRF Photometry Related to Scanning Geometry and BP/RP excess factor cites this paper.

Systematic Effects in Gaia CRF Photometry Related to Scanning Geometry and BP/RP excess factor Gaia Early Data Release 3: Parallax bias versus magnitude, colour, and position

Reference 5

Resolution
unresolved
no resolver link, observed 2026-08-01T12:21:21.244411Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T12:21:21.244411Z digest=sha256:9779dd504c28c422727388de8388ec621c3fea30f3db5cc752aca181a3b0979f

Observation 83357bf4-493e-4169-bac6-f1c4c507a7be · inbound

LBT-MODS spectroscopy of young stellar objects in the distant metal-poor star forming region Sh2-284: Stellar and accretion properties cites this paper.

LBT-MODS spectroscopy of young stellar objects in the distant metal-poor star forming region Sh2-284: Stellar and accretion properties Gaia Early Data Release 3: Parallax bias versus magnitude, colour, and position

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-01T04:29:12.224496Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T04:29:12.224496Z digest=sha256:0d79f659fb1c2ac9c72c03497c4def62bca2d0c92148e8277b3b4faa85c366c2

Observation 0fceb510-91ec-4e84-9634-6484eb3e6084 · inbound

Cosmological constraints and standard sirens forecasts for non-dynamical dark energy in Horndeski gravity cites this paper.

Cosmological constraints and standard sirens forecasts for non-dynamical dark energy in Horndeski gravity Gaia Early Data Release 3: Parallax bias versus magnitude, colour, and position

Reference 59

Resolution
unresolved
no resolver link, observed 2026-08-08T00:42:49.788240Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation f9553fe3-1015-4fab-91b8-917e03af3647 · inbound

A Galactic intermediate-mass stripped star with a Wolf-Rayet-like wind cites this paper.

A Galactic intermediate-mass stripped star with a Wolf-Rayet-like wind Gaia Early Data Release 3: Parallax bias versus magnitude, colour, and position

Reference 143

Resolution
unresolved
no resolver link, observed 2026-08-08T16:32:31.934975Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T16:32:31.934975Z digest=sha256:9321701c47d78e8ca827cafa381ece2bf6974db339fb19f5e2d29c11a45d0f76

Observation 540d5f92-b616-4a99-979e-772102f1c53e · inbound

Tracing the early Milky Way thin disc with the Gaia-ESO Survey cites this paper.

Tracing the early Milky Way thin disc with the Gaia-ESO Survey Gaia Early Data Release 3: Parallax bias versus magnitude, colour, and position

Reference 83

Resolution
unresolved
no resolver link, observed 2026-08-10T05:52:04.669818Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T05:52:04.669818Z digest=sha256:5cf3660a2e1ac45b8df939d8ea831f7700460c2f01524d22b03f043e70533e61

Observation 5ce4ac9c-bd71-477a-8370-7c5158c32f17 · inbound

Kings of the Milky Way: A Homogeneous Gaia DR3 Analysis of King Open Clusters and the Galactic Disc Metallicity Gradient cites this paper.

Kings of the Milky Way: A Homogeneous Gaia DR3 Analysis of King Open Clusters and the Galactic Disc Metallicity Gradient Gaia Early Data Release 3: Parallax bias versus magnitude, colour, and position

Reference 285

Resolution
unresolved
no resolver link, observed 2026-08-12T00:23:46.034096Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T00:23:46.034096Z digest=sha256:4c8217e1dc93015bd3048013ee1b1bfc3e1d6c8802405573c0ab50ba07b49ccb

Observation e1cc1314-900f-480b-8802-af54ae9ae32c · inbound

Diameters and Temperatures VII: High-angular resolution measurements of Solar-type stars with the CHARA Array cites this paper.

Diameters and Temperatures VII: High-angular resolution measurements of Solar-type stars with the CHARA Array Gaia Early Data Release 3: Parallax bias versus magnitude, colour, and position

Reference 17

Resolution
unresolved
no resolver link, observed 2026-08-15T14:17:31.162104Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-15T14:17:31.162104Z digest=sha256:8f8e964a016fb87e07ae3451844448c542951c3b19328a9e34c633ce891428b1

Observation da3623c4-9dcc-477c-9597-76d2b634fb8e · inbound

A Helium-shell Burning Blue Horizontal Branch Star Produced from Common Envelope Evolution cites this paper.

A Helium-shell Burning Blue Horizontal Branch Star Produced from Common Envelope Evolution Gaia Early Data Release 3: Parallax bias versus magnitude, colour, and position

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-16T00:46:38.391148Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:46:38.391148Z digest=sha256:3b34e354006d945071ab12c8e9b26585fa99b18910dd2d6cc876fb64f487364c

Observation cc48e442-673c-4ecc-a92f-9b7c6dcd5c8d · inbound

Gaia parallax bias via spherical harmonics: A Python tool and discussion of possible causes cites this paper.

Gaia parallax bias via spherical harmonics: A Python tool and discussion of possible causes Gaia Early Data Release 3: Parallax bias versus magnitude, colour, and position

Reference 14

Resolution
unresolved
no resolver link, observed 2026-08-16T00:11:56.122983Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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