Paper Citation Record · LEDGER

The majority of hot Jupiters formed beyond the water ice line

As of 12 August 2026, this Paper Citation Record lists 60 of 60 outbound references and 1 inbound Pith citation observation for arXiv:2607.15144.

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

pith.paper-citation-record.v1
2607.15144 v1

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measured 60 of 60 reference resolution

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Source: paper_references, paper_reference_links, observed 2026-08-02T00:06:51.327288Z

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00

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Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T16:19:18.591636Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-06T18:16:30.548575Z

Reference resolution

60 of 60 outbound references displayed

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Outbound references

Observation 9b64f476-21b3-46e1-b30d-31075e763fe5 · outbound

This paper cites Disk Frequencies and Lifetimes in Young Clusters.

The majority of hot Jupiters formed beyond the water ice line Disk Frequencies and Lifetimes in Young Clusters

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:47.256943Z

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Observation 999eefa4-d232-470c-a3eb-ddf44f7c1848 · outbound

This paper cites Protoplanetary Disks and Their Evolution.

The majority of hot Jupiters formed beyond the water ice line Protoplanetary Disks and Their Evolution

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:47.307651Z

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Observation 2919edec-051c-4660-9e7d-7922f8b5140b · outbound

This paper cites Protoplanetary disk lifetimes vs stellar mass and possible implications for giant planet populations.

The majority of hot Jupiters formed beyond the water ice line Protoplanetary disk lifetimes vs stellar mass and possible implications for giant planet populations

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:47.363594Z

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Unavailable: canonical work link unavailable.

Observation a831c936-2127-4f20-8019-f4bd3083fe0c · outbound

This paper cites Planetesimal rings as the cause of the Solar System's planetary architecture.

The majority of hot Jupiters formed beyond the water ice line Planetesimal rings as the cause of the Solar System's planetary architecture

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:47.418913Z

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Unavailable: canonical work link unavailable.

Observation 84584406-1cf2-47ec-8f77-61e1735aa291 · outbound

This paper cites , year = 1995, month = nov, volume =.

The majority of hot Jupiters formed beyond the water ice line , year = 1995, month = nov, volume =

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:47.476252Z

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Observation f9958a37-e544-4f5e-a152-f3ca1b8ce972 · outbound

This paper cites , year = 1996, month = apr, volume =.

The majority of hot Jupiters formed beyond the water ice line , year = 1996, month = apr, volume =

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:47.531025Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2a15ac7a-5e9c-4e14-87fe-349f6dc0ed0b · outbound

This paper cites an unresolved cited work.

The majority of hot Jupiters formed beyond the water ice line Unresolved cited work

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:47.654940Z

Source-reported events for the cited work

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Observation ea623e0b-e6be-4749-9d79-9f5486fa08ab · outbound

This paper cites Extrasolar planet population synthesis I: Method, formation tracks and mass-distance distribution.

The majority of hot Jupiters formed beyond the water ice line Extrasolar planet population synthesis I: Method, formation tracks and mass-distance distribution

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:47.735104Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ad1689cb-ce4a-453a-ad3e-f63e1289634f · outbound

This paper cites The growth of planets by pebble accretion in evolving protoplanetary discs.

The majority of hot Jupiters formed beyond the water ice line The growth of planets by pebble accretion in evolving protoplanetary discs

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:47.868194Z

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Observation 35398e30-7234-4bac-8aa3-6b3c974b6ce5 · outbound

This paper cites Science , keywords =.

The majority of hot Jupiters formed beyond the water ice line Science , keywords =

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:47.963776Z

Source-reported events for the cited work

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Observation 0379f0e4-6fd6-46c3-88ca-7b970e57569c · outbound

This paper cites Shrinking binary and planetary orbits by Kozai cycles with tidal friction.

The majority of hot Jupiters formed beyond the water ice line Shrinking binary and planetary orbits by Kozai cycles with tidal friction

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:48.068829Z

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Observation 3f3dd274-cf15-4170-bb73-49776499cc38 · outbound

This paper cites Multiple-Planet Scattering and the Origin of Hot Jupiters.

The majority of hot Jupiters formed beyond the water ice line Multiple-Planet Scattering and the Origin of Hot Jupiters

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:48.172686Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 457c252e-bde3-4555-865d-3d0557a4cdf8 · outbound

This paper cites Origins of Hot Jupiters.

The majority of hot Jupiters formed beyond the water ice line Origins of Hot Jupiters

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:48.273770Z

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Observation 4daeb565-5a38-483d-ba2e-994bde797a79 · outbound

This paper cites The effects of snowlines on C/O in planetary atmospheres.

The majority of hot Jupiters formed beyond the water ice line The effects of snowlines on C/O in planetary atmospheres

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:48.410619Z

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Observation 4c9bc51c-2351-4ec9-aa2a-0c6e066eeed5 · outbound

This paper cites Molecular abundances and C/O ratios in chemically evolving planet-forming disk midplanes.

The majority of hot Jupiters formed beyond the water ice line Molecular abundances and C/O ratios in chemically evolving planet-forming disk midplanes

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:48.504921Z

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Observation 38d4d3f9-ba05-4648-bd3b-a0c0f78f27bf · outbound

This paper cites Interpreting the atmospheric composition of exoplanets: sensitivity to planet formation assumptions.

The majority of hot Jupiters formed beyond the water ice line Interpreting the atmospheric composition of exoplanets: sensitivity to planet formation assumptions

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:48.655345Z

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Observation 2029c169-83d8-4289-a0ce-ae1bb5bc8936 · outbound

This paper cites Atmospheric Signatures of Giant Exoplanet Formation by Pebble Accretion.

The majority of hot Jupiters formed beyond the water ice line Atmospheric Signatures of Giant Exoplanet Formation by Pebble Accretion

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:48.783955Z

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Observation f3fff980-bf05-432e-9a0a-782d70970248 · outbound

This paper cites Composition of Early Planetary Atmospheres II: Coupled Dust and Chemical Evolution in Protoplanetary Disks.

The majority of hot Jupiters formed beyond the water ice line Composition of Early Planetary Atmospheres II: Coupled Dust and Chemical Evolution in Protoplanetary Disks

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:48.914479Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bd1ceeb4-0091-4e94-bcb6-a52f725989ae · outbound

This paper cites How drifting and evaporating pebbles shape giant planets I: Heavy element content and atmospheric C/O.

The majority of hot Jupiters formed beyond the water ice line How drifting and evaporating pebbles shape giant planets I: Heavy element content and atmospheric C/O

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:49.085278Z

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Observation 02046054-ea64-49c2-afa2-8f84e589405e · outbound

This paper cites Tracing the formation history of giant planets in protoplanetary disks with Carbon, Oxygen, Nitrogen and Sulphur.

The majority of hot Jupiters formed beyond the water ice line Tracing the formation history of giant planets in protoplanetary disks with Carbon, Oxygen, Nitrogen and Sulphur

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:49.168782Z

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Observation 88c9b06b-a18b-43c4-97cf-0e29fe9af7f5 · outbound

This paper cites How drifting and evaporating pebbles shape giant planets III: The formation of WASP-77A b and $\tau$ Bo\"otis b.

The majority of hot Jupiters formed beyond the water ice line How drifting and evaporating pebbles shape giant planets III: The formation of WASP-77A b and $\tau$ Bo\"otis b

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:49.213333Z

Source-reported events for the cited work

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Observation bca71ab8-e65e-4645-9260-7be2b96ffa7d · outbound

This paper cites Volatiles in protoplanetary disks.

The majority of hot Jupiters formed beyond the water ice line Volatiles in protoplanetary disks

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:49.266206Z

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Unavailable: canonical work link unavailable.

Observation f1db0d34-1b07-4469-afd3-4aa71a7588f7 · outbound

This paper cites C/O and Snowline Locations in Protoplanetary Disks: The Effect of Radial Drift and Viscous Gas Accretion.

The majority of hot Jupiters formed beyond the water ice line C/O and Snowline Locations in Protoplanetary Disks: The Effect of Radial Drift and Viscous Gas Accretion

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:49.338038Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6fb6a2e5-222b-4abc-aa4d-e6010ee441a5 · outbound

This paper cites Chemical enrichment of giant planets and discs due to pebble drift.

The majority of hot Jupiters formed beyond the water ice line Chemical enrichment of giant planets and discs due to pebble drift

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:49.396821Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8bed84b3-a15d-4218-b938-188778c5f7fb · outbound

This paper cites How to make giant planets via pebble accretion.

The majority of hot Jupiters formed beyond the water ice line How to make giant planets via pebble accretion

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:49.462135Z

Source-reported events for the cited work

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Observation 57c1286f-2cf1-4e36-9afc-920b5ddfe005 · outbound

This paper cites Composition of giant planets: the roles of pebbles and planetesimals.

The majority of hot Jupiters formed beyond the water ice line Composition of giant planets: the roles of pebbles and planetesimals

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:49.518253Z

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Observation 1048b4de-f298-4270-b126-088146aac1d8 · outbound

This paper cites BOWIE-ALIGN: How formation and migration histories of giant planets impact atmospheric compositions.

The majority of hot Jupiters formed beyond the water ice line BOWIE-ALIGN: How formation and migration histories of giant planets impact atmospheric compositions

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:49.569628Z

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Observation d6f372bc-aeb2-4e76-9d9a-883387a8c37c · outbound

This paper cites , keywords =.

The majority of hot Jupiters formed beyond the water ice line , keywords =

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:49.600728Z

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Observation 1392689a-25a8-4cde-b85a-3c69696fa6fd · outbound

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

The majority of hot Jupiters formed beyond the water ice line Stellar Abundances in the Solar Neighborhood: The Hypatia Catalog

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:49.647846Z

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Observation dad92808-f88a-421f-9ea7-884fb78aa482 · outbound

This paper cites Burned to ashes: How the thermal decomposition of refractory organics in the inner protoplanetary disc impacts the gas-phase C/O ratio.

The majority of hot Jupiters formed beyond the water ice line Burned to ashes: How the thermal decomposition of refractory organics in the inner protoplanetary disc impacts the gas-phase C/O ratio

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:49.700933Z

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Observation 51075519-a0bc-4217-bdf4-8b0c74252b26 · outbound

This paper cites , keywords =.

The majority of hot Jupiters formed beyond the water ice line , keywords =

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:49.754432Z

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Observation 58e2aa90-e2b2-4940-ab5f-8f16ac9571cd · outbound

This paper cites Re-analysis of 10 Hot-Jupiter Atmospheres with disequilibrium chemistry retrieval.

The majority of hot Jupiters formed beyond the water ice line Re-analysis of 10 Hot-Jupiter Atmospheres with disequilibrium chemistry retrieval

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:49.807110Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 45c9a040-9e35-4df5-80de-e61bb785c90a · outbound

This paper cites A simple model for the evolution of the dust population in protoplanetary disks.

The majority of hot Jupiters formed beyond the water ice line A simple model for the evolution of the dust population in protoplanetary disks

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:49.858716Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 769d56dc-45ef-44a7-b564-96e36ee19454 · outbound

This paper cites Probing the impact of varied migration and gas accretion rates for the formation of giant planets in the pebble accretion scenario.

The majority of hot Jupiters formed beyond the water ice line Probing the impact of varied migration and gas accretion rates for the formation of giant planets in the pebble accretion scenario

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:49.931730Z

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Observation f4bb0772-fa97-46ed-82b5-21594652a457 · outbound

This paper cites The multifaceted planetesimal formation process.

The majority of hot Jupiters formed beyond the water ice line The multifaceted planetesimal formation process

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:49.978110Z

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Observation b8c30e92-a788-4bb3-bed3-8b2349035058 · outbound

This paper cites Effects of diffusion.

The majority of hot Jupiters formed beyond the water ice line Effects of diffusion

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:50.012361Z

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Observation 14b4c4f6-1556-4ba9-9049-2e468340fcfa · outbound

This paper cites A solar C/O and sub-solar metallicity in a hot Jupiter atmosphere.

The majority of hot Jupiters formed beyond the water ice line A solar C/O and sub-solar metallicity in a hot Jupiter atmosphere

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:50.075860Z

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Observation 1529e54a-2b3d-4224-82b0-6f4f44dd37c9 · outbound

This paper cites SiO and a super-stellar C/O ratio in the atmosphere of the giant exoplanet WASP-121b.

The majority of hot Jupiters formed beyond the water ice line SiO and a super-stellar C/O ratio in the atmosphere of the giant exoplanet WASP-121b

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:50.152035Z

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Observation 28c953d5-331f-4a67-a199-7f484d731141 · outbound

This paper cites Atmospheres, Atmospheres! Do I Look Like I Care About Atmospheres? , year = 2021, month = oct, eid =.

The majority of hot Jupiters formed beyond the water ice line Atmospheres, Atmospheres! Do I Look Like I Care About Atmospheres? , year = 2021, month = oct, eid =

Reference 39

Resolution: verified exact; doi, observed 2026-08-02T00:09:21.000598Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 5a90ace4-23cd-4241-9e85-a4b0134fa85b · outbound

This paper cites , keywords =.

The majority of hot Jupiters formed beyond the water ice line , keywords =

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:50.336554Z

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Unavailable: canonical work link unavailable.

Observation a3af537c-3564-4775-9a22-045438ed9fa0 · outbound

This paper cites Disk and atmosphere composition of multi-planet systems.

The majority of hot Jupiters formed beyond the water ice line Disk and atmosphere composition of multi-planet systems

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:50.438009Z

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Observation f07f1bbe-9d2e-4afa-a627-ccfac0048889 · outbound

This paper cites Initial Conditions of Planet Formation: Lifetimes of Primordial Disks.

The majority of hot Jupiters formed beyond the water ice line Initial Conditions of Planet Formation: Lifetimes of Primordial Disks

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:50.606868Z

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Observation 8c13e14c-0291-49c8-98bc-131140aefeb0 · outbound

This paper cites Most planets might have more than 5 Myr of time to form.

The majority of hot Jupiters formed beyond the water ice line Most planets might have more than 5 Myr of time to form

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:50.716059Z

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Unavailable: canonical work link unavailable.

Observation 05c282ce-ca0f-4b95-b0f9-f818892c4431 · outbound

This paper cites Early Dynamical Instabilities in the Giant Planet Systems.

The majority of hot Jupiters formed beyond the water ice line Early Dynamical Instabilities in the Giant Planet Systems

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:50.810407Z

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Observation 90b47778-d5c2-4bd7-a073-bcd85d4268c8 · outbound

This paper cites Giants are bullies: how their growth influences systems of inner sub-Neptunes and super-Earths.

The majority of hot Jupiters formed beyond the water ice line Giants are bullies: how their growth influences systems of inner sub-Neptunes and super-Earths

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:50.867343Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 720c5463-f728-4264-8901-1452ed02398e · outbound

This paper cites , year = 2012, month = nov, volume =.

The majority of hot Jupiters formed beyond the water ice line , year = 2012, month = nov, volume =

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:50.976239Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 38ad83d5-a570-4d33-b406-561b1d8adef2 · outbound

This paper cites Tidal Evolution of Close-in Extra-Solar Planets.

The majority of hot Jupiters formed beyond the water ice line Tidal Evolution of Close-in Extra-Solar Planets

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:51.071887Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 06f7ee82-16f0-47c7-a733-6859af77ec40 · outbound

This paper cites , keywords =.

The majority of hot Jupiters formed beyond the water ice line , keywords =

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:51.176469Z

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Observation 9a0322c0-406c-4196-945d-5a1967fcf374 · outbound

This paper cites Hot Stars with Hot Jupiters Have High Obliquities.

The majority of hot Jupiters formed beyond the water ice line Hot Stars with Hot Jupiters Have High Obliquities

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:51.230514Z

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Observation d8b14861-ccd5-43eb-8162-c94adb5cc84f · outbound

This paper cites , keywords =.

The majority of hot Jupiters formed beyond the water ice line , keywords =

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:51.280374Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f220336b-1bbb-45c3-9245-49b3b8796577 · outbound

This paper cites Disk eccentricity and embedded planets.

The majority of hot Jupiters formed beyond the water ice line Disk eccentricity and embedded planets

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:51.284768Z

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Unavailable: canonical work link unavailable.

Observation e1983a65-5b06-4811-bdab-dddad617cf07 · outbound

This paper cites Highly inclined and eccentric massive planets I: Planet-disc interactions.

The majority of hot Jupiters formed beyond the water ice line Highly inclined and eccentric massive planets I: Planet-disc interactions

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:51.289124Z

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Observation d95c906f-0d2c-4216-bf8e-bf0cc0115d74 · outbound

This paper cites Dynamical Origin of Extrasolar Planet Eccentricity Distribution.

The majority of hot Jupiters formed beyond the water ice line Dynamical Origin of Extrasolar Planet Eccentricity Distribution

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:51.293492Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7549197d-c588-42e5-a2d6-26c17fc036bd · outbound

This paper cites Jupiter Analogues Orbit Stars with an Average Metallicity Close to that of the Sun.

The majority of hot Jupiters formed beyond the water ice line Jupiter Analogues Orbit Stars with an Average Metallicity Close to that of the Sun

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:51.302365Z

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Unavailable: canonical work link unavailable.

Observation 06d2e969-56a3-41f8-9576-ba8071120c40 · outbound

This paper cites Transport of CO in Protoplanetary Disks: Consequences of Pebble Formation, Settling, and Radial Drift.

The majority of hot Jupiters formed beyond the water ice line Transport of CO in Protoplanetary Disks: Consequences of Pebble Formation, Settling, and Radial Drift

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:51.306743Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8cdb5a5b-071d-4dc3-8844-375e703fb935 · outbound

This paper cites JWST ice band profiles reveal mixed ice compositions in the HH 48 NE disk.

The majority of hot Jupiters formed beyond the water ice line JWST ice band profiles reveal mixed ice compositions in the HH 48 NE disk

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:51.310981Z

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Observation 56a66368-d1b1-4261-9d5e-996bbbb027c0 · outbound

This paper cites , keywords =.

The majority of hot Jupiters formed beyond the water ice line , keywords =

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:51.315305Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 91a9513e-6151-4da4-afd0-f5ef220aa135 · outbound

This paper cites Close-in ice lines and the super-stellar C/O ratio in discs around very low-mass stars.

The majority of hot Jupiters formed beyond the water ice line Close-in ice lines and the super-stellar C/O ratio in discs around very low-mass stars

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:51.319357Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7205b37b-73ce-4775-ba56-e2541e064b5c · outbound

This paper cites , keywords =.

The majority of hot Jupiters formed beyond the water ice line , keywords =

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:51.323295Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 64e91c6a-c9d8-4bc0-9ad6-6e48929f497b · outbound

This paper cites Giant planets orbiting metal-rich stars show signatures of planet-planet interactions.

The majority of hot Jupiters formed beyond the water ice line Giant planets orbiting metal-rich stars show signatures of planet-planet interactions

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:51.327288Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Pith citing papers

Observation f780ca88-0c90-48f7-abb1-080f473ac042 · inbound

Spatial distribution of water ice in the protoplanetary silhouette disk d216-0939 cites this paper.

Spatial distribution of water ice in the protoplanetary silhouette disk d216-0939 The majority of hot Jupiters formed beyond the water ice line

Reference 121

Resolution: metadata mismatch; local_arxiv, observed 2026-08-06T16:19:19.390366Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.