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Paper Citation Record · LEDGER

Magnetic field strengths of hot giant exoplanets consistent with Solar System values

As of 6 August 2026, this Paper Citation Record lists 100 of 299 outbound references and 1 inbound Pith citation observation for arXiv:2606.22455.

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

pith.paper-citation-record.v1
2606.22455 v1

Coverage vector

measured 100 of 299 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-06-26T10:04:57.654930Z

measured 101 of 101 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-05T06:32:48.257954+00:00

measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-03T14:30:50.928843Z

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

100 of 299 outbound references displayed

  • verified exact68
  • verified fuzzy0
  • unresolved1
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch31

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 5e1ff909-c0a9-4056-a4f4-170f35aa07ce · outbound

This paper cites T., Roberge, W.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values T., Roberge, W

Reference 1

Resolution
metadata mismatch
doi, observed 2026-06-26T10:29:19.283020Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

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Observation ab02c2b8-e976-4026-9252-fa38c9e69d53 · outbound

This paper cites keywords =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values keywords =

Reference 2

Resolution
metadata mismatch
doi, observed 2026-06-26T10:09:18.815713Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:1289347ce21e3cc626375a09d053c902a06bb73ff2be890400b0b83ec91f09ec

Observation dc302d3d-e2c1-4e3c-a2ce-3f40c7d6cabc · outbound

This paper cites Astronomy & Astrophysics , author =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values Astronomy & Astrophysics , author =

Reference 3

Resolution
verified exact
doi, observed 2026-06-26T10:29:19.281408Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:de90d542d8a9a777b743b834e30388146d5524b53b35dbbb218f1ef9b9506bef

Observation be15ee07-2290-4941-a38c-04d486db244e · outbound

This paper cites KELT-25b and KELT-26b: A Hot Jupiter and a Substellar Companion Transiting Young A-stars Observed by TESS.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values KELT-25b and KELT-26b: A Hot Jupiter and a Substellar Companion Transiting Young A-stars Observed by TESS

Reference 4

Resolution
verified exact
arxiv_id, observed 2026-06-26T10:09:18.772388Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:10e8b54683c9b29b51cd8c8c7ed2a84fc3c6995f81cf29d8a166f24f4ef88c75

Observation 29e7e644-a051-4280-8443-9b03be2e9954 · outbound

This paper cites Astronomy & Astrophysics , author =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values Astronomy & Astrophysics , author =

Reference 5

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.791152Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:a5240d360dd874b0d29c8df145827f4de67c908de9c7745e1c9ed2cf87f8e8f8

Observation f6bfc8ff-64ca-467d-8201-0812a48bc33a · outbound

This paper cites D., Beatty, T.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values D., Beatty, T

Reference 6

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.789165Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:7ec06d9e839cdf6c528cdc22965539355806725b7e4214c8513434665e473212

Observation 38ac388b-a430-426b-b23d-c5a4283fdcc9 · outbound

This paper cites and Rainer, M.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values and Rainer, M

Reference 7

Resolution
metadata mismatch
doi, observed 2026-06-26T10:09:18.794995Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:c10874a192b583682f0a29c1cfe5b73ee981b2f8af64993c17bb8160fd718745

Observation 477e6e08-bb53-4cb9-ac12-11b43a3b1b21 · outbound

This paper cites 2025 , pages =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values 2025 , pages =

Reference 8

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.769972Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:9da102ddd445f7e56fda150756feedde395e9b657c73d414ea8d5f6684888c54

Observation b1d6f509-ad1e-41d2-9a8d-1c2d10a1734e · outbound

This paper cites and Wang, Ji and Asnodkar, Anusha Pai and Petz, Sydney and Duck, Alison and Strassmeier, Klaus G.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values and Wang, Ji and Asnodkar, Anusha Pai and Petz, Sydney and Duck, Alison and Strassmeier, Klaus G

Reference 9

Resolution
verified exact
arxiv_id, observed 2026-06-26T10:09:18.777175Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:f6b65d056068d2489e8f51fdfc0e7ae6343dc25ba4f4255811bcf97c0da555ff

Observation 2763222a-aee5-47f0-8334-9edf74b12441 · outbound

This paper cites The Astrophysical Journal , author =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values The Astrophysical Journal , author =

Reference 10

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.715997Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:d97b15ecaf3fc0ff62c08bb348b75630c50cf0ef2afd38fd9669bed9fdcb5a94

Observation fc1ee9c2-3e28-499b-8feb-b4ac72889e6d · outbound

This paper cites J., et al.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values J., et al

Reference 11

Resolution
metadata mismatch
doi, observed 2026-06-26T10:09:18.723288Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:fd98620e619a1b9771c7b0a25cf9ab8541e68ee1db27af425bc79407c9c57ecd

Observation 882571cc-1799-4896-a790-7960c68e9e85 · outbound

This paper cites Astronomy & Astrophysics , author =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values Astronomy & Astrophysics , author =

Reference 12

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.763517Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:57d2bd3cfd11c005f132e55c6e44321088225f6e3f82e2efb6fc97f995b135a5

Observation 600b0a96-37c2-448a-a28e-05aa6f2dbbed · outbound

This paper cites 2025, title Rossby Number Regime, Convection Suppression, and Dynamo-generated Magnetism in Inflated Hot Jupiters , , 990, 38, 10.3847/1538-4357/adf057.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values 2025, title Rossby Number Regime, Convection Suppression, and Dynamo-generated Magnetism in Inflated Hot Jupiters , , 990, 38, 10.3847/1538-4357/adf057

Reference 13

Resolution
metadata mismatch
doi, observed 2026-06-26T10:09:18.630916Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:0e8fed631c96437f8ed7c41d02a07b760b5d7d5432dff5eeb845ec622be383ad

Observation 8c08417d-6129-46d2-b4fe-deeabb2a30fb · outbound

This paper cites A., Allan, A., & Kubyshkina, D.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values A., Allan, A., & Kubyshkina, D

Reference 14

Resolution
metadata mismatch
doi, observed 2026-06-26T10:09:18.494067Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:088f70cb097fc9e467d60858a645865ed50f8822bd9b5efa1010ff351fab9b3a

Observation 5595e792-c2e3-4475-b883-0dcccddc9312 · outbound

This paper cites K., & Thorngren, D.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values K., & Thorngren, D

Reference 15

Resolution
metadata mismatch
doi, observed 2026-06-26T10:09:18.497654Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:e98925bf2f127091c359e603b39b3e1efe2491674514e242f0f7bebbf7c2dc59

Observation c97acfb6-8563-41f2-ae56-bb229973456c · outbound

This paper cites 2010, , 716, 1060, 10.1088/0004-637X/716/2/1060.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values 2010, , 716, 1060, 10.1088/0004-637X/716/2/1060

Reference 16

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.499568Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:9a8de54a8ebfd041e5dfce76311bf2c2ae042a90ae9ada78fd437f3185d194a6

Observation f59078d5-188e-41cd-9dbc-81b0267ad2b4 · outbound

This paper cites Super-Earths and Earth-like Exoplanets.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values Super-Earths and Earth-like Exoplanets

Reference 17

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verified exact
arxiv_id, observed 2026-06-26T10:09:18.392626Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:90f270fe7cc2877b1f8279a275a423c840061b542b93caac4ae98630add190cc

Observation b95253e3-2986-4832-980e-9162ee0092d0 · outbound

This paper cites and Graham, Matthew , month = oct, year =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values and Graham, Matthew , month = oct, year =

Reference 18

Resolution
verified exact
arxiv_id, observed 2026-06-26T10:09:18.429577Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:0c3e6b5e3e6d17774e827984be4d80708148058f98c233d492abd94a8af07fd6

Observation 18fdbcb3-eedf-4fd5-996f-a00784d33401 · outbound

This paper cites and Gonzalez-Gaitan, S.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values and Gonzalez-Gaitan, S

Reference 19

Resolution
verified exact
arxiv_id, observed 2026-06-26T10:09:18.446651Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:56347748052f27f9d4e4f0f3319d14d5e5e8090eabf65dcad3a91531ce71997a

Observation e753367d-d401-4ddd-887d-07623ec6647d · outbound

This paper cites Exoplanet climate characterization with transit asymmetries -- A comprehensive population study from the optical to the infrared.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values Exoplanet climate characterization with transit asymmetries -- A comprehensive population study from the optical to the infrared

Reference 20

Resolution
verified exact
local_arxiv, observed 2026-06-26T10:09:18.502181Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:12a50064e14860ee75afe93da4c8909e30da45339e31f1dfae4ffb429aec8652

Observation f7ba02ef-0fae-436b-b4b1-e545b4fd2486 · outbound

This paper cites and Boldt-Christmas, Linn , month = sep, year =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values and Boldt-Christmas, Linn , month = sep, year =

Reference 21

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arxiv_id, observed 2026-06-26T10:09:18.512050Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:a0bdfa9e4c9446587bc585061c46c73fbb6004d9e749063b0a33026fbec39d96

Observation 6fae6728-ebdf-4a39-9b59-98291074b930 · outbound

This paper cites 2015, ApJ, 806, 180, doi: 10.1088/0004-637X/806/2/180 Mars as an Exoplanet23.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values 2015, ApJ, 806, 180, doi: 10.1088/0004-637X/806/2/180 Mars as an Exoplanet23

Reference 22

Resolution
metadata mismatch
doi, observed 2026-06-26T10:09:18.516415Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:faaff55afed9ea704b9eeded4c9584ee05a0119c8f520a2c6c575d8f7c0642bb

Observation c243f039-03be-4571-834f-2aab1876e249 · outbound

This paper cites Goodis and Karalidi, Theodora and Bott, Kimberly M.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values Goodis and Karalidi, Theodora and Bott, Kimberly M

Reference 23

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arxiv_id, observed 2026-06-26T10:09:18.514707Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:db1d13f58cc4a242aefea141187370971be5821b136d724a735bc64c364af253

Observation a1164bf1-f0e5-4961-9ab3-881fcf1686bc · outbound

This paper cites An idealized general circulation model for the atmospheric circulation on the ice giants , url =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values An idealized general circulation model for the atmospheric circulation on the ice giants , url =

Reference 24

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verified exact
arxiv_id, observed 2026-06-26T10:09:18.509542Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:85b973aac4b48f6b5a31ba207a65372dda4964afb5a133abccc62c11f0646584

Observation 843cc7d0-fe59-4154-a5b4-ff00565db762 · outbound

This paper cites and R, Dhanush S.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values and R, Dhanush S

Reference 25

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verified exact
arxiv_id, observed 2026-06-26T10:09:18.506706Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:1becc442fb8819fe7429a4c8d25f73f0f2984f334f6c0b0f8ea963c4afddf34a

Observation e713d11c-6c4a-45fc-87ab-e7dfe69644c6 · outbound

This paper cites arXiv e-prints , author =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values arXiv e-prints , author =

Reference 26

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verified exact
arxiv_id, observed 2026-06-26T10:09:18.462635Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:5fe409cf5f36f38a74cf53aa746b67c27312950577a1984e0cdf0f056e877011

Observation 0ebeeab8-4fa2-45b5-b2bf-d0908812ee7d · outbound

This paper cites arXiv e-prints , author =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values arXiv e-prints , author =

Reference 27

Resolution
verified exact
arxiv_id, observed 2026-06-26T10:09:18.521734Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:44d7ad194825734e4e1b413e9fa6e826a3d0e45d4b56994777fd783d9691e033

Observation 7f7cf656-c95f-4a3d-b810-aa0f59165854 · outbound

This paper cites and Kopparla, Pushkar and Li, Jiazheng and Yung, Yuk L.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values and Kopparla, Pushkar and Li, Jiazheng and Yung, Yuk L

Reference 28

Resolution
verified exact
arxiv_id, observed 2026-06-26T10:09:18.644480Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:c39fbe1cab36201e62a2a74ff8240a0cb0868a99185276f430efca90f7eadaa5

Observation 8957077b-9ab3-439a-89ca-b0b4e2ce5f48 · outbound

This paper cites Estimating the magnetic field strength in hot Jupiters.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values Estimating the magnetic field strength in hot Jupiters

Reference 29

Resolution
metadata mismatch
local_arxiv, observed 2026-06-26T10:09:18.538690Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:be6770d47f5b39264dd6c503c9259561d85bcb49f3d3530d73846b77756a7bc6

Observation 50a9c503-883f-4159-b944-88a83cbc6e59 · outbound

This paper cites and G, Zhilkin A.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values and G, Zhilkin A

Reference 30

Resolution
verified exact
arxiv_id, observed 2026-06-26T10:09:18.542907Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:0a42c55380b54fe6f62e37ce597ad5de4fe5d9e6f5b0c8deec71e1074e75e73d

Observation 6fb5c8ce-5edb-44fc-86da-ca5256d343c8 · outbound

This paper cites Searching for GEMS: TOI-5916 b & TOI-6158 b are two Saturn-density planets orbiting M2 dwarfs.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values Searching for GEMS: TOI-5916 b & TOI-6158 b are two Saturn-density planets orbiting M2 dwarfs

Reference 31

Resolution
verified exact
arxiv_id, observed 2026-07-29T01:24:25.612560Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:8eed2d3619d5eea14cb7936c4a08b907b71630f36c9afedc987187b05c30457c

Observation 0109c8ff-0fd1-4705-9f96-fe72a2c8fe0d · outbound

This paper cites Simulating RISTRETTO: Proxima b detectability in reflected light.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values Simulating RISTRETTO: Proxima b detectability in reflected light

Reference 32

Resolution
verified exact
arxiv_id, observed 2026-06-26T10:09:18.484729Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:22cbc51a73560c90527b96c4aa4f8cb54376f1028bbc7500990cfe5a27410896

Observation 76e7855e-9cda-424c-8c79-e5e5d9b232f9 · outbound

This paper cites 2016 , pages =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values 2016 , pages =

Reference 33

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.540466Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:7797abf2cda3d6b9a1d9d6a28a2c489e20893a15ec7a1caaa25da8da7ba70b2b

Observation aa666c5d-debe-4eac-baf4-8fbf2ce479ca · outbound

This paper cites 2025, arXiv e-prints, arXiv:2509.09760, doi: 10.48550/arXiv.2509.09760.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values 2025, arXiv e-prints, arXiv:2509.09760, doi: 10.48550/arXiv.2509.09760

Reference 34

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metadata mismatch
arxiv_id, observed 2026-06-26T10:09:18.548002Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:c4ae6d66d353cb5f78b9ebcaaa6f994015efa73b9d910803a7bf0f91f8f5663b

Observation 086da35c-8b21-4fb9-912a-fe5541277ca4 · outbound

This paper cites an unresolved cited work.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values Unresolved cited work

Reference 35

Resolution
verified exact
arxiv_id, observed 2026-06-26T10:09:18.550439Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:0c45b357a7da7e4bfaa96bb280870e5c0e6ddda22ac5d7e85d3e57fed3b79e4c

Observation 736c016a-98cb-4a15-8b4b-9c58cc7b806b · outbound

This paper cites Nature , author =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values Nature , author =

Reference 36

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.494891Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:729456aa41ec48c516c7ef43e5fa3979154c008c61ff6fc422b95be2053122e7

Observation 61b3c7f8-9ebb-4801-b971-4e8db6f05629 · outbound

This paper cites 2010, Mechanisms of Jet Formation on the Giant Planets , 10.1175/2010JAS3492.1.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values 2010, Mechanisms of Jet Formation on the Giant Planets , 10.1175/2010JAS3492.1

Reference 37

Resolution
metadata mismatch
doi, observed 2026-06-26T10:09:18.552182Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:e4fd5e953fcb990ed3524c5a79adc4a3c86295f562866a5f895af66904320f75

Observation a4ff7a1d-fa99-4a2e-8daf-7eb62b42582a · outbound

This paper cites , keywords =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values , keywords =

Reference 38

Resolution
metadata mismatch
doi, observed 2026-06-26T10:09:18.554025Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:6766f1f50a4b333be773e5325cc2bb63aa33c6639b50cb513b40564b14e3d60e

Observation 3521a2ec-f3cb-4a26-83f9-a716d9686fc6 · outbound

This paper cites keywords =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values keywords =

Reference 39

Resolution
metadata mismatch
doi, observed 2026-06-26T10:09:18.496493Z

Source-reported events for the cited work

correction dated 2020-02-04. Source: crossref record 10.3847/2041-8213/ab6d6c->10.3847/2041-8213/ab43d0:correction, observed 2026-07-11T03:02:31.773195+00:00. This notice travels one citation hop only.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:e3f724b2db0e3e60a4a19fd52ddb210e0809b67c7596166ab412835b26831379

Observation ddbb7771-3f87-4e04-ab21-8134b84ce9a4 · outbound

This paper cites The Astrophysical Journal , author =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values The Astrophysical Journal , author =

Reference 40

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.322673Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:f339700388aacf998cb1598f52a9e1bbe7b1d8b9471acdef8a0e827cd85e5f3c

Observation f424cec1-547d-4299-ae40-ba73e59d7b89 · outbound

This paper cites On the radiative equilibrium of irradiated planetary atmospheres.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values On the radiative equilibrium of irradiated planetary atmospheres

Reference 41

Resolution
metadata mismatch
doi, observed 2026-06-26T10:09:18.482397Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:349660bb2b97a93b2df6579109e4079a2e51cb65a05f8b4e80db5dde29c977e3

Observation f5772bf8-6e96-4b46-b5f5-0892550db2d1 · outbound

This paper cites Astronomy & Astrophysics, Volume 692, id.A113, 19 pp.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values Astronomy & Astrophysics, Volume 692, id.A113, 19 pp

Reference 42

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.371176Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:d8ee15a060b0ecf909306ffd32ea78c859471878d1d970f81870ff1c0b342880

Observation d0be521d-9501-48cb-9028-9f5d9f77ba73 · outbound

This paper cites an unresolved cited work.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values Unresolved cited work

Reference 43

Resolution
unresolved
no resolver link, observed 2026-06-26T10:04:57.654930Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:1046167c1c56fc5415bd2c5b68c79b0949cd2c28031c3aea63fc95fc97f3364d

Observation 3064d82a-d3eb-4c21-8b7f-4dc13c51e614 · outbound

This paper cites The Astrophysical Journal, Volume 714, Issue 1, pp.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values The Astrophysical Journal, Volume 714, Issue 1, pp

Reference 44

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.501914Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:4d86437a0ffefbc30c4a572b109e620fc6d33e9e463165de2444e7ea43514153

Observation 952e22d1-b35f-4c60-a327-8b883d1254f5 · outbound

This paper cites Modelling magnetic star-planet interaction in the iconic M dwarfs Proxima Centauri, YZ Ceti and GJ 1151.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values Modelling magnetic star-planet interaction in the iconic M dwarfs Proxima Centauri, YZ Ceti and GJ 1151

Reference 45

Resolution
verified exact
arxiv_id, observed 2026-06-26T10:09:18.717953Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:78f221b51472840d5d7c901d7d4d7f15d472b1e9ef75cb1251b35f34d003115a

Observation 7c745d4b-9621-4753-94ca-8213e8c17f23 · outbound

This paper cites and Oklopčić, A.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values and Oklopčić, A

Reference 46

Resolution
verified exact
arxiv_id, observed 2026-06-26T10:09:18.562909Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:32bda4769319ba609beb67d6e48299700aad64b8b82039287bbfe87d40ff2a8c

Observation f7126ce4-691f-41d4-bed5-8736d2fdcda3 · outbound

This paper cites Astronomy and Astrophysics , author =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values Astronomy and Astrophysics , author =

Reference 47

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.313581Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:32e1c6a9eb675979768b5f532b65ec7e8eb96b0b67d39c7d700405fb810762f7

Observation d10c243b-f5e3-4dda-a1c5-c2c093a21cb1 · outbound

This paper cites Journal of Geophysical Research: Space Physics, Volume 129, Issue 5, article id.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values Journal of Geophysical Research: Space Physics, Volume 129, Issue 5, article id

Reference 48

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.557646Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:ef5ddb886f06a2d1e29b11b0a18527fdcdc389b6a8db5df8bdddc2ba34f60d07

Observation f36cb1f2-5e76-4143-a8b9-e5ad2730cf43 · outbound

This paper cites Nature Communications , year = 2023, month = oct, volume =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values Nature Communications , year = 2023, month = oct, volume =

Reference 49

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.564793Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:26214ce9ed545805880a6e26896c49e1004aa5ffafa709a71500da6aac08061c

Observation 8d7639be-d0c7-48d0-b197-25e6f2903fb6 · outbound

This paper cites and Lafrenière, David and Cowan, Nicolas B.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values and Lafrenière, David and Cowan, Nicolas B

Reference 50

Resolution
verified exact
arxiv_id, observed 2026-06-26T10:09:18.567372Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:4b2de5bf1c3351401eda5cfc959175f020744f5328b792c06a99bb8492266f31

Observation 8759f5cc-9132-4774-845f-d63a00fc4edc · outbound

This paper cites arXiv e-prints , keywords =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values arXiv e-prints , keywords =

Reference 51

Resolution
metadata mismatch
arxiv_id, observed 2026-06-26T10:09:18.511548Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:36704afefb28ad0512a915ab1ec3976a7a978cb9b10ed88c64b96de7be68d8f5

Observation c4db916a-3715-4396-8836-47855fce5615 · outbound

This paper cites Astronomy & Astrophysics , author =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values Astronomy & Astrophysics , author =

Reference 52

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.569395Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:bd16c9aabdea325c17c7d2ff99d1f863a873e0eb5a2e94396eeef9d872cfc1a5

Observation 11121e71-e165-43af-94da-7359f18d3a21 · outbound

This paper cites VLT/CRIRES+ observations of warm Neptune WASP-107 b: Challenges in detecting molecules with ground-based transmission spectroscopy of cooler and cloudy exoplanets.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values VLT/CRIRES+ observations of warm Neptune WASP-107 b: Challenges in detecting molecules with ground-based transmission spectroscopy of cooler and cloudy exoplanets

Reference 53

Resolution
verified exact
local_arxiv, observed 2026-06-26T10:09:18.572738Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:497f7f14e532b9ba6a858c2f8cb4d1885bcf96c9ee761eb9ce8a8b8b44bb993e

Observation 65e7609f-b136-4554-9f07-4ce5e8392c0a · outbound

This paper cites J., Beatty, T.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values J., Beatty, T

Reference 54

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.526279Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:6b921643033ff78c4443d0a6d2d2281d12caeec2d068bead19203ca3976cd7ef

Observation 3b734cf4-bf73-41ed-a5bb-8eb64fe646ee · outbound

This paper cites P., & Fortney, J.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values P., & Fortney, J

Reference 55

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.524745Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:8a3ceae25dd632973afad949f9cd8611432bc23d93f81d93753387882015ce39

Observation d1ef0cd4-98a7-4230-b8c4-93f7e63d568f · outbound

This paper cites , keywords =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values , keywords =

Reference 56

Resolution
metadata mismatch
doi, observed 2026-06-26T10:09:18.523194Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:253f9732628b62a08aae273740290ec09b9106d24660ba13608998d7377dbae0

Observation 789f04e8-86a7-46e2-bb38-9421807162d9 · outbound

This paper cites The Roasting Marshmallows Program with IGRINS on Gemini South II -- WASP-121 b has super-stellar C/O and refractory-to-volatile ratios.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values The Roasting Marshmallows Program with IGRINS on Gemini South II -- WASP-121 b has super-stellar C/O and refractory-to-volatile ratios

Reference 57

Resolution
verified exact
arxiv_id, observed 2026-06-26T10:09:18.577157Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:9ece69d99559d878a9c07a3c056920cc5b619694981204ad7518372cf704914a

Observation 12b503f4-a5f4-42c3-afdc-ee7f2d10c2c0 · outbound

This paper cites , keywords =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values , keywords =

Reference 58

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.531613Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:7738a84bfe460a811193fb973ee86898978484c07b644bc45dba84a643d68b60

Observation 6d000bf2-599b-4e75-8033-a15f418ebcd2 · outbound

This paper cites Time Resolved Absorption of Six Chemical Species With MAROON-X Points to Strong Drag in the Ultra Hot Jupiter TOI-1518 b.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values Time Resolved Absorption of Six Chemical Species With MAROON-X Points to Strong Drag in the Ultra Hot Jupiter TOI-1518 b

Reference 59

Resolution
verified exact
arxiv_id, observed 2026-06-26T10:09:18.579911Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:83a8e1e78d52eaf6b3e44838a6f53f63e293b6c7a8ce6c829ade4df88077bcc5

Observation af00e1ab-ccac-4534-8356-69d758b2210a · outbound

This paper cites Astronomy and Astrophysics , author =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values Astronomy and Astrophysics , author =

Reference 60

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.581557Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:f33ebdc2d69330a3f0d042ce7609ae490fbd21a07dd5a4d816d85d8e33e85844

Observation 7049af32-adb9-4cab-8c3c-84029d590423 · outbound

This paper cites and Polvani, Lorenzo M.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values and Polvani, Lorenzo M

Reference 61

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.535110Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:9732ae22253a52f48020c51c56301ccae391b23a82349621e57a00f455e83a92

Observation 9d4e289f-e2e7-4fe2-8621-5c77b310c244 · outbound

This paper cites Monthly Notices of the Royal Astronomical Society , volume =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values Monthly Notices of the Royal Astronomical Society , volume =

Reference 62

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.281981Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:db74a8769a317b8e00037f80345c351c2ecd39ba3e2c4589e7103bf202abcd50

Observation 315f8f3b-a321-45ff-ba7e-81b7626c8f80 · outbound

This paper cites The Astronomical Journal , author =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values The Astronomical Journal , author =

Reference 63

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.283031Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:fd399d75e45fa0b79bfcc3bc471890fdfad675d93004a9582c6947e4e5ac7d71

Observation 1dc3f0cf-2155-4c65-917e-1c22f2974cba · outbound

This paper cites The Astrophysical Journal , author =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values The Astrophysical Journal , author =

Reference 64

Resolution
metadata mismatch
doi, observed 2026-06-26T10:09:18.588020Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:88727ee28e809821a76bbbc64e79b030b753ab2441f196f6cca61ebf39a2bfd0

Observation b4a6ce00-e3b3-45e0-a673-cc551a6fc256 · outbound

This paper cites McKinney.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values McKinney

Reference 65

Resolution
metadata mismatch
arxiv_id, observed 2026-06-26T10:09:18.590723Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:866cd3809ac63ef076b5b7194bb6a486b7d37cb0f618d12fbc82390b58e872a9

Observation cd6f135e-71b6-415f-8abf-01de181f28ef · outbound

This paper cites R., Brogi, M., Bean, J.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values R., Brogi, M., Bean, J

Reference 66

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.540034Z

Source-reported events for the cited work

correction dated 2021-12-15. Source: crossref record 10.1038/s41586-021-04192-w->10.1038/s41586-021-03912-6:correction, observed 2026-07-11T03:04:06.993112+00:00. This notice travels one citation hop only.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:4d812490a7c7820c4f1e8bb6fbc894790d88846e45855b39219ef17f6b2f9f61

Observation 481a8ccc-7ad6-4c6a-926e-a0d6d4a280d9 · outbound

This paper cites Retrieving wind properties from the ultra-hot dayside of WASP-189b with CRIRES$^+$.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values Retrieving wind properties from the ultra-hot dayside of WASP-189b with CRIRES$^+$

Reference 67

Resolution
verified exact
arxiv_id, observed 2026-06-26T10:09:18.542523Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:19a5e553700c10dc8a9786a90208084fcc7bab3da6b0a4af06f6c4f3af96bb1f

Observation b8316632-7bd3-4286-a4f0-c7500b36937a · outbound

This paper cites an unresolved cited work.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values Unresolved cited work

Reference 68

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.283941Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:86d15bd893589fc362ac51e5ee14d8f5479cdb7c020bdbef7cbf493cb18a820d

Observation 84d686c2-40b9-478b-b643-b88eae26022f · outbound

This paper cites , keywords =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values , keywords =

Reference 69

Resolution
metadata mismatch
doi, observed 2026-06-26T10:09:18.536922Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:304237c380f637a2325940d071091251dc1b5850f6dbdd7b29c79043c9fb5a91

Observation 1eb309aa-be73-4221-b111-728ecc32ca89 · outbound

This paper cites R., Barkaoui, K., et al.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values R., Barkaoui, K., et al

Reference 70

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.545825Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:a03d1948501c336b27b978d82b9674c1251093c12f7128babd29e334ef5adf6f

Observation 286f8be0-3687-4d01-b3a4-90594a608a86 · outbound

This paper cites J., Challener, R.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values J., Challener, R

Reference 71

Resolution
metadata mismatch
doi, observed 2026-06-26T10:09:18.544253Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:534694ba23852f508f958d8fcb49e40151f07f771db0a8963703222a7ff9f8c4

Observation 9228c671-4e64-436e-935a-6b16247a6c61 · outbound

This paper cites The Astronomical Journal , author =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values The Astronomical Journal , author =

Reference 72

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.549096Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:b681c87d102b2675421c5947680b76f7ddaf1f14310fa204397d15b0193bb2f7

Observation bec468ab-b23a-453c-a394-0df7f0ec2d9a · outbound

This paper cites The Astronomical Journal , author =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values The Astronomical Journal , author =

Reference 73

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.605842Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:b5f27de3d6c308ab120dff9405cbbd460ed79980eb97d2eea9f532d48668a8c0

Observation 675afdbd-8c86-4d23-99d3-b5fece27ffe3 · outbound

This paper cites Space Science Reviews, v.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values Space Science Reviews, v

Reference 74

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.608459Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:a9b278b978b70c5abdd3f4698d84fc9ce26e29d03c04fbcc5e3db4865a93a738

Observation c763bdbf-c4ae-40c2-bca2-af5504bf2b73 · outbound

This paper cites keywords =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values keywords =

Reference 75

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.538513Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:083367bc370115eb29e6d85ca3f8645a70d7a7385243cefd1fd385f04109cf3e

Observation 078ba61b-b28c-4b3b-aa2b-e36f68302829 · outbound

This paper cites , keywords =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values , keywords =

Reference 76

Resolution
metadata mismatch
doi, observed 2026-06-26T10:09:18.552346Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:78e3a8b32032eae3ce0fe584dfb376348beeaaaa6d3bcb7280a75afdc50d43c7

Observation bb044d39-2f63-4540-9202-efaf543ab43f · outbound

This paper cites and Todorov, Kamen O.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values and Todorov, Kamen O

Reference 77

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.550640Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:aa205c23674f70f8353223ea2bf64b334afbe39438a2285da3424c6ee2b23c6e

Observation 9aafca27-2047-4930-af32-281f8eeb2ea8 · outbound

This paper cites Magnetic.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values Magnetic

Reference 79

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.612703Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:78bff5259ec7bfb207a3570cb94fb80ad2c975bfebe15b6a6e049b756d613736

Observation fd6bc98b-9af4-4451-a9bf-b5e9ca8af7a7 · outbound

This paper cites and Cook, Neil J.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values and Cook, Neil J

Reference 80

Resolution
verified exact
arxiv_id, observed 2026-06-26T10:09:18.556310Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:ea432848251ed7c8694deee1454e84c210751d1913077ec61a187c460b3f12cc

Observation 64175416-ccc1-4496-a7a7-877ed484967a · outbound

This paper cites 2018 , pages =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values 2018 , pages =

Reference 81

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.614424Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:22c17c94485f745194748da283e97eabb9ad0380c13295aca4c5b73f53f29be0

Observation ad9f1fd4-f3bd-4e58-8beb-66bbe789b570 · outbound

This paper cites Astronomy and Astrophysics , author =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values Astronomy and Astrophysics , author =

Reference 82

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.616671Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:71c771b956477140b4352d716fa407da8281d04cf30ac18aee581a1bdc1a7775

Observation 6eeb3d2b-9c3b-4c65-bf1a-3dfc53503e3f · outbound

This paper cites The Astronomical Journal , author =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values The Astronomical Journal , author =

Reference 83

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.557858Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:58b2a59cd478f6c5f224bfaa8335ac09573bfd502b9992a71edb5d699b4e7dd5

Observation c9191d24-ddbf-45ba-8c71-bab561a2cf18 · outbound

This paper cites Astronomy and Astrophysics , author =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values Astronomy and Astrophysics , author =

Reference 84

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.561569Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:1d4e5b0a27f67280d636d55570d0b2fc7e8b1caa8e8ca2a37d5ba11b5bf610ea

Observation 3615c624-ac6b-4135-b6cd-8195d4a4fc98 · outbound

This paper cites B., Jaziri, A.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values B., Jaziri, A

Reference 85

Resolution
metadata mismatch
doi, observed 2026-06-26T10:09:18.618869Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:edfbd3449b9405bc418514b1d14ebe8d2cd555bb4875d5efaf968028c48e72a7

Observation 43f7df81-a30f-4444-b20f-258fcd912fe0 · outbound

This paper cites keywords =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values keywords =

Reference 86

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.623030Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:a8d61739b500e281f7e1fb95b51055d831256c39ab14078d91218a309d28b6ee

Observation c903e0fe-e5bb-4cbe-8e04-7b15db113e7b · outbound

This paper cites Overcast mornings and clear evenings in hot Jupiter exoplanet atmospheres.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values Overcast mornings and clear evenings in hot Jupiter exoplanet atmospheres

Reference 87

Resolution
metadata mismatch
arxiv_id, observed 2026-06-26T10:09:18.269473Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:ea6ea13b8e88733928a22ce54b4a01e6452b04bd235ad167db350913e8aa88ed

Observation e9e03829-6199-49d8-9ae9-dec38c0b772e · outbound

This paper cites A Precise Metallicity and Carbon-to-Oxygen Ratio for a Warm Giant Exoplanet from its Panchromatic JWST Emission Spectrum.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values A Precise Metallicity and Carbon-to-Oxygen Ratio for a Warm Giant Exoplanet from its Panchromatic JWST Emission Spectrum

Reference 88

Resolution
metadata mismatch
arxiv_id, observed 2026-06-26T10:09:18.625985Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:8b546020577ddb606d6235c2108ed3040d6e00748b2b3cf7d8659c36b92cacb4

Observation 883944e2-a031-4845-b94b-cfa53f80c403 · outbound

This paper cites The Astrophysical Journal , author =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values The Astrophysical Journal , author =

Reference 89

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.628336Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:6d0aa34679e361c34beb4ff86f6095e5249f94cb8a90436dba26ec94325846cd

Observation f440c04a-cb98-45dc-80a5-ef10e9f289c8 · outbound

This paper cites R., Thorngren, D., Morley, C.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values R., Thorngren, D., Morley, C

Reference 90

Resolution
metadata mismatch
doi, observed 2026-06-26T10:09:18.236322Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:8e713d149d713bf9bc3ffe6b3a03ca7018d2fbe25400e1e717e4c7dbd6112acf

Observation fe00fef0-536b-40e0-a8b0-fe916e863a03 · outbound

This paper cites keywords =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values keywords =

Reference 91

Resolution
metadata mismatch
doi, observed 2026-06-26T10:09:18.574083Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:c07ce3ff79c658e4afa52045dc0393c37bdd0153547ef6a1de34039aed9a3d3a

Observation 59a1b040-fcf8-41ba-bfca-db1fd48a725e · outbound

This paper cites keywords =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values keywords =

Reference 92

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.575758Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:79d5dde3bbe306e6aa64ad230d977fd51406bc286d5189f458c20169a2aca508

Observation f2188122-57d8-4087-af19-ca25e7484f55 · outbound

This paper cites A., Dai, F., Howard, A.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values A., Dai, F., Howard, A

Reference 93

Resolution
metadata mismatch
doi, observed 2026-06-26T10:09:18.262477Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:52570493bf2af135a972f34a6e01f52cfd9d8c82bada2837a22abf3c11baa3f5

Observation 6f9c0d39-c309-4111-abd1-ed0b1c7805fd · outbound

This paper cites Astronomy and Astrophysics , author =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values Astronomy and Astrophysics , author =

Reference 94

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.577276Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:563fd2a29eaf88eb7bc28e2278b47e7826982d4bd1e65f6058c2e8ce853a987b

Observation f0108330-900e-4ab6-9015-b9a3c7d18383 · outbound

This paper cites 2024 , pages =.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values 2024 , pages =

Reference 95

Resolution
verified exact
doi, observed 2026-06-26T10:09:18.578911Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:976155d5123b1a929194aa2a84e1c2c9b2ac084c0847d9a2e48c4add5e27d337

Observation 956fea45-c202-4d67-8116-8393fe3c5690 · outbound

This paper cites 2024, ApJ, 972, 159, doi: 10.3847/1538-4357/ad5ffb.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values 2024, ApJ, 972, 159, doi: 10.3847/1538-4357/ad5ffb

Reference 96

Resolution
metadata mismatch
doi, observed 2026-06-26T10:09:18.648208Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:593f3d6fd05e07107a8a5e85218716c5ae74072d15720ad50e166ae0cee4c73a

Observation f93af60d-5462-42ad-bcf7-52ef2e9f07af · outbound

This paper cites M., et al., 2024a, @doi [Nature Astronomy] 10.1038/s41550-024-02367-9 , https://ui.adsabs.harvard.edu/abs/2024NatAs...8.1562M 8.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values M., et al., 2024a, @doi [Nature Astronomy] 10.1038/s41550-024-02367-9 , https://ui.adsabs.harvard.edu/abs/2024NatAs...8.1562M 8

Reference 97

Resolution
metadata mismatch
doi, observed 2026-06-26T10:09:18.650422Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:3548750ace4221e23d4ab88813b60ec466e980c6e82d5ce54951849bf0816c3a

Observation 1e44adb4-421d-4205-ba64-9b5ba7f0f27c · outbound

This paper cites 2025, ApJ, 985, 87, doi: 10.3847/1538-4357/adccc4.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values 2025, ApJ, 985, 87, doi: 10.3847/1538-4357/adccc4

Reference 98

Resolution
metadata mismatch
doi, observed 2026-06-26T10:09:18.572421Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:99144bb6a9deca11b2321a19cc9f64af79fd8ebb4e1db0f7bca18e51ab3da843

Observation 43d31379-0061-438d-b77c-96d0d4d05ec8 · outbound

This paper cites Continuous helium absorption from the leading and trailing tails of WASP-107b.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values Continuous helium absorption from the leading and trailing tails of WASP-107b

Reference 99

Resolution
metadata mismatch
arxiv_id, observed 2026-06-26T10:09:18.653556Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:c5e54246590aadc7ba1047888c822bcf1081be6573d554833aecdb677113caec

Observation 0529404d-e0e8-49ea-924b-7d150e071d58 · outbound

This paper cites Tempests in the Troposphere: Mapping the Impact of Giant Storms on Jupiter's Deep Atmosphere.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values Tempests in the Troposphere: Mapping the Impact of Giant Storms on Jupiter's Deep Atmosphere

Reference 100

Resolution
verified exact
arxiv_id, observed 2026-06-26T10:09:18.656852Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:2c5a05620a649e9366107e27c5d2abbad2229a82705dc40c0496aac886e53d15

Observation 06bcc4c3-0d0e-4e6b-86dc-614ddc721223 · outbound

This paper cites Internal Heat and Energy Imbalance of Uranus.

Magnetic field strengths of hot giant exoplanets consistent with Solar System values Internal Heat and Energy Imbalance of Uranus

Reference 101

Resolution
verified exact
arxiv_id, observed 2026-06-26T10:09:18.218452Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-06-26T10:04:57.654930Z digest=sha256:edc5d2a869f4334ad8c293cea21d8a136071219c7c1bcc027d0990bfed061cbc

Pith citing papers

Observation 8b113406-96b4-4f27-bacd-6523c170ae50 · inbound

A Physically Driven Parameterisation of Multidimensional Atmospheres: Application to the JWST Phase Curve of WASP-121b cites this paper.

A Physically Driven Parameterisation of Multidimensional Atmospheres: Application to the JWST Phase Curve of WASP-121b Magnetic field strengths of hot giant exoplanets consistent with Solar System values

Reference 155

Resolution
unresolved
no resolver link, observed 2026-08-03T14:30:50.928843Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-03T14:30:50.928843Z digest=sha256:13ed9eb85a4d9054679e39c2a1e5722a2b3edafc59f71e66cb5da6ef2abdc239