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Paper Citation Record · LEDGER

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes

As of 18 August 2026, this Paper Citation Record lists 100 of 115 outbound references and 0 inbound Pith citation observations for arXiv:1908.02742.

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

pith.paper-citation-record.v1
1908.02742 v2

Coverage vector

measured 100 of 115 reference resolution

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Pith citing papers itemized under the disclosed page cap.

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Reference resolution

100 of 115 outbound references displayed

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External citation measurements

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Outbound references

Observation 3717a2ff-ca87-4001-9fa9-2d6797f0c5a5 · outbound

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

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes , " * write output.state after.block = add.period write newline

Reference 1

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Observation 0a839a5a-a4f1-486e-b25a-4513163c2d61 · outbound

This paper cites write newline.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes write newline

Reference 2

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Observation 3630adf5-2677-48d9-9a6c-a1cc1d51894e · outbound

This paper cites E., & Cridland , A.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes E., & Cridland , A

Reference 3

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Observation c80bfd44-1e68-4eef-b3ae-cc16422ba837 · outbound

This paper cites 2017, , 606, A69.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes 2017, , 606, A69

Reference 4

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Observation 4d7983bc-3afa-4fc6-b75c-b2aa5e96892e · outbound

This paper cites an unresolved cited work.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes Unresolved cited work

Reference 5

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Observation 5a93147c-fefc-4fa3-8ded-b1cd24883fd4 · outbound

This paper cites 2004, , 419, L13.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes 2004, , 419, L13

Reference 6

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Observation 3148c3b0-c38d-493d-a855-c6e56be57fd5 · outbound

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How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes Unresolved cited work

Reference 7

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Observation f540b3c7-2c27-4dc2-9f49-654f509ed242 · outbound

This paper cites 2013, Stellar Structure and Evolution (Springer), 47--63.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes 2013, Stellar Structure and Evolution (Springer), 47--63

Reference 8

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Observation 1986bb0c-d06f-4789-9fed-5bdb03e77e2a · outbound

This paper cites an unresolved cited work.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes Unresolved cited work

Reference 9

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Observation 6ccb9626-43c6-430c-8200-bc974b9006c7 · outbound

This paper cites & Asphaug , E.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes & Asphaug , E

Reference 10

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Observation 7c7884a7-a844-49e0-ab72-8aeff5274568 · outbound

This paper cites K., Irwin , J., Charbonneau , D., et al.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes K., Irwin , J., Charbonneau , D., et al

Reference 11

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Observation 02271bfd-4077-44ec-bc69-b9dc0c4fd115 · outbound

This paper cites N., & Izidoro , A.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes N., & Izidoro , A

Reference 12

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Observation 5da2f54c-60cc-484f-9032-b947fbafb98f · outbound

This paper cites J., Lissauer , J.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes J., Lissauer , J

Reference 13

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Observation 7969f6b1-00ca-4892-a149-b3be1bd7489c · outbound

This paper cites J., Koch , D.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes J., Koch , D

Reference 14

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Observation 67b27de4-e4ac-4f1a-b252-bb59c17a85fa · outbound

This paper cites G., Vazan , A., & Ormel , C.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes G., Vazan , A., & Ormel , C

Reference 15

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Observation d9a06b1d-fe19-4cf9-9a19-843a5a10b183 · outbound

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How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes & Laughlin , G

Reference 16

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Observation 1b2d5bed-a114-4cd5-95b6-f744953a2e9b · outbound

This paper cites F., Thomas , P.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes F., Thomas , P

Reference 17

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Observation 0552cd0a-2557-4e6e-bb7b-fd93412ee569 · outbound

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

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes P., Kuiper , R., & Ormel , C

Reference 18

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Observation 0e70dbd8-12dc-40a0-bd40-099a6e25a349 · outbound

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How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes Unresolved cited work

Reference 19

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Observation af187f1b-f935-4d84-b33f-4fe28deb168c · outbound

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How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes Unresolved cited work

Reference 20

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Observation c8dbcc8b-3ca5-4f47-a50b-09eb98ad7291 · outbound

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How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes & Bodenheimer , P

Reference 21

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Observation 2173cae0-45cf-4dc1-81f9-71c2b9853f70 · outbound

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How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes & Podolak , M

Reference 22

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Observation 10824d60-2dce-47b5-85cb-7da0df680458 · outbound

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

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes I., Chiang , E., & Lee , E

Reference 23

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This paper cites D., Charbonneau , D., & Newton , E.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes D., Charbonneau , D., & Newton , E

Reference 24

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Observation d080cf1d-8bf5-4186-a269-b71f753b7fe6 · outbound

This paper cites 2018, Computer Physics Communications, 227, 117.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes 2018, Computer Physics Communications, 227, 117

Reference 25

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How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes 2013, , 766, 81

Reference 26

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How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes Unresolved cited work

Reference 27

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Observation 33d1589c-df3a-4f4f-b855-b4a9e66aa203 · outbound

This paper cites J., Petigura , E.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes J., Petigura , E

Reference 28

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Observation 3f4f3ceb-a2b6-49b8-a1f2-3c14bda2d840 · outbound

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How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes 2015, , 811, 101

Reference 29

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Observation 31d1b671-69a2-4906-8738-7650a77924d3 · outbound

This paper cites E., & Sari , R.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes E., & Sari , R

Reference 30

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How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes E., & Sari , R

Reference 31

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How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes 2010, , 520, A27

Reference 32

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Observation d1bf89ea-a91e-4463-9887-eed2f2898e0c · outbound

This paper cites Sculpting the Valley in the Radius Distribution of Small Exoplanets as a by-product of Planet Formation: The Core-Powered Mass-Loss Mechanism.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes Sculpting the Valley in the Radius Distribution of Small Exoplanets as a by-product of Planet Formation: The Core-Powered Mass-Loss Mechanism

Reference 33

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This paper cites 1981, Progress of Theoretical Physics Supplement, 70, 35.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes 1981, Progress of Theoretical Physics Supplement, 70, 35

Reference 34

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How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes & Guillot , T

Reference 35

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How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes & Stevenson , D

Reference 36

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How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes & Ikoma , M

Reference 37

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How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes Unresolved cited work

Reference 38

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Observation ae25501e-b1d4-49f9-97c1-a8b965d5112e · outbound

This paper cites B., Hattori , M.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes B., Hattori , M

Reference 39

Resolution
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

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Observation b152803d-8a69-4a18-98f1-c6945ed46af7 · outbound

This paper cites an unresolved cited work.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes Unresolved cited work

Reference 40

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T14:45:38.357474Z digest=sha256:7aa7bd13be1a14131853d14e7e1387574cee3964205b21071f56f625edfb3931

Observation adca26ad-a278-4ba0-a405-08d0d43edac9 · outbound

This paper cites & Podolak , M.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes & Podolak , M

Reference 41

Resolution
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T14:45:38.360804Z digest=sha256:5e60984725ab495e861004b2e403c21436075b84fa1d2f4aaf8f5925a06d49a2

Observation 3c2f7610-3896-4dfa-b25b-0f012dfa18ea · outbound

This paper cites & Hori , Y.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes & Hori , Y

Reference 42

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T14:45:38.363616Z digest=sha256:6b649f8faf32900a093f6c6ba90f26369baece1e0f237ad55cce18b973e9b8ef

Observation a10e4c28-bdfd-46ea-b225-2e2266f81d17 · outbound

This paper cites an unresolved cited work.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes Unresolved cited work

Reference 43

Resolution
unresolved
raw_fallback, observed 2026-08-14T14:45:39.348605Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T14:45:38.366438Z digest=sha256:bc3d1e349e1faaaeb74a6daff7f8f0801c941b9516475c647a296bb300ef0cb9

Observation 03f2349f-d2ce-4c52-9d70-388337067115 · outbound

This paper cites & Mordasini , C.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes & Mordasini , C

Reference 44

Resolution
unresolved
no resolver link, observed 2026-08-14T14:45:38.369182Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T14:45:38.369182Z digest=sha256:56ef3f4f2b9862f94b16023d31ad273fd03d990795d48d21b5cd73141cdace87

Observation 51f3dbe4-e3f7-4585-806f-6ea3c89bfc22 · outbound

This paper cites S., Mac Low , M.-M., et al.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes S., Mac Low , M.-M., et al

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-14T14:45:38.372072Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T14:45:38.372072Z digest=sha256:d1becf6960dd00f6c2959d03c06bd238c67fa15ad56151a4fd748cfbbdbe3ec6

Observation 526cb231-9fe3-4531-8059-3a93de7dc487 · outbound

This paper cites 2009, , 704, L75.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes 2009, , 704, L75

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-14T14:45:38.374879Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T14:45:38.374879Z digest=sha256:50ff869d4852ff01c00e857b4d5ce9380837f4d364dd69797c280db028605ad5

Observation bd88d658-fd9f-4f32-aac7-9d4d6bf01d42 · outbound

This paper cites & Weigert , A.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes & Weigert , A

Reference 47

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T14:45:38.377526Z digest=sha256:41241263ebbc2c6a2bfd9c7d8097ddedb890057905f207afa647fddca44f6f09

Observation 3f2266f1-931f-490a-a17b-a82199e97844 · outbound

This paper cites G., Stewart , S.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes G., Stewart , S

Reference 48

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T14:45:39.308664Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T14:45:38.380866Z digest=sha256:a9c91df7654d1af7f622ac6839085e600ae274a2daebce43e071371f95d90f44

Observation f1890357-dcf1-481b-979d-9a797b0c337e · outbound

This paper cites & Johansen , A.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes & Johansen , A

Reference 49

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 55ae8728-c6d6-4ae0-b358-87364cf79324 · outbound

This paper cites 2014, , 572, A35.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes 2014, , 572, A35

Reference 50

Resolution
unresolved
no resolver link, observed 2026-08-14T14:45:38.388626Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T14:45:38.388626Z digest=sha256:c3a0b911202097db74588294ce91fc5cab082b4e66e66c8d733986a98cb57af0

Observation f3dd0913-584b-472d-a596-dd0cf3853128 · outbound

This paper cites A., et al.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes A., et al

Reference 51

Resolution
unresolved
no resolver link, observed 2026-08-14T14:45:38.392297Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T14:45:38.392297Z digest=sha256:99a38e7ea9c81d701ed4b39afb6d818f493aab89b41fb5b4166a3d786a21ceac

Observation b4b646fd-f156-474e-9b09-9d0305c274b4 · outbound

This paper cites an unresolved cited work.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes Unresolved cited work

Reference 52

Resolution
unresolved
no resolver link, observed 2026-08-14T14:45:38.395653Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T14:45:38.395653Z digest=sha256:59bccb949799929a79c812e8ee9bf6a080116dcdf8bdd1d85cb546a09ec86ccd

Observation e3a0da94-36f4-4a5a-99de-0cf3b57f73df · outbound

This paper cites an unresolved cited work.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes Unresolved cited work

Reference 53

Resolution
unresolved
no resolver link, observed 2026-08-14T14:45:38.399085Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T14:45:38.399085Z digest=sha256:03cfa8633e534fb3cd481ab7116209140dcac5d0763d9ac07067a1fdec16c0aa

Observation 43e5ba18-18e2-47e0-be14-8278d6a74699 · outbound

This paper cites an unresolved cited work.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes Unresolved cited work

Reference 54

Resolution
unresolved
raw_fallback, observed 2026-08-14T14:45:39.267862Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T14:45:38.402520Z digest=sha256:3832eccdf9269254629347f71c7f99575919f85ce6b9cb10dae30ca79bd59e49

Observation 37d7c0b0-5bcd-4442-b3c2-7204b4e26a66 · outbound

This paper cites J., Chiang , E., & Ormel , C.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes J., Chiang , E., & Ormel , C

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-14T14:45:38.405755Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T14:45:38.405755Z digest=sha256:2dc31078eb0d21d04c592e17314a6322d4df3bde0fe72fb8322bce193ea96b0c

Observation 2aafb6b0-ac71-4780-bca9-5a659fdd79e3 · outbound

This paper cites Demographics of Planetesimals Formed by the Streaming Instability.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes Demographics of Planetesimals Formed by the Streaming Instability

Reference 56

Resolution
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

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Observation ddaef791-334d-4228-9e89-923641181146 · outbound

This paper cites J., Hubickyj , O., D'Angelo , G., & Bodenheimer , P.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes J., Hubickyj , O., D'Angelo , G., & Bodenheimer , P

Reference 57

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T14:45:38.413138Z digest=sha256:de040b22bf7cd5cf535cd4f5b4827496e85078e779796b14323bb1f84133f005

Observation e645381c-f463-4751-bb75-1623564b3e1e · outbound

This paper cites an unresolved cited work.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes Unresolved cited work

Reference 58

Resolution
unresolved
raw_fallback, observed 2026-08-14T14:45:39.245179Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T14:45:38.416634Z digest=sha256:6f91d20f2f5d87dfdb5051f3d02e70b30e3136174650cd18f2b40926528c00c5

Observation 10abef36-f478-4678-a0fa-cc97fd18e5d6 · outbound

This paper cites Growth after the streaming instability: from planetesimal accretion to pebble accretion.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes Growth after the streaming instability: from planetesimal accretion to pebble accretion

Reference 59

Resolution
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

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Observation ac0a13ac-2b37-4209-b08a-f961a5cea4a0 · outbound

This paper cites an unresolved cited work.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes Unresolved cited work

Reference 60

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 90ee4db5-b8c0-48d9-bca1-29e1534bee0f · outbound

This paper cites an unresolved cited work.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes Unresolved cited work

Reference 61

Resolution
unresolved
no resolver link, observed 2026-08-14T14:45:38.428583Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T14:45:38.428583Z digest=sha256:2d8e9bde08a9365fa92d534f3fb938ba8317892ce6f9756465d30847ce096075

Observation c8053c97-b95d-4dc4-9d40-b78c89afba17 · outbound

This paper cites D., Fortney , J.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes D., Fortney , J

Reference 62

Resolution
unresolved
no resolver link, observed 2026-08-14T14:45:38.432872Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T14:45:38.432872Z digest=sha256:0d5e0e6ea1e92a5c7bda03bbc94c4a4e78f836cc198a2a1187f0126205a3311f

Observation 7c61d9b6-b15c-4a28-8a0d-00563a832e35 · outbound

This paper cites 2018, , 866, 49.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes 2018, , 866, 49

Reference 63

Resolution
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

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Observation 20beb07f-e271-4c2e-af90-90ab39c5f066 · outbound

This paper cites D., & Bodenheimer , P.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes D., & Bodenheimer , P

Reference 64

Resolution
unresolved
no resolver link, observed 2026-08-14T14:45:38.440388Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T14:45:38.440388Z digest=sha256:0d00cdaf60a5aebf1b71957395f63899e77f829f2b6c4a79791c20372635a0d6

Observation 64734004-80a5-4a65-a02e-cb8fcb0592dd · outbound

This paper cites W., Isaacson , H., Howard , A.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes W., Isaacson , H., Howard , A

Reference 65

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T14:45:38.443751Z digest=sha256:55fe604c2a01134aec9034f4bc550f0c8557942a2d1b00a15bbeddd4a755d19f

Observation 5aa4c7e0-c420-493f-b18c-b8a220ed0b86 · outbound

This paper cites an unresolved cited work.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes Unresolved cited work

Reference 66

Resolution
unresolved
raw_fallback, observed 2026-08-14T14:45:39.185453Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

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Observation 5f967527-179e-4c4e-a81c-1d7ff9b98310 · outbound

This paper cites an unresolved cited work.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes Unresolved cited work

Reference 67

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T14:45:38.450292Z digest=sha256:b97fe36ab7f5c17e38edc97bd70ea80088a6afb8aad3ad2f26f79c44ac922c36

Observation 0b0a9e89-8979-4e31-b140-1f0fd7d1d156 · outbound

This paper cites an unresolved cited work.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes Unresolved cited work

Reference 68

Resolution
unresolved
raw_fallback, observed 2026-08-14T14:45:39.168674Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T14:45:38.453752Z digest=sha256:336756ef89930e2f09694ac0638f9415314373e3cc0756fed1dfc600efc304c5

Observation 575b7c70-f425-499e-8041-814d50ae256d · outbound

This paper cites 1980, Progress of Theoretical Physics, 64, 544.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes 1980, Progress of Theoretical Physics, 64, 544

Reference 69

Resolution
unresolved
no resolver link, observed 2026-08-14T14:45:38.457206Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T14:45:38.457206Z digest=sha256:c454fcec36c798f7c9a8ea02c6fbd782072300022e9b2528b468a19867224a7e

Observation aeb0e6c9-188f-4acb-827c-cb04f5046a40 · outbound

This paper cites 2015, , 258, 418.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes 2015, , 258, 418

Reference 70

Resolution
unresolved
no resolver link, observed 2026-08-14T14:45:38.460744Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T14:45:38.460744Z digest=sha256:0d6bf6d34176103db394ff5618a6d7cf0fae9de594dd96ac54c55a1a10d00a2c

Observation b8561d9b-593c-4ca2-ba68-c8e6f5722526 · outbound

This paper cites & Nesvorny , D.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes & Nesvorny , D

Reference 71

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T14:45:38.463969Z digest=sha256:5fe7491c9f6516f4b912424679497c85650e72426e8f505b43008742901ca3d6

Observation 49017d62-239e-4a3d-8fbf-90aa7e34ebaa · outbound

This paper cites 2014, , 572, A118.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes 2014, , 572, A118

Reference 72

Resolution
unresolved
no resolver link, observed 2026-08-14T14:45:38.468439Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T14:45:38.468439Z digest=sha256:1b96cd0ab2b297fccd0906caba2f89008b12bfbb92d09f7990a9295de7f482a0

Observation c8df2a5b-26c2-40b5-9693-6954d1e26840 · outbound

This paper cites 2015, International Journal of Astrobiology, 14, 201.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes 2015, International Journal of Astrobiology, 14, 201

Reference 73

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T14:45:39.122113Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T14:45:38.472656Z digest=sha256:e05ed0f77e5fba6332db9d621bb1ab610469d9e9e1d07f0cc983eadb92326806

Observation cbece330-7b2a-4708-a616-00ce5bfe2a87 · outbound

This paper cites The Exoplanet Population Observation Simulator. II -- Population Synthesis in the Era of Kepler.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes The Exoplanet Population Observation Simulator. II -- Population Synthesis in the Era of Kepler

Reference 74

Resolution
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local_arxiv, observed 2026-08-14T14:45:38.662202Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

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Observation 08467759-a459-435e-9d8e-e512ccdc9746 · outbound

This paper cites A., Chiang , E.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes A., Chiang , E

Reference 75

Resolution
unresolved
no resolver link, observed 2026-08-14T14:45:38.479995Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T14:45:38.479995Z digest=sha256:21c2884f871f81ecc7c76f168e09bef81f2d001a0172b89b3b5ed077344973f1

Observation e3d74993-8792-482c-8880-a965b8679f48 · outbound

This paper cites an unresolved cited work.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes Unresolved cited work

Reference 76

Resolution
unresolved
raw_fallback, observed 2026-08-14T14:45:39.102135Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T14:45:38.483789Z digest=sha256:cbed39480d87bdcd55be9f698ef44a8557d67f2a27a9d71f6b4bc1bfb6b66170

Observation 02476b23-2324-4b24-b759-eff4730ecdb9 · outbound

This paper cites an unresolved cited work.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes Unresolved cited work

Reference 77

Resolution
unresolved
no resolver link, observed 2026-08-14T14:45:38.486991Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T14:45:38.486991Z digest=sha256:98dd281689e8f2e6e09d7266d1b00e359fa2f931154348f8a486df8ec0cfa1f0

Observation c7a55e8b-db03-4517-824d-baacb8d70b26 · outbound

This paper cites an unresolved cited work.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes Unresolved cited work

Reference 78

Resolution
unresolved
no resolver link, observed 2026-08-14T14:45:38.490335Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T14:45:38.490335Z digest=sha256:8448f5a960435f02c7ef6b9b6035abe38a41d13706a34d9b85d84f36caa6f861

Observation 71600506-e753-44f0-925e-25f45edc1b34 · outbound

This paper cites W., Shi , J.-M., & Kuiper , R.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes W., Shi , J.-M., & Kuiper , R

Reference 79

Resolution
unresolved
no resolver link, observed 2026-08-14T14:45:38.493788Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T14:45:38.493788Z digest=sha256:35f078214527bf0137062b54810a145be87fbb604ed1d8aa542448b4d97ce25a

Observation f468e621-4127-4ba5-bca2-a634fad00eac · outbound

This paper cites an unresolved cited work.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes Unresolved cited work

Reference 80

Resolution
unresolved
no resolver link, observed 2026-08-14T14:45:38.497242Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T14:45:38.497242Z digest=sha256:5dfc9adecbe98f1a0edf09f8ab3bdd603769874479c7fce62c983f6201ebe07f

Observation e6870b33-725b-41d1-bc05-cd52b2762fdb · outbound

This paper cites an unresolved cited work.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes Unresolved cited work

Reference 81

Resolution
unresolved
no resolver link, observed 2026-08-14T14:45:38.500654Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T14:45:38.500654Z digest=sha256:1d45e92eed94fdb21c9095a98aebefe493dd81e95eae904e30c9993391f78c99

Observation 1a5c01d3-b00f-4b70-a063-e523447df682 · outbound

This paper cites an unresolved cited work.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes Unresolved cited work

Reference 82

Resolution
unresolved
raw_fallback, observed 2026-08-14T14:45:39.051181Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T14:45:38.505185Z digest=sha256:8b43e0fffa9e19eb9afcaffc44deb21ad39a143abd971c4f88e87fc0a91dea41

Observation 22244d4b-48ab-4022-9885-9b855478ad63 · outbound

This paper cites an unresolved cited work.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes Unresolved cited work

Reference 83

Resolution
unresolved
raw_fallback, observed 2026-08-14T14:45:39.039185Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T14:45:38.508870Z digest=sha256:5fa25d3ae50c4ab30a749f7c7b58e0c6c20dd47fc39fc3848f063e4062b3583c

Observation bf37eb4c-738c-4826-9315-e1adfda2670c · outbound

This paper cites & Chiang , E.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes & Chiang , E

Reference 84

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T14:45:39.028425Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T14:45:38.513132Z digest=sha256:2bf3cb230a9220e0b3341a54b8e34362f9e62e9dcc0cf73a74ff560f4498ed0e

Observation 8d14b626-468b-4543-89c5-1b166e4b713d · outbound

This paper cites 2002, in COSPAR Meeting, Vol.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes 2002, in COSPAR Meeting, Vol

Reference 85

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T14:45:39.016991Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T14:45:38.516815Z digest=sha256:3a342c6601066893cfd64316c490a4b658b6bd3b895b1b0aa8bac03831ec74b6

Observation aa2332b0-a3a8-4518-974b-f260a59e98da · outbound

This paper cites 2016, , 463, 4516.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes 2016, , 463, 4516

Reference 86

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T14:45:39.004962Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T14:45:38.519933Z digest=sha256:c36d6611218922f26b360e8a9766167e013696e27528682e77b45b0ebcc7fe0a

Observation 8afb3931-5ce4-4c00-845a-3307915c7c46 · outbound

This paper cites an unresolved cited work.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes Unresolved cited work

Reference 87

Resolution
unresolved
no resolver link, observed 2026-08-14T14:45:38.522740Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T14:45:38.522740Z digest=sha256:03101eb09d2fccc3ca63de94b38932ac16f7983df8bd338b32dc7f94f75ce500

Observation 57444082-9762-441e-a706-be847f9ac022 · outbound

This paper cites A., Youdin , A.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes A., Youdin , A

Reference 88

Resolution
unresolved
no resolver link, observed 2026-08-14T14:45:38.525613Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T14:45:38.525613Z digest=sha256:5732854efaaf0f8e57fbf7abe4cb5a236ce96d8cde8e73230feae8128b5fe505

Observation 30cea61e-4cff-4ca4-99c2-0b4d65a8452b · outbound

This paper cites B., & Reynolds , R.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes B., & Reynolds , R

Reference 89

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T14:45:38.976418Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T14:45:38.528604Z digest=sha256:b8e097fcd5270edc3e390ca897424beb1cd5533b05a367d6323c585107595d7c

Observation 8e692de1-bfe8-495a-8668-50861feee329 · outbound

This paper cites B., Hubickyj , O., Bodenheimer , P., et al.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes B., Hubickyj , O., Bodenheimer , P., et al

Reference 90

Resolution
unresolved
no resolver link, observed 2026-08-14T14:45:38.531547Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T14:45:38.531547Z digest=sha256:64a1fa61866644d28f45fbbf2f7aeb7120eff9b1ae13c948b5522010f2fb1fdd

Observation e0b0178a-0a66-4019-94bb-59ed5f11d21e · outbound

This paper cites K., et al.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes K., et al

Reference 91

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T14:45:38.956555Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T14:45:38.535118Z digest=sha256:a5899b43967303b82a80fd548f7ff5e0a982518f51a2bb50b0aa7ad9518c260b

Observation 94b27886-a9f1-4299-8922-197c439301af · outbound

This paper cites N., Boulet , T., Izidoro , A., Esteves , L., & Bitsch , B.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes N., Boulet , T., Izidoro , A., Esteves , L., & Bitsch , B

Reference 92

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T14:45:38.944972Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T14:45:38.538598Z digest=sha256:04a65669e232260b599638884b1c1222238dca543b65c5de90af5263b5a6a18c

Observation 94e6e29c-05ad-4e21-8131-7ea2097ef092 · outbound

This paper cites an unresolved cited work.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes Unresolved cited work

Reference 93

Resolution
unresolved
no resolver link, observed 2026-08-14T14:45:38.542127Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T14:45:38.542127Z digest=sha256:69a757fa55d8710e1e9ceaa9d6a6299d1543364b62263ea9494a8f0db18e11b9

Observation 7767ebca-4000-4434-bbfd-6bc6d53f305c · outbound

This paper cites an unresolved cited work.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes Unresolved cited work

Reference 94

Resolution
unresolved
no resolver link, observed 2026-08-14T14:45:38.545557Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T14:45:38.545557Z digest=sha256:0c6e8059641101b0096b63357e482d4237930b64c12eb2c6f4e06f80416b638a

Observation 866f8600-3090-443b-b7a5-de03a3de751a · outbound

This paper cites an unresolved cited work.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes Unresolved cited work

Reference 95

Resolution
unresolved
raw_fallback, observed 2026-08-14T14:45:38.917546Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T14:45:38.549004Z digest=sha256:1f3ba0a039d40de0152b97074ea6c3acab066afcc25e8c5a8aa700ab14e0b2af

Observation 4896440b-751c-4773-8a98-13035d0733e6 · outbound

This paper cites an unresolved cited work.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes Unresolved cited work

Reference 96

Resolution
unresolved
raw_fallback, observed 2026-08-14T14:45:38.903057Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T14:45:38.552329Z digest=sha256:811f418e88c2bc3b7c0a700c4323fb95d992bd611694bad03e03faf7b5c085fc

Observation 2b80fde0-31ba-4850-99dc-b1d4874bbdea · outbound

This paper cites 2015, , 799, 180.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes 2015, , 799, 180

Reference 97

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T14:45:38.890865Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T14:45:38.555640Z digest=sha256:fdabb093b08d78139028ded7f00be4924c896cdb0768bc2e7cc1917c874afabc

Observation b5703543-ce5f-4bef-9b9e-82727d234eb1 · outbound

This paper cites B., Armitage , P.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes B., Armitage , P

Reference 98

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T14:45:38.878940Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T14:45:38.559230Z digest=sha256:510a1732a3856413bda08ba62b17a7f4c78bd71cc70d4da97b2eb1cf7ccbdbe9

Observation b908cb5c-a1dd-4cb2-b14c-f5631f6b118c · outbound

This paper cites an unresolved cited work.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes Unresolved cited work

Reference 99

Resolution
unresolved
raw_fallback, observed 2026-08-14T14:45:38.865937Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T14:45:38.562910Z digest=sha256:43e91a8e1025f57681a9ee3b42b8ccfb43a24c16b7eb8966a1f3f6724ff85d81

Observation 687bcebc-1c22-4f55-b72d-a76e3a59e5e4 · outbound

This paper cites an unresolved cited work.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes Unresolved cited work

Reference 100

Resolution
unresolved
raw_fallback, observed 2026-08-14T14:45:38.853324Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-08-14T14:45:38.566241Z digest=sha256:a3b68bdd9e76304a5c030e2d6977341987ddef57d51d099e068bfd8f1956eb5f

Pith citing papers

No inbound Pith citation observations are available.