Paper Citation Record · LEDGER

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars

As of 23 August 2026, this Paper Citation Record lists 100 of 170 outbound references and 4 inbound Pith citation observations for arXiv:2412.04438.

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

pith.paper-citation-record.v1
2412.04438 v3

Coverage vector

measured 100 of 170 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-11T21:30:15.239450Z

measured 104 of 104 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-23T06:30:58.430688+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T11:40:37.492574Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-10T05:30:23.456663Z

Reference resolution

100 of 170 outbound references displayed

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verified fuzzy0
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External citation measurements

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pith, observed 2026-08-10T05:30:23.456663Z

Outbound references

Observation 072bf7be-b7b0-4f5c-bb1b-7f94f6596488 · outbound

This paper cites , " * write output.state after.block = add.period write newline.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars , " * write output.state after.block = add.period write newline

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.809402Z

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Observation de2d2a93-30f0-43c0-b3c5-10ae5f867344 · outbound

This paper cites write newline.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars write newline

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.813878Z

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Observation 0750cffc-56dc-4f9d-9917-51eddabc3252 · outbound

This paper cites * d7nnWR|AZw J _ .f pɓ_ nnm I'9ϥw 7^4rDؽm4lb KvCJNn ^ ]- k<pR E s xR\\ c i X S> x Bn[j|sݯ _r|XZ.DWiB # j4|z RFv + ^=Ʋ VPٮ@ t ;Aې +l\7AWǻ Aٮ@ t ;AW|D?v fݗ 4AW0 ̫ ].UWI:h.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars * d7nnWR|AZw J _ .f pɓ_ nnm I'9ϥw 7^4rDؽm4lb KvCJNn ^ ]- k<pR E s xR\\ c i X S> x Bn[j|sݯ _r|XZ.DWiB # j4|z RFv + ^=Ʋ VPٮ@ t ;Aې +l\7AWǻ Aٮ@ t ;AW|D?v fݗ 4AW0 ̫ ].UWI:h

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.819482Z

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Observation 066169a5-cb1e-4cfb-b1c8-b95a75affc24 · outbound

This paper cites S., & Snellen , I.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars S., & Snellen , I

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.829800Z

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Observation 6e08d6e6-f5bd-4eb4-a6a3-63ecc6b43f94 · outbound

This paper cites N., Marcy , G.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars N., Marcy , G

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.833706Z

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Observation 92c14105-5597-4ca3-910b-59fc54780fb0 · outbound

This paper cites N., Johnson , J.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars N., Johnson , J

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.837612Z

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Observation 5ef416eb-6e8a-4c7a-81f4-9f003bb631dd · outbound

This paper cites H., Dawson , R.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars H., Dawson , R

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.842161Z

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Observation ca1e8e6c-754a-459d-9fe1-ace3ae6db732 · outbound

This paper cites R., Winn , J.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars R., Winn , J

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.846738Z

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Observation caae2789-4b44-4e6b-934a-ba6c3d8a95d0 · outbound

This paper cites 2019, , 885, L29, 10.3847/2041-8213/ab5062.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2019, , 885, L29, 10.3847/2041-8213/ab5062

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.851541Z

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Observation b5d178c1-0d49-4d62-bc6c-64d6596075d6 · outbound

This paper cites 2012, , 751, 119, 10.1088/0004-637X/751/2/119.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2012, , 751, 119, 10.1088/0004-637X/751/2/119

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.855916Z

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Observation fdfbd314-6ec1-4a65-9f52-6aa46be31ae4 · outbound

This paper cites 2020, , 496, 1922, 10.1093/mnras/staa1522.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2020, , 496, 1922, 10.1093/mnras/staa1522

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.860481Z

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Observation bc2b1a5e-856d-42f8-9e08-ac27461b6819 · outbound

This paper cites 2021, , 916, L2, 10.3847/2041-8213/ac0f83.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2021, , 916, L2, 10.3847/2041-8213/ac0f83

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.865635Z

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Observation 384b41b0-6966-4ccb-9fc7-f3b2b470e8ca · outbound

This paper cites Y., Krushinsky , V.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars Y., Krushinsky , V

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.870063Z

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Observation ba90ecd0-124f-466e-9767-98d6a36abc91 · outbound

This paper cites 2013, , 428, 182, 10.1093/mnras/sts019.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2013, , 428, 182, 10.1093/mnras/sts019

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.874213Z

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Observation 3d5eb0c8-83ae-4d82-be99-fa0c027396cb · outbound

This paper cites 2019, , 486, 2075, 10.1093/mnras/stz549.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2019, , 486, 2075, 10.1093/mnras/stz549

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.878472Z

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Observation 2ff633fe-883b-4b39-9a63-cb3bf9df7544 · outbound

This paper cites 2014, , 569, A111, 10.1051/0004-6361/201423945.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2014, , 569, A111, 10.1051/0004-6361/201423945

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.882841Z

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Observation f17366f3-2909-4c63-b1f2-1e93b66bb76d · outbound

This paper cites S., Desidera , S., Benatti , S., et al.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars S., Desidera , S., Benatti , S., et al

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.888470Z

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Observation fcd51dad-a21e-490c-ae8e-5d6101b49c93 · outbound

This paper cites J., Koch , D.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars J., Koch , D

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.892924Z

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Observation a0e33969-2490-4e7a-a948-c8db3e289978 · outbound

This paper cites 2018, , 553, 477, 10.1038/nature24677.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2018, , 553, 477, 10.1038/nature24677

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.896842Z

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Observation a9c0847e-46c7-4948-93b3-2e9c66faa2fa · outbound

This paper cites A Small Brown Dwarf in an Aligned Orbit around a Young, Fully-Convective M Star.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars A Small Brown Dwarf in an Aligned Orbit around a Young, Fully-Convective M Star

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.900723Z

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Observation 675d4909-0b51-440c-b12b-2d457e6aeff6 · outbound

This paper cites B., Matsumura , S., & Rasio , F.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars B., Matsumura , S., & Rasio , F

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.905456Z

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Observation f3b1098c-03c2-452e-871d-6d21f8db5ed0 · outbound

This paper cites 2016, , 823, 102, 10.3847/0004-637X/823/2/102.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2016, , 823, 102, 10.3847/0004-637X/823/2/102

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.909602Z

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Observation bb0343cc-63cb-425f-a4c8-f97ee267d756 · outbound

This paper cites 2011, , 529, A75, 10.1051/0004-6361/201116451.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2011, , 529, A75, 10.1051/0004-6361/201116451

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.914355Z

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Observation 13fd1195-cdfa-4e57-aa48-6247c3cd21b6 · outbound

This paper cites A., Miller , G.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars A., Miller , G

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.918653Z

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Observation 41e54ecf-24f4-4f06-ad9e-f12de9a6ee9b · outbound

This paper cites 2012, in Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series, Vol.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2012, in Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series, Vol

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.922734Z

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Observation 3807ee6f-9048-43b5-a3e3-cf39eb240617 · outbound

This paper cites 2014, in Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series, Vol.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2014, in Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series, Vol

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.927982Z

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Observation c254e7ca-cbd1-4413-bb50-316e9d82b826 · outbound

This paper cites M., Skrutskie , M.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars M., Skrutskie , M

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.932556Z

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Observation 310a75ad-334e-427f-90ad-0d63722c97a7 · outbound

This paper cites M., Wright , E.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars M., Wright , E

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.936695Z

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Observation 674a0813-f0c4-4120-91e2-734b175a0d0f · outbound

This paper cites an unresolved cited work.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars Unresolved cited work

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.941061Z

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Observation cf3d35dc-269d-4699-80c1-81bc5d910e11 · outbound

This paper cites 2023, , 165, 33, 10.3847/1538-3881/aca327.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2023, , 165, 33, 10.3847/1538-3881/aca327

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.946412Z

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Observation a4073008-df80-4f1f-b069-12a68a56acc4 · outbound

This paper cites 2024, , 168, 239, 10.3847/1538-3881/ad83a6.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2024, , 168, 239, 10.3847/1538-3881/ad83a6

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.949863Z

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Observation b3206c08-00c9-4bb0-8fee-fae252db1651 · outbound

This paper cites an unresolved cited work.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars Unresolved cited work

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.953377Z

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Observation 81c58754-6c52-4eb1-9206-41ab7620979f · outbound

This paper cites X., Zhou , G., et al.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars X., Zhou , G., et al

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.957410Z

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Observation 6050576b-2e11-4e7b-9145-4c9f96945411 · outbound

This paper cites TOI-1859b: A 64-Day Warm Jupiter on an Eccentric and Misaligned Orbit.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars TOI-1859b: A 64-Day Warm Jupiter on an Eccentric and Misaligned Orbit

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.960838Z

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Observation 1f31e30d-3bf8-45b3-89a6-e4f6af620bfd · outbound

This paper cites Origins of Super Jupiters: TOI-2145b Has a Moderately Eccentric and Nearly Aligned Orbit.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars Origins of Super Jupiters: TOI-2145b Has a Moderately Eccentric and Nearly Aligned Orbit

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.965693Z

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Observation 10133bb0-7489-4a65-a74e-d9f23658ff14 · outbound

This paper cites 2016, , 222, 8, 10.3847/0067-0049/222/1/8.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2016, , 222, 8, 10.3847/0067-0049/222/1/8

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.970264Z

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Observation 76656367-b07b-4e8d-a713-51d3e2ab15ac · outbound

This paper cites P., Davies , G.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars P., Davies , G

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.974395Z

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Observation f9dd31ae-be7e-4206-98c7-22ad6bf93cfc · outbound

This paper cites The First Spin-Orbit Obliquity of an M dwarf/brown dwarf System: An eccentric and aligned TOI-2119 b.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars The First Spin-Orbit Obliquity of an M dwarf/brown dwarf System: An eccentric and aligned TOI-2119 b

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.979555Z

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Observation 6867f610-8689-4a3f-bb06-4261bbc32555 · outbound

This paper cites 2017, EXOFASTv2: Generalized publication-quality exoplanet modeling code.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2017, EXOFASTv2: Generalized publication-quality exoplanet modeling code

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.983928Z

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Unavailable: canonical work link unavailable.

Observation 941cbf34-2b5f-4a17-8709-737df24c0427 · outbound

This paper cites EXOFASTv2: A public, generalized, publication-quality exoplanet modeling code.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars EXOFASTv2: A public, generalized, publication-quality exoplanet modeling code

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.987679Z

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Observation b890e3f3-3a14-4098-ac8b-117e139e9d24 · outbound

This paper cites 1997, ESA Special Publication, Vol.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 1997, ESA Special Publication, Vol

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.992015Z

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Observation d5b4a077-c717-4d5d-8bbd-a0ff83d233a0 · outbound

This paper cites I., Brahm , R., Petrovich , C., et al.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars I., Brahm , R., Petrovich , C., et al

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:14.996947Z

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Observation 02b2494b-332b-4609-8c33-2cf4669c19c3 · outbound

This paper cites 2016, , 128, 115001, 10.1088/1538-3873/128/969/115001.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2016, , 128, 115001, 10.1088/1538-3873/128/969/115001

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.001224Z

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Observation 0c97425e-d347-4c61-9094-b61fa4b845c2 · outbound

This paper cites 2007, , 669, 1298, 10.1086/521702.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2007, , 669, 1298, 10.1086/521702

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.005545Z

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Observation 05777ec8-eeb0-40d9-8724-53377c145fae · outbound

This paper cites 2024, , 168, 145, 10.3847/1538-3881/ad6b7f.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2024, , 168, 145, 10.3847/1538-3881/ad6b7f

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.010464Z

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Observation d8a9e19f-451c-4eaa-b6ea-2c221fec8685 · outbound

This paper cites M., & Kraus , A.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars M., & Kraus , A

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.014682Z

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Observation 11d3b994-6f59-4980-ae06-f500565b7382 · outbound

This paper cites J., Petigura , E.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars J., Petigura , E

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.019316Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d1847f83-a2cf-4f5e-9c6c-c22e15081f76 · outbound

This paper cites an unresolved cited work.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars Unresolved cited work

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.022889Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3a6a59c4-2105-4b7e-953f-4ef6875c8c24 · outbound

This paper cites 2018, , 616, A1, 10.1051/0004-6361/201833051.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2018, , 616, A1, 10.1051/0004-6361/201833051

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.026749Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4500f89f-9c38-4e05-853a-3097976ec3d3 · outbound

This paper cites an unresolved cited work.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars Unresolved cited work

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.031102Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e60089fe-a458-44ee-86ed-e6fc90941298 · outbound

This paper cites 2014, , 437, 2909, 10.1093/mnras/stt2108.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2014, , 437, 2909, 10.1093/mnras/stt2108

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.036298Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2b136405-b957-47a4-a84d-c6836aef9511 · outbound

This paper cites X., Dai , F., et al.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars X., Dai , F., et al

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.040626Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cd411067-1081-48f8-bcf8-3b76635d947a · outbound

This paper cites 2017, Astronomische Nachrichten, 338, 35, 10.1002/asna.201613208.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2017, Astronomische Nachrichten, 338, 35, 10.1002/asna.201613208

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.044825Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2db89bb3-1cfd-4367-8760-3531949479c4 · outbound

This paper cites an unresolved cited work.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars Unresolved cited work

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.049905Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d69f19d5-cbc2-4468-b5fa-13715b71f1bf · outbound

This paper cites J., et al.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars J., et al

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.054611Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 852162d2-cc83-4c72-989f-80b6fc81f2bc · outbound

This paper cites 2019, , 487, 681, 10.1093/mnras/stz1322.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2019, , 487, 681, 10.1093/mnras/stz1322

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.059760Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ca7baf87-631e-40a5-ab59-6a243b9d18e0 · outbound

This paper cites 2004, , 42, 549, 10.1146/annurev.astro.42.053102.134004.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2004, , 42, 549, 10.1146/annurev.astro.42.053102.134004

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.063988Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 82ee7264-d7cd-4f3d-8620-a61580e1be4e · outbound

This paper cites V., Dai , F., & Wang , S.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars V., Dai , F., & Wang , S

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.068037Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e21d09f1-f34f-49a0-8919-bb5c36704df0 · outbound

This paper cites V., & Wang , S.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars V., & Wang , S

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.072388Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6e4b133e-9326-4c3b-a1cd-e20b80f12721 · outbound

This paper cites O., & Corbally , C.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars O., & Corbally , C

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.076505Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b697268f-ab85-4c55-a2bb-6e4ad67d7043 · outbound

This paper cites F., Millholland , S.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars F., Millholland , S

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.080659Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3af21714-1fa9-4b51-98a7-8f06e344d371 · outbound

This paper cites 2008, , 486, 951, 10.1051/0004-6361:200809724.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2008, , 486, 951, 10.1051/0004-6361:200809724

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.084721Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 94b416e5-a201-4116-b36b-b2257acde8f3 · outbound

This paper cites R., Millman, K.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars R., Millman, K

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.088804Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4cb05e74-5cbe-4447-a2dd-5f9f28d5d614 · outbound

This paper cites 2008, , 488, 763, 10.1051/0004-6361:200810056.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2008, , 488, 763, 10.1051/0004-6361:200810056

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.092803Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation adb75cb6-a839-46f2-ae19-0cf4bcbcbb69 · outbound

This paper cites 2011, , 527, L11, 10.1051/0004-6361/201016331.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2011, , 527, L11, 10.1051/0004-6361/201016331

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.096827Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation eb804ced-a6c1-49f9-88c2-81b266278da4 · outbound

This paper cites 2021, , 645, A106, 10.1051/0004-6361/201936291.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2021, , 645, A106, 10.1051/0004-6361/201936291

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.100274Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 222a9451-455b-49c3-a475-44c181d2a799 · outbound

This paper cites J., Mulders , G.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars J., Mulders , G

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.104077Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b51ede00-9c00-443e-b712-e399221859f8 · outbound

This paper cites 2011 a , , 63, L57, 10.1093/pasj/63.6.L57.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2011 a , , 63, L57, 10.1093/pasj/63.6.L57

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.107628Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cf9a4de9-c043-453a-8489-735b5d3560fa · outbound

This paper cites N., et al.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars N., et al

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.111076Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation dc3952a5-1200-41b2-90ea-5dbebcceabf5 · outbound

This paper cites 2023, , 949, L35, 10.3847/2041-8213/acd6f5.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2023, , 949, L35, 10.3847/2041-8213/acd6f5

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.114684Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b0fcdf44-fa6c-4e6b-a380-aa5b96ca732b · outbound

This paper cites 2021, Proceedings of the National Academy of Science, 118, e2017418118, 10.1073/pnas.2017418118.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2021, Proceedings of the National Academy of Science, 118, e2017418118, 10.1073/pnas.2017418118

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.118288Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c95969f1-2d13-47d6-b093-8959080ddae9 · outbound

This paper cites J., Robertson , P., Hartigan , P., Oelkers , R.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars J., Robertson , P., Hartigan , P., Oelkers , R

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.122411Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c7f716c6-fada-4d34-84d2-b8bfa754bd59 · outbound

This paper cites 2024, arXiv e-prints, arXiv:2402.07346.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2024, arXiv e-prints, arXiv:2402.07346

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.126694Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a8f3888c-780b-466f-9cfc-f03840af3433 · outbound

This paper cites an unresolved cited work.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars Unresolved cited work

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.130809Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4b035a9d-e413-4d9f-a2fc-a877941c15f2 · outbound

This paper cites S., & Winn , J.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars S., & Winn , J

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.135612Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation def343f4-5fb2-46e7-ad10-ea2f9b9e8a0f · outbound

This paper cites M., Twicken , J.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars M., Twicken , J

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.139965Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c777f206-eb9f-42ca-8711-dc5b1945349f · outbound

This paper cites M., McCullough , P.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars M., McCullough , P

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.144327Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1b257b3d-82eb-4070-9482-147eb830e400 · outbound

This paper cites C., Cochran , W.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars C., Cochran , W

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.148310Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e2eaccdf-7647-4755-a716-9a20e071c798 · outbound

This paper cites 1755, Allgemeine Naturgeschichte und Theorie des Himmels.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 1755, Allgemeine Naturgeschichte und Theorie des Himmels

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.152524Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 01b235ee-e84b-447b-86db-af602d4be39a · outbound

This paper cites 2023, , 672, L7, 10.1051/0004-6361/202245608.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2023, , 672, L7, 10.1051/0004-6361/202245608

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.156589Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 047d96b7-4a07-4ab2-bb15-076f94b50b6a · outbound

This paper cites 2023, , 523, 1182, 10.1093/mnras/stad1492.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2023, , 523, 1182, 10.1093/mnras/stad1492

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.160692Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 336ed4d1-43b2-4dea-a3e7-7cfc025b8719 · outbound

This paper cites 2024, , 532, 604, 10.1093/mnras/stae1423.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2024, , 532, 604, 10.1093/mnras/stae1423

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.164738Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation df07e475-83c7-4a1c-a718-c5fa8509cf4f · outbound

This paper cites H., Winn , J.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars H., Winn , J

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.169099Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d46b80a8-c55c-44df-8694-d5b0957a122a · outbound

This paper cites A., Fulton , B.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars A., Fulton , B

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.173170Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 987a13a8-db1d-44a3-8476-9c1fcd82cf26 · outbound

This paper cites M., Kraus , A.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars M., Kraus , A

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.177592Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 05e92f7a-cf22-4d73-b3cf-092e3f93e07f · outbound

This paper cites an unresolved cited work.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars Unresolved cited work

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.181741Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 70aad999-8b2d-4524-958b-ca67875d0398 · outbound

This paper cites an unresolved cited work.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars Unresolved cited work

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.185781Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8ce65e6c-fabd-4b71-b37f-aa4e586fd7b1 · outbound

This paper cites 2018, , 616, A2, 10.1051/0004-6361/201832727.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2018, , 616, A2, 10.1051/0004-6361/201832727

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.190172Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation dce5d583-345d-4fa8-b0a3-0e1c6b3704a8 · outbound

This paper cites A., Hern \'a ndez , J., et al.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars A., Hern \'a ndez , J., et al

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.195054Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7ad5ad1c-4a9d-46fb-97a2-b5d0cdc83602 · outbound

This paper cites 2014, Proceedings of the National Academy of Sciences, 111, 12610, 10.1073/pnas.1308261110.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2014, Proceedings of the National Academy of Sciences, 111, 12610, 10.1073/pnas.1308261110

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.199471Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 542bd172-c8f8-4a28-96d7-2c35db8b51a5 · outbound

This paper cites 2023, , 959, L5, 10.3847/2041-8213/ad0fea.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2023, , 959, L5, 10.3847/2041-8213/ad0fea

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.203855Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f177e4ce-86a9-45ee-9149-f2ce4b155499 · outbound

This paper cites 2015, , 579, A136, 10.1051/0004-6361/201526030.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2015, , 579, A136, 10.1051/0004-6361/201526030

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.208066Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a52bcef0-dbce-4e24-85f4-410680dd0014 · outbound

This paper cites 2010, in Proceedings of the 9th Python in Science Conference, Vol.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2010, in Proceedings of the 9th Python in Science Conference, Vol

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.212249Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2944d451-f822-4260-84f1-dada8ca05851 · outbound

This paper cites an unresolved cited work.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars Unresolved cited work

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.216530Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 05b73106-542c-4581-a6cf-9c9ddda4e8e9 · outbound

This paper cites 2017, , 849, L33, 10.3847/2041-8213/aa9714.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2017, , 849, L33, 10.3847/2041-8213/aa9714

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.220730Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b93a36a5-aaad-4020-8499-1c0e2957eb06 · outbound

This paper cites an unresolved cited work.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars Unresolved cited work

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.224814Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c66bc592-ee83-470c-a8f0-3db8f12af962 · outbound

This paper cites 2011, , 742, 72, 10.1088/0004-637X/742/2/72.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2011, , 742, 72, 10.1088/0004-637X/742/2/72

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.228740Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 541fa27e-9577-4c03-b7d4-4a69ef22c489 · outbound

This paper cites 2008, , 678, 498, 10.1086/529369.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars 2008, , 678, 498, 10.1086/529369

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.232325Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 41bcf084-2914-4a1a-b8f8-475a094876cc · outbound

This paper cites A., & Mead, R.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars A., & Mead, R

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.235904Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6033b538-4d6d-446e-9af9-511ac189bb30 · outbound

This paper cites A., Hinkley , S., et al.

From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars A., Hinkley , S., et al

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-11T21:30:15.239450Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Pith citing papers

Observation 615139cb-8303-4a93-b973-5b0e2a892989 · inbound

Statistical Reevaluation of the USP Classification Boundary: Smaller Planets Within 1 Day, Larger Period Ratios Below 2 Days cites this paper.

Statistical Reevaluation of the USP Classification Boundary: Smaller Planets Within 1 Day, Larger Period Ratios Below 2 Days From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-08T11:40:37.492574Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 454032ce-172a-4e45-b747-803c3e5675da · inbound

Ten Aligned Orbits: Planet Migration in the Era of JWST and Ariel cites this paper.

Ten Aligned Orbits: Planet Migration in the Era of JWST and Ariel From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-07T13:59:14.731214Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b50689fa-8c9a-4d26-a6b1-6e3a606eba6f · inbound

TOI-880 is an Aligned, Coplanar, Multi-planet System cites this paper.

TOI-880 is an Aligned, Coplanar, Multi-planet System From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars

Reference 61

Resolution: metadata mismatch; local_arxiv, observed 2026-08-06T15:24:24.837273Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 59dca3b3-8598-483c-815c-fd42bfeed5a0 · inbound

Warm Sub-Saturns Orbiting Single Stars Are Spin-Orbit Aligned cites this paper.

Warm Sub-Saturns Orbiting Single Stars Are Spin-Orbit Aligned From Misaligned Sub-Saturns to Aligned Brown Dwarfs: The Highest $M_{\rm p}/M{_*}$ Systems Exhibit Low Obliquities, Even around Hot Stars

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-03T04:43:50.931811Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.