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Paper Citation Record · LEDGER

How to Constrain Your M dwarf II: the mass-luminosity-metallicity relation from 0.075 to 0.70$M_\odot$

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:1811.06938.

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

pith.paper-citation-record.v1
1811.06938 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T12:38:25.408477Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-30T04:24:19.807205Z

Reference resolution

0 of 0 outbound references displayed

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External citation measurements

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 5f3a0920-834f-411a-8e85-3451e03b19a5 · inbound

Absence of a thick atmosphere on the terrestrial exoplanet LHS 3844b cites this paper.

Absence of a thick atmosphere on the terrestrial exoplanet LHS 3844b How to Constrain Your M dwarf II: the mass-luminosity-metallicity relation from 0.075 to 0.70$M_\odot$

Reference 42

Resolution
unresolved
no resolver link, observed 2026-08-14T12:38:25.408477Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 10ff2d33-434e-46fb-826e-2160f9cea3d3 · inbound

The mass of TOI-1883 b: A low density super-Neptune in the ridge regime transiting an early-M dwarf cites this paper.

The mass of TOI-1883 b: A low density super-Neptune in the ridge regime transiting an early-M dwarf How to Constrain Your M dwarf II: the mass-luminosity-metallicity relation from 0.075 to 0.70$M_\odot$

Reference 81

Resolution
verified exact
local_arxiv, observed 2026-06-27T21:21:16.670721Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:f18074e69b80312764f8cb4f5f3a22661d7df8a6258875c16c1dfee21609cf02

Observation 7e0f3e95-7aac-499b-9808-252f5c864fd6 · inbound

Revisiting the Exo-Mercury Candidate GJ 367 b with ESPRESSO and a Self-Consistent Tidal Distortion Model cites this paper.

Revisiting the Exo-Mercury Candidate GJ 367 b with ESPRESSO and a Self-Consistent Tidal Distortion Model How to Constrain Your M dwarf II: the mass-luminosity-metallicity relation from 0.075 to 0.70$M_\odot$

Reference 146

Resolution
verified exact
local_arxiv, observed 2026-06-26T22:50:13.723439Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:d6e0fce4ea3f041f8c04fe2a8c20b4381a298c2c6adbbc9fcef0d739bca3638b

Observation 735bcb0f-deb7-4fb0-80af-b51226c5b1de · inbound

ASTEP confirmation of a pair of long-period Jupiter-sized planets with extremely low densities transiting TOI-791 cites this paper.

ASTEP confirmation of a pair of long-period Jupiter-sized planets with extremely low densities transiting TOI-791 How to Constrain Your M dwarf II: the mass-luminosity-metallicity relation from 0.075 to 0.70$M_\odot$

Reference 178

Resolution
verified exact
local_arxiv, observed 2026-06-30T04:24:19.809495Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:84b956c5e147e54baaa83253afe934c6cdfdd34af6353ad0b1eec5b06cd3f8e3

Observation 8c26d653-e4fa-4c63-8b5c-64e1219c4673 · inbound

BOSS-CLAM: Utilizing a Constrained Linear Absorption Model to Infer Stellar Parameters from BOSS Spectra cites this paper.

BOSS-CLAM: Utilizing a Constrained Linear Absorption Model to Infer Stellar Parameters from BOSS Spectra How to Constrain Your M dwarf II: the mass-luminosity-metallicity relation from 0.075 to 0.70$M_\odot$

Reference 91

Resolution
unresolved
no resolver link, observed 2026-08-01T04:28:39.987568Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T04:28:39.987568Z digest=sha256:612ac6239045b82cbfd97e9ede9539f9cae53c27dd835c3623e61ff9edf2de65

Observation 731f0976-aee1-4e29-8617-5691d2e475b1 · inbound

The Twentieth Data Release of the Sloan Digital Sky Survey: First All-Sky BOSS Spectra, eROSITA-SDSS-V Mapper Coordinated Observations, and a Preview of the Local Volume Mapper cites this paper.

The Twentieth Data Release of the Sloan Digital Sky Survey: First All-Sky BOSS Spectra, eROSITA-SDSS-V Mapper Coordinated Observations, and a Preview of the Local Volume Mapper How to Constrain Your M dwarf II: the mass-luminosity-metallicity relation from 0.075 to 0.70$M_\odot$

Reference 290

Resolution
unresolved
no resolver link, observed 2026-08-01T00:41:50.145636Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T00:41:50.145636Z digest=sha256:c0635f17a190f16c4dc4c94d50e35b888a6abf98568b9c38a6d197659fec872b