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Paper Citation Record · LEDGER

The effectively optically thin accretion flow and its implication in supermassive black holes

As of 17 August 2026, this Paper Citation Record lists 57 of 57 outbound references and 0 inbound Pith citation observations for arXiv:2506.22904.

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

pith.paper-citation-record.v1
2506.22904 v1

Coverage vector

measured 57 of 57 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-06T22:05:32.574200Z

measured 57 of 57 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00

measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

57 of 57 outbound references displayed

  • verified exact11
  • verified fuzzy8
  • unresolved37
  • parse uncertain0
  • malformed identifier0
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External citation measurements

No source-named external measurement is stored.

Outbound references

Observation b5399cdc-e5fe-41ce-acfb-6e66254700d3 · outbound

This paper cites an unresolved cited work.

The effectively optically thin accretion flow and its implication in supermassive black holes Unresolved cited work

Reference 1

Resolution
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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.

source=arxiv_source observed=2026-08-06T22:05:28.186401Z digest=sha256:5d45f3bfc626e78377960bd330cdd528acc8369743b2f9f382b8640f8185bc44

Observation 229f07f3-7554-49e6-857d-4f4b34cd43ad · outbound

This paper cites A., Czerny B., Lasota J.

The effectively optically thin accretion flow and its implication in supermassive black holes A., Czerny B., Lasota J

Reference 2

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no resolver link, observed 2026-08-06T22:05:28.235576Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T22:05:28.235576Z digest=sha256:f560731c161c40945d0247e9129f8861e3fa8f3fc0b0c32ec263d8975cf8cc92

Observation 3a41858f-564d-4ed5-8ad5-b2f62911bfc1 · outbound

This paper cites V., Bisnovatyi-Kogan G.

The effectively optically thin accretion flow and its implication in supermassive black holes V., Bisnovatyi-Kogan G

Reference 3

Resolution
verified exact
doi, observed 2026-08-06T22:05:34.631469Z

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.

source=arxiv_source observed=2026-08-06T22:05:28.267815Z digest=sha256:1ce9fb35d4f9d1ecc1bcf0aa6aeb3dbd7dfc1ffb0a01025d3cbaf7bf083f02e1

Observation c18bd860-403f-48b2-96fa-e5662ab11fd9 · outbound

This paper cites A., Chen X., Lasota J.-P., 1996, @doi [ ] 10.1086/177587 , https://ui.adsabs.harvard.edu/abs/1996ApJ...467...99B 467, 99.

The effectively optically thin accretion flow and its implication in supermassive black holes A., Chen X., Lasota J.-P., 1996, @doi [ ] 10.1086/177587 , https://ui.adsabs.harvard.edu/abs/1996ApJ...467...99B 467, 99

Reference 5

Resolution
verified exact
doi, observed 2026-08-06T22:05:34.438089Z

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.

source=arxiv_source observed=2026-08-06T22:05:28.383354Z digest=sha256:57a5b7258c513b0106591a676cc51ae8cbce6f641a2af99f56440bf2143f986b

Observation df5c000c-6fe5-49c7-b366-91bf27b43764 · outbound

This paper cites J., Blundell K.

The effectively optically thin accretion flow and its implication in supermassive black holes J., Blundell K

Reference 6

Resolution
unresolved
no resolver link, observed 2026-08-06T22:05:28.422570Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T22:05:28.422570Z digest=sha256:2afeece98e851e2c5c3add3ae5736d8eee05268a60ad2bf9a50f420c406101b0

Observation 33e5fc3b-0ee2-4dc6-bcc6-dc3945a12022 · outbound

This paper cites J., van de Hulst H.

The effectively optically thin accretion flow and its implication in supermassive black holes J., van de Hulst H

Reference 7

Resolution
verified exact
doi, observed 2026-08-06T22:05:34.310105Z

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.

source=arxiv_source observed=2026-08-06T22:05:28.488560Z digest=sha256:798653cbd0047ddbd9f307ceba2f7b0da603498191d23a0631507c85f765bd16

Observation 8cd95c1d-ca57-4c0f-b80c-7c66ebd9a0c1 · outbound

This paper cites S., 1977, , https://ui.adsabs.harvard.edu/abs/1977A&A....59..127C 59, 127.

The effectively optically thin accretion flow and its implication in supermassive black holes S., 1977, , https://ui.adsabs.harvard.edu/abs/1977A&A....59..127C 59, 127

Reference 8

Resolution
verified fuzzy
raw_fallback, observed 2026-08-06T22:05:36.375676Z

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.

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Observation f4332683-b39b-4055-b0c4-2c2a5bd93cad · outbound

This paper cites New York: Dover.

The effectively optically thin accretion flow and its implication in supermassive black holes New York: Dover

Reference 9

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verified fuzzy
raw_fallback, observed 2026-08-06T22:05:36.163097Z

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.

source=arxiv_source observed=2026-08-06T22:05:28.569488Z digest=sha256:fca33c10c8ef8769a097e488c42d9c3afd45587fdea7ec08430b517da1128634

Observation afa9a741-bb04-485a-ae1c-80b4e32a9275 · outbound

This paper cites an unresolved cited work.

The effectively optically thin accretion flow and its implication in supermassive black holes Unresolved cited work

Reference 10

Resolution
unresolved
no resolver link, observed 2026-08-06T22:05:28.636286Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T22:05:28.636286Z digest=sha256:b2623b27a53763f5d99ded90af6a3799e90f37c97c232438257035eec57617d9

Observation 56deacce-0286-4b2c-aad1-5ef53f2d3922 · outbound

This paper cites A., Lasota J.-P., Narayan R., Yi I., 1995, @doi [ ] 10.1086/187836 , https://ui.adsabs.harvard.edu/abs/1995ApJ...443L..61C 443, L61.

The effectively optically thin accretion flow and its implication in supermassive black holes A., Lasota J.-P., Narayan R., Yi I., 1995, @doi [ ] 10.1086/187836 , https://ui.adsabs.harvard.edu/abs/1995ApJ...443L..61C 443, L61

Reference 11

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doi, observed 2026-08-06T22:05:34.187683Z

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.

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Observation 00fd72fc-6b5b-4673-9911-98d6f73069bf · outbound

This paper cites D., 1983, Principles of stellar evolution and nucleosynthesis.

The effectively optically thin accretion flow and its implication in supermassive black holes D., 1983, Principles of stellar evolution and nucleosynthesis

Reference 12

Resolution
verified fuzzy
raw_fallback, observed 2026-08-06T22:05:35.922711Z

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.

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Observation 9d749973-df36-4bf7-861b-1086457b73e0 · outbound

This paper cites C., Gallo L., Ross R.

The effectively optically thin accretion flow and its implication in supermassive black holes C., Gallo L., Ross R

Reference 13

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no resolver link, observed 2026-08-06T22:05:28.715077Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T22:05:28.715077Z digest=sha256:b113c7e9b7dfadeeb59a7ab60d3919c44cbc19ea0c47290de408e8ab604415be

Observation cc0a1e8b-fbc7-42bd-acfa-80ac0a07f579 · outbound

This paper cites an unresolved cited work.

The effectively optically thin accretion flow and its implication in supermassive black holes Unresolved cited work

Reference 14

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unresolved
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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T22:05:28.765240Z digest=sha256:5d14b7e6e3cd03f5d287597695d042cbba1e68005a5b08fc4128e3118e474ce0

Observation 74c5b3bb-11ce-407d-b560-3b42998fd0d2 · outbound

This paper cites D., Liang E.

The effectively optically thin accretion flow and its implication in supermassive black holes D., Liang E

Reference 15

Resolution
unresolved
no resolver link, observed 2026-08-06T22:05:28.799101Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T22:05:28.799101Z digest=sha256:f539f63372d553f5e5271b9e1c8b18c0929851baedef33e4e2c05bef0f2b3b42

Observation 074b6865-e84f-4b86-9cd8-b2be9a098167 · outbound

This paper cites W., Jin C., Blaes O., Ward M., 2012, @doi [ ] 10.1111/j.1365-2966.2011.19779.x , https://ui.adsabs.harvard.edu/abs/2012MNRAS.420.1848D 420, 1848.

The effectively optically thin accretion flow and its implication in supermassive black holes W., Jin C., Blaes O., Ward M., 2012, @doi [ ] 10.1111/j.1365-2966.2011.19779.x , https://ui.adsabs.harvard.edu/abs/2012MNRAS.420.1848D 420, 1848

Reference 16

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Unavailable: canonical work link unavailable.

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Observation 15985323-a03f-4f78-b155-76119af40bea · outbound

This paper cites an unresolved cited work.

The effectively optically thin accretion flow and its implication in supermassive black holes Unresolved cited work

Reference 17

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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 84baeb48-5526-42d4-95f3-abe6464524c2 · outbound

This paper cites J., 2002, Accretion Power in Astrophysics: Third Edition.

The effectively optically thin accretion flow and its implication in supermassive black holes J., 2002, Accretion Power in Astrophysics: Third Edition

Reference 18

Resolution
verified fuzzy
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Source-reported events for the cited work

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

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Observation 7fb0f419-672e-4b4f-9b16-54b149239127 · outbound

This paper cites an unresolved cited work.

The effectively optically thin accretion flow and its implication in supermassive black holes Unresolved cited work

Reference 19

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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 034231f7-2525-44f7-98ef-031a54e5ebd5 · outbound

This paper cites an unresolved cited work.

The effectively optically thin accretion flow and its implication in supermassive black holes Unresolved cited work

Reference 20

Resolution
verified exact
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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.

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Observation 38bbc106-46b2-491a-b5e9-550553ba7680 · outbound

This paper cites an unresolved cited work.

The effectively optically thin accretion flow and its implication in supermassive black holes Unresolved cited work

Reference 21

Resolution
unresolved
no resolver link, observed 2026-08-06T22:05:29.228641Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation b272fdd2-1cf0-435d-a4d1-c85b2c2aa260 · outbound

This paper cites an unresolved cited work.

The effectively optically thin accretion flow and its implication in supermassive black holes Unresolved cited work

Reference 22

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T22:05:29.254810Z digest=sha256:7c2594f99a009b44f0f82d73c7e27a5107271c4ecee186c4756975bd00438865

Observation 89acefb2-f838-47ea-b74d-233064307fdd · outbound

This paper cites an unresolved cited work.

The effectively optically thin accretion flow and its implication in supermassive black holes Unresolved cited work

Reference 23

Resolution
verified exact
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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.

source=arxiv_source observed=2026-08-06T22:05:29.305706Z digest=sha256:926aea4149a9c9c7d12ed8613c99a0bf6795ccc528a197060ad7d09aa8f936c0

Observation 5639ded9-2c6c-4127-b2c9-7972b183a92d · outbound

This paper cites an unresolved cited work.

The effectively optically thin accretion flow and its implication in supermassive black holes Unresolved cited work

Reference 24

Resolution
verified exact
doi, observed 2026-08-06T22:05:33.801233Z

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.

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Observation 64cb2a4a-7d1c-4daa-8bc1-2fbb1e4b0fbc · outbound

This paper cites P., 2017, @doi [ ] 10.1146/annurev-astro-091916-055259 , https://ui.adsabs.harvard.edu/abs/2017ARA&A..55..303K 55, 303.

The effectively optically thin accretion flow and its implication in supermassive black holes P., 2017, @doi [ ] 10.1146/annurev-astro-091916-055259 , https://ui.adsabs.harvard.edu/abs/2017ARA&A..55..303K 55, 303

Reference 25

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source=arxiv_source observed=2026-08-06T22:05:29.509600Z digest=sha256:4c4cb9fce833ab4acc24932c1e0bbe26f3c45916e4bfbe0fa89b0221c0c6a37e

Observation 264d2ebb-267f-47d4-9576-6f2e41af0c1e · outbound

This paper cites Kyoto University Press.

The effectively optically thin accretion flow and its implication in supermassive black holes Kyoto University Press

Reference 26

Resolution
verified fuzzy
raw_fallback, observed 2026-08-06T22:05:35.689443Z

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.

source=arxiv_source observed=2026-08-06T22:05:29.671543Z digest=sha256:00693864723cc62de2030fdb255c00e2243fb192d5caeb22f0465812965dc9a6

Observation 6c79662c-f607-4375-b49f-56ea397e71e2 · outbound

This paper cites I., 1977, @doi [ ] 10.1086/155355 , https://ui.adsabs.harvard.edu/abs/1977ApJ...215..265K 215, 265.

The effectively optically thin accretion flow and its implication in supermassive black holes I., 1977, @doi [ ] 10.1086/155355 , https://ui.adsabs.harvard.edu/abs/1977ApJ...215..265K 215, 265

Reference 27

Resolution
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no resolver link, observed 2026-08-06T22:05:29.759040Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 79922702-e7f0-4f3b-8143-c6504c40ca8d · outbound

This paper cites R., Pringle J.

The effectively optically thin accretion flow and its implication in supermassive black holes R., Pringle J

Reference 28

Resolution
unresolved
no resolver link, observed 2026-08-06T22:05:29.857349Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T22:05:29.857349Z digest=sha256:e2dbd2b49a5a62e1c335e221fe503e7531fe53c507a30705cdb3c5e809113016

Observation fbfa850a-c4ae-41f2-8d1f-d53247bedd7b · outbound

This paper cites S., Bisnovatyi-Kogan G.

The effectively optically thin accretion flow and its implication in supermassive black holes S., Bisnovatyi-Kogan G

Reference 29

Resolution
verified exact
doi, observed 2026-08-06T22:05:33.649511Z

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.

source=arxiv_source observed=2026-08-06T22:05:29.927320Z digest=sha256:319f2bdd26612c60b40b62ed6c31c94fce7af104a8d0be34ba9a53c3153e5837

Observation 818e155f-243f-4fce-bee4-66c027e207c4 · outbound

This paper cites C., Ricci C., Trakhtenbrot B., 2024a, @doi [ ] 10.3847/1538-4357/ad77a5 , https://ui.adsabs.harvard.edu/abs/2024ApJ...975...50L 975, 50.

The effectively optically thin accretion flow and its implication in supermassive black holes C., Ricci C., Trakhtenbrot B., 2024a, @doi [ ] 10.3847/1538-4357/ad77a5 , https://ui.adsabs.harvard.edu/abs/2024ApJ...975...50L 975, 50

Reference 30

Resolution
unresolved
no resolver link, observed 2026-08-06T22:05:30.012560Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T22:05:30.012560Z digest=sha256:15e758d04fa5c4a8912d1849952b4fb1c354afa6be1442efb8ac5af1fe2564f4

Observation c028e2b7-4c4d-46f8-8e20-722c58f725f5 · outbound

This paper cites C., Trakhtenbrot B., Kara E., Masterson M., Arcavi I., 2024b, @doi [ ] 10.3847/1538-4357/ad7aed , https://ui.adsabs.harvard.edu/abs/2024ApJ...975..140L 975, 140.

The effectively optically thin accretion flow and its implication in supermassive black holes C., Trakhtenbrot B., Kara E., Masterson M., Arcavi I., 2024b, @doi [ ] 10.3847/1538-4357/ad7aed , https://ui.adsabs.harvard.edu/abs/2024ApJ...975..140L 975, 140

Reference 31

Resolution
unresolved
no resolver link, observed 2026-08-06T22:05:30.082503Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T22:05:30.082503Z digest=sha256:ec4cdd182f1e1f5b19d066d795fc9691cd5653834d8891b452b648f18ae98b75

Observation 00ace82e-84a1-4a4b-b0c9-39f84bac10f6 · outbound

This paper cites P., Nolan P.

The effectively optically thin accretion flow and its implication in supermassive black holes P., Nolan P

Reference 32

Resolution
verified exact
doi, observed 2026-08-06T22:05:33.439888Z

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.

source=arxiv_source observed=2026-08-06T22:05:30.218400Z digest=sha256:0a91f388054c2bd8e6696d3430adf68752cbc3d867326792dc2a91effebd7dbb

Observation 6fbde92e-3425-4179-a43b-9a2129e3739f · outbound

This paper cites P., Shapiro S.

The effectively optically thin accretion flow and its implication in supermassive black holes P., Shapiro S

Reference 33

Resolution
verified exact
doi, observed 2026-08-06T22:05:33.280955Z

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.

source=arxiv_source observed=2026-08-06T22:05:30.339892Z digest=sha256:315c13ac5b7e0a67ac1c5bbe529ad488a59d967c145d911602f828617e7db792

Observation c7f60493-97c1-4d9d-a69c-310de4b7b15e · outbound

This paper cites F., Wang Y., Cheng H., Yuan W., 2025, @doi [ ] 10.1093/mnras/staf459 , https://ui.adsabs.harvard.edu/abs/2025MNRAS.tmp..440L.

The effectively optically thin accretion flow and its implication in supermassive black holes F., Wang Y., Cheng H., Yuan W., 2025, @doi [ ] 10.1093/mnras/staf459 , https://ui.adsabs.harvard.edu/abs/2025MNRAS.tmp..440L

Reference 34

Resolution
unresolved
no resolver link, observed 2026-08-06T22:05:30.415185Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T22:05:30.415185Z digest=sha256:cedb29015192320d4970254d61c309207abe0c95a48e4b6b3fea608354131898

Observation f1fc6715-72ae-43a2-bfa7-2d13dcc3164e · outbound

This paper cites M., Zdziarski A.

The effectively optically thin accretion flow and its implication in supermassive black holes M., Zdziarski A

Reference 35

Resolution
unresolved
no resolver link, observed 2026-08-06T22:05:30.509354Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T22:05:30.509354Z digest=sha256:757dd38b35f378d7ff2196225a286aecfc5b8fa24ebf26396098e8bc81ee801c

Observation 477d41bf-3b0f-44d0-84a3-dbc6b4f89548 · outbound

This paper cites A., 1983, @doi [ ] 10.1086/160981 , https://ui.adsabs.harvard.edu/abs/1983ApJ...268..582M 268, 582.

The effectively optically thin accretion flow and its implication in supermassive black holes A., 1983, @doi [ ] 10.1086/160981 , https://ui.adsabs.harvard.edu/abs/1983ApJ...268..582M 268, 582

Reference 36

Resolution
unresolved
no resolver link, observed 2026-08-06T22:05:30.650506Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T22:05:30.650506Z digest=sha256:c20bff6a76641641a5f7420b389adae214359a72ecbb58abe3a585c49cb81e61

Observation 489b506e-2b43-4e22-a531-81124a3d2ea9 · outbound

This paper cites A., Sargent W.

The effectively optically thin accretion flow and its implication in supermassive black holes A., Sargent W

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-06T22:05:30.785853Z

Source-reported events for the cited work

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source=arxiv_source observed=2026-08-06T22:05:30.785853Z digest=sha256:03dbd12a9fec652d82afcf050a325d99e0dbd91eb8530c53d0c890a27be8b714

Observation 2918219d-831b-4887-b25f-f6853f07a7ce · outbound

This paper cites an unresolved cited work.

The effectively optically thin accretion flow and its implication in supermassive black holes Unresolved cited work

Reference 38

Resolution
unresolved
no resolver link, observed 2026-08-06T22:05:30.920113Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T22:05:30.920113Z digest=sha256:463c78a2a87c5699babbba37505fe9bf6893af7dffd775d0f09a6f4e68f35e7d

Observation b474bf07-c5fb-4985-b1c4-f1e91a3034b0 · outbound

This paper cites R., van den Oord G.

The effectively optically thin accretion flow and its implication in supermassive black holes R., van den Oord G

Reference 39

Resolution
unresolved
no resolver link, observed 2026-08-06T22:05:31.004271Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T22:05:31.004271Z digest=sha256:3df78c77ef5be23e4efb130cc0aadeb4230ee6f9e0a48612e48440cb6354ba8e

Observation 381184eb-a16a-44aa-87d9-5c2aacbab42d · outbound

This paper cites W., 1984, Foundations of radiation hydrodynamics.

The effectively optically thin accretion flow and its implication in supermassive black holes W., 1984, Foundations of radiation hydrodynamics

Reference 40

Resolution
verified fuzzy
raw_fallback, observed 2026-08-06T22:05:35.509804Z

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.

source=arxiv_source observed=2026-08-06T22:05:31.092090Z digest=sha256:47ff13906c911bb9ab5a0baf97d4f91e2750b47497ae404f3a7dae3309668e57

Observation 271e4eb3-4569-49ca-ae25-9332c26b04b4 · outbound

This paper cites an unresolved cited work.

The effectively optically thin accretion flow and its implication in supermassive black holes Unresolved cited work

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-06T22:05:31.166556Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T22:05:31.166556Z digest=sha256:51ab9067e910ff3e575fa4c7bc3dbae955283500ccf5a897179682e684f00c2e

Observation 2a2bf57e-84a1-44fb-9f4f-e07daf02229f · outbound

This paper cites an unresolved cited work.

The effectively optically thin accretion flow and its implication in supermassive black holes Unresolved cited work

Reference 42

Resolution
unresolved
no resolver link, observed 2026-08-06T22:05:31.225077Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T22:05:31.225077Z digest=sha256:25535cd99f468d650d0eec26e171a4c485c26e75145b671ee368984c575d83db

Observation 915ebe0d-9de7-4efd-bb2b-7a735869a569 · outbound

This paper cites D., Thorne K.

The effectively optically thin accretion flow and its implication in supermassive black holes D., Thorne K

Reference 43

Resolution
unresolved
no resolver link, observed 2026-08-06T22:05:31.314779Z

Source-reported events for the cited work

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source=arxiv_source observed=2026-08-06T22:05:31.314779Z digest=sha256:4ef58762cf0650cb43d47808cbc871a74c69b1cfbbccbc515f1ee15721f51751

Observation 84c03b8d-2c46-4c51-a620-c5cb0013bc38 · outbound

This paper cites O., et al., 2013, @doi [ ] 10.1051/0004-6361/201219956 , https://ui.adsabs.harvard.edu/abs/2013A&A...549A..73P 549, A73.

The effectively optically thin accretion flow and its implication in supermassive black holes O., et al., 2013, @doi [ ] 10.1051/0004-6361/201219956 , https://ui.adsabs.harvard.edu/abs/2013A&A...549A..73P 549, A73

Reference 44

Resolution
unresolved
no resolver link, observed 2026-08-06T22:05:31.394890Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T22:05:31.394890Z digest=sha256:80b983a78656371c930a9e836d3273a631b9b603a78abc34cf1def8648a8c193

Observation b3c7b362-0185-485e-a0a3-24126cf5fd6d · outbound

This paper cites an unresolved cited work.

The effectively optically thin accretion flow and its implication in supermassive black holes Unresolved cited work

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-06T22:05:31.481863Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T22:05:31.481863Z digest=sha256:0aecd808b8a41325370423e5331734b4337c5ccb2bc4526637a0a3e5916612dd

Observation 1b820b97-138e-4cce-8a94-a9ade4dd403e · outbound

This paper cites J., 1988, @doi [ ] 10.1038/333523a0 , https://ui.adsabs.harvard.edu/abs/1988Natur.333..523R 333, 523.

The effectively optically thin accretion flow and its implication in supermassive black holes J., 1988, @doi [ ] 10.1038/333523a0 , https://ui.adsabs.harvard.edu/abs/1988Natur.333..523R 333, 523

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-06T22:05:31.569613Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T22:05:31.569613Z digest=sha256:c3a4ef52603df0aceefaf5613d76232cdc30b0db7e785ead0b5571708c006307

Observation 0ba1eb17-5092-45f6-a878-62e25cf0e4a3 · outbound

This paper cites Broadband reflection spectroscopy of MAXI J1535-571 using AstroSat: Estimation of black hole mass and spin.

The effectively optically thin accretion flow and its implication in supermassive black holes Broadband reflection spectroscopy of MAXI J1535-571 using AstroSat: Estimation of black hole mass and spin

Reference 47

Resolution
unresolved
no resolver link, observed 2026-08-06T22:05:31.699757Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T22:05:31.699757Z digest=sha256:91a4be305bb9c557150b23299d21cf4d9ac7819004453eee7dad38817b9fb5d3

Observation ff239251-1f2f-4521-81be-8b8f039e5738 · outbound

This paper cites B., Lightman A.

The effectively optically thin accretion flow and its implication in supermassive black holes B., Lightman A

Reference 48

Resolution
verified fuzzy
raw_fallback, observed 2026-08-06T22:05:35.363022Z

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.

source=arxiv_source observed=2026-08-06T22:05:31.788596Z digest=sha256:1d351894da00409cdf1a93dbbc899490fa8a3c7c52a7adcc41cc98675877317b

Observation 09dac6dd-5930-4b26-8592-a00187af7a02 · outbound

This paper cites J., Coroniti F.

The effectively optically thin accretion flow and its implication in supermassive black holes J., Coroniti F

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-06T22:05:31.874962Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T22:05:31.874962Z digest=sha256:3d628058fee26b66f4ebab1367f69ad10648f4dd85c0b6d66bd6f3ce7c27a166

Observation 12bacd63-4f89-4322-b1f4-a87636aa3258 · outbound

This paper cites I., Sunyaev R.

The effectively optically thin accretion flow and its implication in supermassive black holes I., Sunyaev R

Reference 50

Resolution
unresolved
no resolver link, observed 2026-08-06T22:05:31.984847Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T22:05:31.984847Z digest=sha256:0459e84027ebef59c683fd3428d62690550840227dfd347aa581e8e160cd8612

Observation 1a62c2f6-2411-4e9e-92ea-11010b31ce46 · outbound

This paper cites L., Lightman A.

The effectively optically thin accretion flow and its implication in supermassive black holes L., Lightman A

Reference 51

Resolution
unresolved
no resolver link, observed 2026-08-06T22:05:32.043329Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T22:05:32.043329Z digest=sha256:add3aef305c666ed40ba6728a7eddca27841f76b2562b2c5160c80548718f3bb

Observation 59cdaaf8-987f-4c10-bb4e-b4f62083cc5d · outbound

This paper cites Characteristic temperatures and spectral appearance of ULX disks.

The effectively optically thin accretion flow and its implication in supermassive black holes Characteristic temperatures and spectral appearance of ULX disks

Reference 52

Resolution
metadata mismatch
local_arxiv, observed 2026-08-06T22:05:33.042730Z

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.

source=arxiv_source observed=2026-08-06T22:05:32.099272Z digest=sha256:d47da8ee075473c9907b81a276d8d655767bab11573e7c92bec97ecbdc260184

Observation b326fee6-3188-4f1b-ac30-4b57b93b955b · outbound

This paper cites A., Titarchuk L.

The effectively optically thin accretion flow and its implication in supermassive black holes A., Titarchuk L

Reference 53

Resolution
verified fuzzy
raw_fallback, observed 2026-08-06T22:05:35.210985Z

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.

source=arxiv_source observed=2026-08-06T22:05:32.209202Z digest=sha256:9ead1a802488bd97f5ed1243b41b9998fa1833d3506d64b0ebb1f6da9ec4a0fd

Observation c90f8a5e-f4e3-4e34-8d77-77e4efed1e70 · outbound

This paper cites S., Price R.

The effectively optically thin accretion flow and its implication in supermassive black holes S., Price R

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-06T22:05:32.274484Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T22:05:32.274484Z digest=sha256:6de576bc73ee93dbb19d5550a0971ce8289b7252f50146e2e5aae094c28806d4

Observation ff84a473-d8c0-44cc-a0ad-fbbae5d97dc4 · outbound

This paper cites J., Nardini E., Fabian A.

The effectively optically thin accretion flow and its implication in supermassive black holes J., Nardini E., Fabian A

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-06T22:05:32.352324Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T22:05:32.352324Z digest=sha256:b69f76d62572a396fd14cb8d98ce027ed284f38a3b47622b725db40f9fe0d2c9

Observation 41666314-99f9-4317-9b59-bab311421b6b · outbound

This paper cites an unresolved cited work.

The effectively optically thin accretion flow and its implication in supermassive black holes Unresolved cited work

Reference 56

Resolution
verified exact
doi, observed 2026-08-06T22:05:32.894900Z

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.

source=arxiv_source observed=2026-08-06T22:05:32.442344Z digest=sha256:4f56e3fdfcc65ec86ba752ff3e651300913140d7fc44c0f09c1c7c914fa1a436

Observation da4d0f29-9b45-4d17-b9b8-c8764ad16c30 · outbound

This paper cites G., Stone N.

The effectively optically thin accretion flow and its implication in supermassive black holes G., Stone N

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-06T22:05:32.499518Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T22:05:32.499518Z digest=sha256:eb98ef2ecb442f2cd25ad808e050cbf5bbc2d60ec5f13fc6cc309b3358a82474

Observation 04ec1fff-45a6-49d0-abc0-f9a9c11bb65e · outbound

This paper cites C., Gallo L.

The effectively optically thin accretion flow and its implication in supermassive black holes C., Gallo L

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-06T22:05:32.574200Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T22:05:32.574200Z digest=sha256:e878b8ad49027fbdacd3cc1cb8fb590f9ad3d2391f471aad10d376e6b831760e

Pith citing papers

No inbound Pith citation observations are available.