Paper Citation Record · LEDGER

On the formation of super-Jupiters: Core Accretion or Gravitational Instability?

As of 15 August 2026, this Paper Citation Record lists 44 of 44 outbound references and 0 inbound Pith citation observations for arXiv:2412.06594.

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

pith.paper-citation-record.v1
2412.06594 v1

Coverage vector

measured 44 of 44 reference resolution

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Source: paper_references, paper_reference_links, observed 2026-08-11T19:34:24.371140Z

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Pith citing papers itemized under the disclosed page cap.

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measured 0 of 1 external citation measurements

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Source: cited_works

Reference resolution

44 of 44 outbound references displayed

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External citation measurements

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Outbound references

Observation fee3fcd7-4c5f-460c-bf04-d51caa79dfb0 · outbound

This paper cites Heavy metal rules. I. Exoplanet incidence and metallicity.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? Heavy metal rules. I. Exoplanet incidence and metallicity

Reference 1

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Observation 2b25d558-04a9-4f7b-a561-2a453c911060 · outbound

This paper cites Exploring the alpha-enhancement of metal-poor planet-hosting stars. The Kepler and HARPS samples.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? Exploring the alpha-enhancement of metal-poor planet-hosting stars. The Kepler and HARPS samples

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-11T19:34:24.036554Z

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Observation 9c62e139-de10-4b2a-942b-e5c2d49c1f24 · outbound

This paper cites Overabundance of alpha-elements in exoplanet host stars.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? Overabundance of alpha-elements in exoplanet host stars

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-11T19:34:24.043910Z

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Observation cd7aaf1b-37be-4257-9995-a10f2c3461da · outbound

This paper cites Chemical abundances of 1111 FGK stars from the HARPS GTO planet search program.Galactic stellar populations and planets.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? Chemical abundances of 1111 FGK stars from the HARPS GTO planet search program.Galactic stellar populations and planets

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-11T19:34:24.051966Z

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Observation 7655c5fd-42a7-4022-990e-add207363f17 · outbound

This paper cites Orbital and physical properties of planets and their hosts: new insights on planet formation and evolution.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? Orbital and physical properties of planets and their hosts: new insights on planet formation and evolution

Reference 5

Resolution: verified exact; local_arxiv, observed 2026-08-11T19:34:26.083159Z

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Observation 633d9154-e134-4d7a-b65e-6bdbfafeeee6 · outbound

This paper cites The Mass Dependence Between Protoplanetary Disks and their Stellar Hosts.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? The Mass Dependence Between Protoplanetary Disks and their Stellar Hosts

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-11T19:34:24.067569Z

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Observation 3dde7b85-820e-4aeb-981c-61d87f6809f6 · outbound

This paper cites ALMA Survey of Lupus Protoplanetary Disks I: Dust and Gas Masses.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? ALMA Survey of Lupus Protoplanetary Disks I: Dust and Gas Masses

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-11T19:34:24.074182Z

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Observation cd348900-e29c-4db8-bb12-dba6cf44aac9 · outbound

This paper cites The chemical make-up of the Sun: A 2020 vision.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? The chemical make-up of the Sun: A 2020 vision

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-11T19:34:24.086956Z

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Observation 7d9c5065-0f20-4cc8-abce-15ea5fa22798 · outbound

This paper cites Exploring the Milky Way stellar disk. A detailed elemental abundance study of 714 F and G dwarf stars in the Solar neighbourhood.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? Exploring the Milky Way stellar disk. A detailed elemental abundance study of 714 F and G dwarf stars in the Solar neighbourhood

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-11T19:34:24.094380Z

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Observation 1e52a583-7b63-4f51-9524-4603246c7b89 · outbound

This paper cites Science 276:1836--1839.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? Science 276:1836--1839

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-11T19:34:24.108846Z

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Observation 7feba593-b860-4c6c-827e-166d9f9ebba8 · outbound

This paper cites Impacts of radiative accelerations on solar-like oscillating main-sequence stars.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? Impacts of radiative accelerations on solar-like oscillating main-sequence stars

Reference 11

Resolution: verified exact; local_arxiv, observed 2026-08-11T19:34:25.836656Z

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Observation 20d19266-4472-4634-8700-ff7e4b447e34 · outbound

This paper cites Chemical abundances of 1111 FGK stars from the HARPS GTO planet search program IV. Carbon and C/O ratios for Galactic stellar populations and planet hosts.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? Chemical abundances of 1111 FGK stars from the HARPS GTO planet search program IV. Carbon and C/O ratios for Galactic stellar populations and planet hosts

Reference 12

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Observation 06917a87-dc65-4575-afe3-f6ccdd382113 · outbound

This paper cites The Mass Accretion Rate and Stellar Properties in Class I Protostars.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? The Mass Accretion Rate and Stellar Properties in Class I Protostars

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-11T19:34:24.127984Z

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Observation 84007f38-0760-4240-aa12-9b21ebb3c90a · outbound

This paper cites 622(2):1102--1117.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? 622(2):1102--1117

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-11T19:34:24.135492Z

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Observation 2d83681a-7f23-47ed-9251-88812e1b2e6c · outbound

This paper cites The Gaia mission.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? The Gaia mission

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-11T19:34:24.141642Z

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Observation adee7d66-1487-4914-83f1-dd7edb87112c · outbound

This paper cites 399(1):L103--L107.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? 399(1):L103--L107

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-11T19:34:24.150281Z

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Observation e36f7e9a-a997-45ff-a57b-fc98bb55578f · outbound

This paper cites Relation between metallicities and spectral energy distributions of Herbig Ae/Be stars. A potential link with planet formation.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? Relation between metallicities and spectral energy distributions of Herbig Ae/Be stars. A potential link with planet formation

Reference 17

Resolution: verified exact; local_arxiv, observed 2026-08-11T19:34:25.477276Z

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Observation 04d998f0-90d9-4fbf-89da-2da8556d0feb · outbound

This paper cites Stellar Abundances in the Solar Neighborhood: The Hypatia Catalog.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? Stellar Abundances in the Solar Neighborhood: The Hypatia Catalog

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-11T19:34:24.167410Z

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Observation 4c634da5-813e-4bb0-a19d-a65a133c0463 · outbound

This paper cites Computing in Science & Engineering 9(3):90--95.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? Computing in Science & Engineering 9(3):90--95

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-11T19:34:24.172722Z

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Observation 4e80eb4c-8032-4e5b-90cf-3512f810edae · outbound

This paper cites Towards a Deterministic Model of Planetary Formation I: a Desert in the Mass and Semi Major Axis Distributions of Extra Solar Planets.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? Towards a Deterministic Model of Planetary Formation I: a Desert in the Mass and Semi Major Axis Distributions of Extra Solar Planets

Reference 20

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Observation 327c972d-908f-4733-8e2b-1b54840547cb · outbound

This paper cites Dust mass in protoplanetary disks with porous dust opacities.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? Dust mass in protoplanetary disks with porous dust opacities

Reference 21

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Observation 227c5baf-b47f-4d5a-a778-ecdba7f36a8f · outbound

This paper cites Connecting substellar and stellar formation. The role of the host star's metallicity.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? Connecting substellar and stellar formation. The role of the host star's metallicity

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-11T19:34:24.195553Z

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Observation 9b617bfc-cbca-4b93-bc16-926e3ff95d65 · outbound

This paper cites Demographics of young stars and their protoplanetary disks: lessons learned on disk evolution and its connection to planet formation.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? Demographics of young stars and their protoplanetary disks: lessons learned on disk evolution and its connection to planet formation

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-11T19:34:24.201810Z

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Observation c5361b6b-f535-419b-843f-f140a6b5a687 · outbound

This paper cites Formation of a wide-orbit giant planet in a gravitationally unstable subsolar-metallicity protoplanetary disc.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? Formation of a wide-orbit giant planet in a gravitationally unstable subsolar-metallicity protoplanetary disc

Reference 24

Resolution: verified exact; local_arxiv, observed 2026-08-11T19:34:25.285988Z

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Observation 4a01a9c9-82c0-40c2-bc78-4dfe861b82b8 · outbound

This paper cites In: Proceedings of the 9th Python in Science Conference, Austin, TX, pp 51--56.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? In: Proceedings of the 9th Python in Science Conference, Austin, TX, pp 51--56

Reference 25

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Observation c6050de2-37c7-479a-adc6-9add3276b1df · outbound

This paper cites Protoplanetary Disk Masses from Stars to Brown Dwarfs.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? Protoplanetary Disk Masses from Stars to Brown Dwarfs

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-11T19:34:24.222746Z

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Observation c201c221-8b20-45ef-b9c6-fe80eea535ac · outbound

This paper cites Extrasolar planet population synthesis IV. Correlations with disk metallicity, mass and lifetime.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? Extrasolar planet population synthesis IV. Correlations with disk metallicity, mass and lifetime

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-11T19:34:24.230993Z

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Observation 1b2246f3-7b56-43c2-b7ff-4c4c80d9b140 · outbound

This paper cites Properties and occurrence rates of $Kepler$ exoplanet candidates as a function of host star metallicity from the DR25 catalog.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? Properties and occurrence rates of $Kepler$ exoplanet candidates as a function of host star metallicity from the DR25 catalog

Reference 28

Resolution: verified exact; local_arxiv, observed 2026-08-11T19:34:25.133482Z

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Observation be58d2c5-6c81-4f3b-84d0-d07459be8b4c · outbound

This paper cites A Steeper than Linear Disk Mass-Stellar Mass Scaling Relation.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? A Steeper than Linear Disk Mass-Stellar Mass Scaling Relation

Reference 29

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Observation 6977bc1f-694d-448b-a56a-c4fffe7bfc9a · outbound

This paper cites 124(1):62--85.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? 124(1):62--85

Reference 30

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Observation 30050273-b4dc-4973-af2e-eb10ed4dffc2 · outbound

This paper cites Unveiling the time evolution of chemical abundances across the Milky Way disk with APOGEE.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? Unveiling the time evolution of chemical abundances across the Milky Way disk with APOGEE

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-11T19:34:24.262056Z

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Observation 9d44e2b0-18c0-429d-89ae-4408ee7d1ca1 · outbound

This paper cites The PLATO Mission.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? The PLATO Mission

Reference 32

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Observation eb7c25f8-9f56-4b32-b5d0-d187f1e7f8ee · outbound

This paper cites The metal-rich nature of stars with planets.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? The metal-rich nature of stars with planets

Reference 33

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Observation 6155fc07-4195-4a63-bd95-3c2b6114e05d · outbound

This paper cites SWEET-Cat: A catalogue of parameters for Stars With ExoplanETs I. New atmospheric parameters and masses for 48 stars with planets.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? SWEET-Cat: A catalogue of parameters for Stars With ExoplanETs I. New atmospheric parameters and masses for 48 stars with planets

Reference 34

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Observation 91c1f0bb-db9e-44e7-bddf-c7786ea91b75 · outbound

This paper cites Constraining planet structure and composition from stellar chemistry: trends in different stellar populations.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? Constraining planet structure and composition from stellar chemistry: trends in different stellar populations

Reference 35

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Observation 3c57ccdb-9f7a-4014-a242-742c4acbf295 · outbound

This paper cites Observational evidence for two distinct giant planet populations.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? Observational evidence for two distinct giant planet populations

Reference 36

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Observation 0d8c2426-bf20-4351-9beb-3f20cb3f11a4 · outbound

This paper cites Evidence of an Upper Bound on the Masses of Planets and its Implications for Giant Planet Formation.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? Evidence of an Upper Bound on the Masses of Planets and its Implications for Giant Planet Formation

Reference 37

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Observation c5010ad7-5e5b-4ffe-95db-0be281e1933a · outbound

This paper cites In: 9th Python in Science Conference.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? In: 9th Python in Science Conference

Reference 38

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Observation d3160c17-ee55-448e-8652-5e4697f645d8 · outbound

This paper cites arXiv e-prints arXiv:2409.11965.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? arXiv e-prints arXiv:2409.11965

Reference 39

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Observation 9b8e3785-435a-4a18-9cd3-aa27a0e93bb1 · outbound

This paper cites The Deuterium-Burning Mass Limit for Brown Dwarfs and Giant Planets.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? The Deuterium-Burning Mass Limit for Brown Dwarfs and Giant Planets

Reference 40

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Observation 62083565-80fb-49ed-9abb-8d518ab82d68 · outbound

This paper cites Nature Methods 17:261--272.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? Nature Methods 17:261--272

Reference 41

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This paper cites Journal of Open Source Software 6(60):3021.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? Journal of Open Source Software 6(60):3021

Reference 42

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On the formation of super-Jupiters: Core Accretion or Gravitational Instability? , " * write output.state after.block = add.period write newline

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On the formation of super-Jupiters: Core Accretion or Gravitational Instability? write newline

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Pith citing papers

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