Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes | Paper Citation Record

Observation a36e1f4a-2a60-4d1e-9d26-a13363c92a52 · outbound

This paper cites 2018, , 615, A110.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes 2018, , 615, A110

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Observation d2882cbd-9040-4e52-bfce-53655c6179d8 · outbound

This paper cites 2015, , 577, A42.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes 2015, , 577, A42

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This paper cites & Morbidelli , A.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes & Morbidelli , A

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Observation 27326ea4-8409-497b-8ce0-924169745399 · outbound

This paper cites & Bitsch , B.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes & Bitsch , B

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This paper cites 2015, Nature, 520, pp.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes 2015, Nature, 520, pp

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This paper cites 2019, , 887, L14.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes 2019, , 887, L14

Reference 6

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This paper cites C., & Kley , W.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes C., & Kley , W

Reference 7

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Observation 06c194b7-2147-4eed-b64e-f4b0969e4274 · outbound

This paper cites & Izidoro , A.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes & Izidoro , A

Reference 8

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This paper cites 2019 a , , 623, A88.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes 2019 a , , 623, A88

Reference 9

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This paper cites 2015 a , A&A, 575, id.A28.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes 2015 a , A&A, 575, id.A28

Reference 10

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This paper cites 2015 b , A&A, 582, id.A112.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes 2015 b , A&A, 582, id.A112

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This paper cites 2018 a , , 609, C2.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes 2018 a , , 609, C2

Reference 12

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This paper cites 2018 b , A&A, 612, id.A30.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes 2018 b , A&A, 612, id.A30

Reference 13

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This paper cites N., Buchhave , L.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes N., Buchhave , L

Reference 14

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This paper cites N., & Izidoro , A.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes N., & Izidoro , A

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This paper cites & Savvidou , S.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes & Savvidou , S

Reference 16

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Observation d11ab1df-ca30-477c-9b6a-9f282b068fbd · outbound

This paper cites 2020, , 643, A66.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes 2020, , 643, A66

Reference 17

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This paper cites 2017, AJ, 153, id.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes 2017, AJ, 153, id

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Observation e41c4b19-cd1f-4f62-a094-e3dc96d8caa2 · outbound

This paper cites G., Ormel , C.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes G., Ormel , C

Reference 19

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This paper cites an unresolved cited work.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes Unresolved cited work

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Observation 7538e01d-ad0d-47ef-a0ff-689ed4b9bcab · outbound

This paper cites E., Wetherill , G.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes E., Wetherill , G

Reference 21

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This paper cites an unresolved cited work.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes Unresolved cited work

Reference 22

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Observation 51cdec63-8510-48a4-a3c4-0ddb77e46148 · outbound

This paper cites P., Kuiper , R., & Ormel , C.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes P., Kuiper , R., & Ormel , C

Reference 23

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This paper cites an unresolved cited work.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes Unresolved cited work

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Observation ce36719a-54cf-46d6-880f-b146b97c7b6a · outbound

This paper cites & Nelson, R.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes & Nelson, R

Reference 25

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Observation 50f12a60-b59a-4210-b871-5dbd37417685 · outbound

This paper cites & Morbidelli , A.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes & Morbidelli , A

Reference 26

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Observation 81dd47e4-bfc9-4399-b80a-b799644009db · outbound

This paper cites I., Chiang , E., & Lee , E.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes I., Chiang , E., & Lee , E

Reference 27

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T18:40:03.538474Z

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Observation 2b340843-ca6c-4ad1-9d64-4b8c701e0c8d · outbound

This paper cites 2021, , 656, A69.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes 2021, , 656, A69

Reference 28

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This paper cites 2022, , 509, 2856.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes 2022, , 509, 2856

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Observation 57139528-3d5d-4848-bce1-131376aa34aa · outbound

This paper cites N., & Bitsch , B.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes N., & Bitsch , B

Reference 30

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Observation 2464a5c7-26d2-45ef-9d6a-15f8944fe109 · outbound

This paper cites C., Bitsch , B., & Isella , A.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes C., Bitsch , B., & Isella , A

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Observation 01c02367-8918-43e9-97c2-ae48df9aa73c · outbound

This paper cites C., Lissauer , J.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes C., Lissauer , J

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Observation b4f133d7-70bb-4b81-ac17-8c144b034a58 · outbound

This paper cites J., Mulders , G.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes J., Mulders , G

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Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes 2013, ApJ, 766, id.81

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This paper cites J., Petigura , E.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes J., Petigura , E

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Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes 1993, Icarus, 106, 247

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Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes & Schlichting , H

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This paper cites an unresolved cited work.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes Unresolved cited work

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Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes & Bae , J

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Observation af9f3ecc-5e7c-408b-bb98-869daed3c3f5 · outbound

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Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes 1981, Progress of Theoretical Physics Supplement, 70, pp.35

Reference 40

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This paper cites an unresolved cited work.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes Unresolved cited work

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This paper cites & Ormel , C.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes & Ormel , C

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This paper cites A., Pichierri , G., Bitsch , B., & Batygin , K.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes A., Pichierri , G., Bitsch , B., & Batygin , K

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Observation ac366098-c54f-465e-92f0-938d8195e9bf · outbound

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Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes 2000, ApJ, 537, pp

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Observation a1b81bbb-2c1c-4908-9af7-66a494859557 · outbound

This paper cites an unresolved cited work.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes Unresolved cited work

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Observation 8f91a4e9-7359-489d-9873-2023aa8cb18b · outbound

This paper cites N., et al.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes N., et al

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This paper cites N., et al.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes N., et al

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Observation 841b7cba-d43d-4ab3-a2d7-6c32f1b47adb · outbound

This paper cites E., Isella , A., et al.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes E., Isella , A., et al

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Observation 51383448-d862-417a-a73c-6b102c3175eb · outbound

This paper cites an unresolved cited work.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes Unresolved cited work

Reference 49

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Observation 8e9f4019-ce7a-4c09-9484-ceef25a4c91e · outbound

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Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes & Mordasini , C

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This paper cites & Lacerda, P.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes & Lacerda, P

Reference 51

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Observation cfb0e19a-1c43-4a84-b5f9-a3fac113d66b · outbound

This paper cites & Lambrechts, M.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes & Lambrechts, M

Reference 52

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Observation b9f0d09f-8270-4cca-a31f-099e095d817c · outbound

This paper cites M., Lacerda, P., & Bizzarro, M.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes M., Lacerda, P., & Bizzarro, M

Reference 53

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Observation 546f7fe0-bcab-4d4d-b99f-ac6546a53521 · outbound

This paper cites 2021, Science Advances, 7, eabc0444.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes 2021, Science Advances, 7, eabc0444

Reference 54

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Observation 68a980d1-a991-41fd-9320-04292c784c14 · outbound

This paper cites D., Tanaka , H., & Szuszkiewicz , E.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes D., Tanaka , H., & Szuszkiewicz , E

Reference 55

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T18:40:03.197101Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 6ef83e70-bc8a-4fe9-a606-1317ef02d836 · outbound

This paper cites & Nelson, R.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes & Nelson, R

Reference 56

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T18:40:03.183228Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 95820d3f-3986-43aa-ad02-0381f8349fb6 · outbound

This paper cites & Johansen , A.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes & Johansen , A

Reference 57

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T18:40:03.168997Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 3e22fc25-0fd6-4ec7-9ad8-7c0e76973d01 · outbound

This paper cites & Johansen, A.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes & Johansen, A

Reference 58

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T18:40:03.155167Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation a95e183e-e8b5-4cde-9e07-75c1964f8a54 · outbound

This paper cites 2014, A&A, 572, id.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes 2014, A&A, 572, id

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-12T18:40:02.467072Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cdc67f5c-f057-466a-a397-8dedf9f9d5a7 · outbound

This paper cites & Lega , E.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes & Lega , E

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-12T18:40:02.472660Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a5670e95-de21-4404-8504-5e5c86aa4e00 · outbound

This paper cites A., et al.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes A., et al

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-12T18:40:02.476808Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f73ca3a5-ffde-4b54-b1f1-9080364ce791 · outbound

This paper cites an unresolved cited work.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes Unresolved cited work

Reference 62

Resolution: unresolved; raw_fallback, observed 2026-08-12T18:40:03.113860Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 90892b11-0b81-490c-9508-434b82ed6a61 · outbound

This paper cites an unresolved cited work.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes Unresolved cited work

Reference 63

Resolution: unresolved; raw_fallback, observed 2026-08-12T18:40:03.100525Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation f35e0489-0742-447b-9081-2ac603b45274 · outbound

This paper cites C., et al.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes C., et al

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-12T18:40:02.489720Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 47d2df0b-8c7b-453a-b56b-dbe8e17433ed · outbound

This paper cites 2023, in Astronomical Society of the Pacific Conference Series, Vol.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes 2023, in Astronomical Society of the Pacific Conference Series, Vol

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-12T18:40:02.494160Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5e758289-0496-4ab0-a538-64e05975244a · outbound

This paper cites 2024, , 627, 501.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes 2024, , 627, 501

Reference 66

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T18:40:03.070337Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 63eb3eb3-448e-4eee-a893-f02c1929cf18 · outbound

This paper cites an unresolved cited work.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes Unresolved cited work

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-12T18:40:02.502811Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9cfcc6ac-3890-417a-a913-70efbf682f75 · outbound

This paper cites an unresolved cited work.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes Unresolved cited work

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-12T18:40:02.507460Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9217d6af-e3e3-4b88-8b84-994a786baa30 · outbound

This paper cites an unresolved cited work.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes Unresolved cited work

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-12T18:40:02.511509Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9e7d7b95-8d07-4050-9e37-a92a9b575808 · outbound

This paper cites S., Morbidelli , A., Crida , A., & Ferreira , J.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes S., Morbidelli , A., Crida , A., & Ferreira , J

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-12T18:40:02.515710Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bf64b762-41ef-4b3f-9fcb-35111e44cc55 · outbound

This paper cites 2021, , 650, A116.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes 2021, , 650, A116

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-12T18:40:02.519781Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d3f6291f-7c70-4c98-ac19-c69cc749e16c · outbound

This paper cites 2011, ArXiv e-prints.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes 2011, ArXiv e-prints

Reference 72

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T18:40:03.011097Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 24baade0-6171-42d9-a18d-dca65e6cdb88 · outbound

This paper cites 2017, , 849, L33.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes 2017, , 849, L33

Reference 73

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T18:40:02.996828Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation bdf16ab6-631a-49f2-853a-d1565a12d9ed · outbound

This paper cites an unresolved cited work.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes Unresolved cited work

Reference 74

Resolution: unresolved; raw_fallback, observed 2026-08-12T18:40:02.982535Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 5541662d-f411-47a4-946e-aa378e117616 · outbound

This paper cites M., Fabrycky , D.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes M., Fabrycky , D

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-12T18:40:02.536669Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a6e69393-d897-4dec-bbf9-0c81db07c334 · outbound

This paper cites W., Kuiper , R., Kley , W., & Ormel , C.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes W., Kuiper , R., Kley , W., & Ormel , C

Reference 76

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T18:40:02.959342Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation f4372258-9484-4ecc-be76-692a558f4594 · outbound

This paper cites D., Pascucci , I., Apai , D., & Ciesla , F.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes D., Pascucci , I., Apai , D., & Ciesla , F

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-12T18:40:02.545782Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 45578c56-c342-40be-bc47-0a3720475da4 · outbound

This paper cites an unresolved cited work.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes Unresolved cited work

Reference 78

Resolution: unresolved; raw_fallback, observed 2026-08-12T18:40:02.936537Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation ac4deec3-9a1f-4c98-a654-b43693eaaca7 · outbound

This paper cites 2018, , 56, 137.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes 2018, , 56, 137

Reference 79

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T18:40:02.922874Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 0c1cf78a-b110-45b5-9adc-89fd92a47aa9 · outbound

This paper cites K., & Morbidelli , A.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes K., & Morbidelli , A

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-12T18:40:02.558838Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation acacc70b-ef4b-43e4-98eb-8e2da5024ee8 · outbound

This paper cites 2015, , 578, A36.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes 2015, , 578, A36

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-12T18:40:02.562340Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0c0f5775-4e3f-458b-96ae-e3aaa0c266ba · outbound

This paper cites 2024, , 972, 181.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes 2024, , 972, 181

Reference 82

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T18:40:02.890553Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 3435af65-9091-444b-b543-f24acef5b2c6 · outbound

This paper cites an unresolved cited work.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes Unresolved cited work

Reference 83

Resolution: unresolved; raw_fallback, observed 2026-08-12T18:40:02.876428Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation a7937d1b-e1a6-4fa5-95af-387500839456 · outbound

This paper cites an unresolved cited work.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes Unresolved cited work

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-12T18:40:02.573162Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 01a740f4-d97f-4a23-a430-e9248dbb2d0f · outbound

This paper cites J., Baruteau , C., & Kley , W.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes J., Baruteau , C., & Kley , W

Reference 85

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T18:40:02.852974Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 81a5e896-0713-4b37-a6fe-53940ff4bf16 · outbound

This paper cites 2019, , 625, A7.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes 2019, , 625, A7

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-12T18:40:02.580394Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fb0d9165-4db5-4c42-8df2-65bb63eb8eaa · outbound

This paper cites 2023, , 670, A148.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes 2023, , 670, A148

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-12T18:40:02.584146Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f87e0150-ca5f-4df8-83a9-c555f7422d56 · outbound

This paper cites 2024, , 967, 111.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes 2024, , 967, 111

Reference 88

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T18:40:02.821201Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 1588fba5-fa1b-4fa3-b0f2-4ac889e1b0b2 · outbound

This paper cites W., & Dorn , C.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes W., & Dorn , C

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-12T18:40:02.592178Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 20d5e5a9-5cd6-4235-96e5-2d19c77968fe · outbound

This paper cites 2019, , 632, A118.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes 2019, , 632, A118

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-12T18:40:02.596380Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9307980f-6f74-401c-a332-397bb6b37a52 · outbound

This paper cites 2024, , 689, A285.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes 2024, , 689, A285

Reference 91

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T18:40:02.790142Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation b8d024aa-bd72-4a75-a341-1a6fc5769292 · outbound

This paper cites X., Welbanks , L., Teske , J., & Buchner , J.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes X., Welbanks , L., Teske , J., & Buchner , J

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-12T18:40:02.604968Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 282fb0d1-25d8-4ab3-a24c-988fba368519 · outbound

This paper cites P., Sumi , T., et al.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes P., Sumi , T., et al

Reference 93

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T18:40:02.766922Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 370def3a-506e-452b-8e61-56e3b9273cd0 · outbound

This paper cites an unresolved cited work.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes Unresolved cited work

Reference 94

Resolution: unresolved; raw_fallback, observed 2026-08-12T18:40:02.751661Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 3f0ea8e0-d516-468c-a662-fb39ef482f87 · outbound

This paper cites S., et al.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes S., et al

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-12T18:40:02.617462Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a33ae761-e0a8-4422-b245-7b0d0f9dbaa4 · outbound

This paper cites W., Huang , P., & Kuiper , R.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes W., Huang , P., & Kuiper , R

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-12T18:40:02.621522Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d7ec0f17-a175-4c78-a2ad-e39f2c604d07 · outbound

This paper cites an unresolved cited work.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes Unresolved cited work

Reference 97

Resolution: unresolved; raw_fallback, observed 2026-08-12T18:40:02.718398Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 146e9dcd-0d0a-4b70-a741-2c2e8a48b952 · outbound

This paper cites M., Marcy , G.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes M., Marcy , G

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-12T18:40:02.630261Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b8f110aa-b8ba-4769-952b-8c08214e8a12 · outbound

This paper cites A., & Ford , E.

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes A., & Ford , E

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-12T18:40:02.634564Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cc4048f3-7696-4618-80e3-6189c84546ac · outbound

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

Diversity of disc viscosities can explain the period ratios of resonant and non-resonant systems of hot super-Earths and mini-Neptunes , " * write output.state after.block = add.period write newline

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-12T18:40:02.638993Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Coverage vector

Reference resolution

Outbound references

Pith citing papers