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Paper Citation Record · LEDGER

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff

As of 10 August 2026, this Paper Citation Record lists 68 of 68 outbound references and 1 inbound Pith citation observation for arXiv:2605.07976.

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

pith.paper-citation-record.v1
2605.07976 v1

Coverage vector

measured 68 of 68 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-05-11T03:11:10.401986Z

measured 69 of 69 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-06-28T00:23:19.443839Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

68 of 68 outbound references displayed

  • verified exact10
  • verified fuzzy46
  • unresolved8
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External citation measurements

0
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

Observation ac29994d-4e99-4608-8ad2-74c7de3b376c · outbound

This paper cites B., Casey, C.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff B., Casey, C

Reference 1

Resolution
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Observation d8468d69-c21f-405b-94a8-afc7e9f250a9 · outbound

This paper cites Origins of the UV continuum and Balmer emission lines in Little Red Dots: observational validation of dense gas envelope models enshrouding the AGN.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff Origins of the UV continuum and Balmer emission lines in Little Red Dots: observational validation of dense gas envelope models enshrouding the AGN

Reference 2

Resolution
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arxiv_id, observed 2026-05-12T02:44:56.814185Z

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Observation f1a1f491-d36f-404d-8a28-cdd853e6d3aa · outbound

This paper cites Connecting the Dots: UV-Bright Companions of Little Red Dots as Lyman-Werner Sources Enabling Direct Collapse Black Hole Formation.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff Connecting the Dots: UV-Bright Companions of Little Red Dots as Lyman-Werner Sources Enabling Direct Collapse Black Hole Formation

Reference 3

Resolution
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Source-reported events for the cited work

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Observation 800a9f92-e0e8-4d3d-a9d1-43118ce3d734 · outbound

This paper cites an unresolved cited work.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff Unresolved cited work

Reference 4

Resolution
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Source-reported events for the cited work

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Observation 0a351b7b-4018-416e-a5c9-1463c6775db1 · outbound

This paper cites an unresolved cited work.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff Unresolved cited work

Reference 5

Resolution
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Source-reported events for the cited work

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Observation 8e641f4a-3b81-4089-a18d-eae42cc60269 · outbound

This paper cites G., Kocevski, D., et al.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff G., Kocevski, D., et al

Reference 6

Resolution
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arxiv_id, observed 2026-05-11T03:15:55.112530Z

Source-reported events for the cited work

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Observation 21c4656d-d62e-41e6-9a00-f407a4b4945e · outbound

This paper cites G., Kocevski, D.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff G., Kocevski, D

Reference 7

Resolution
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Source-reported events for the cited work

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Observation 9404a124-f2cd-4850-8e37-8a582a8d22c1 · outbound

This paper cites 2026, A&A, 706, A29.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff 2026, A&A, 706, A29

Reference 8

Resolution
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Source-reported events for the cited work

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Observation a913bdfb-87f5-4b06-b918-73029c61b333 · outbound

This paper cites & Valentino, F.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff & Valentino, F

Reference 9

Resolution
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Observation 03e93302-2d93-460c-ae24-6eb24e90dd3c · outbound

This paper cites C., et al.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff C., et al

Reference 10

Resolution
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Observation 4326e932-6dd2-47c5-82cc-c34204361338 · outbound

This paper cites C., McLure, R.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff C., McLure, R

Reference 11

Resolution
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Observation 77b12694-8b81-4b94-a050-31ea60566263 · outbound

This paper cites M., Akins, H.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff M., Akins, H

Reference 12

Resolution
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Source-reported events for the cited work

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Observation 7f20bd90-582a-4213-844e-499e4b715207 · outbound

This paper cites M., Akins, H.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff M., Akins, H

Reference 13

Resolution
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Source-reported events for the cited work

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Observation 1d14da8f-e77a-4387-bd39-a588af950426 · outbound

This paper cites 2003, PASP, 115, 763.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff 2003, PASP, 115, 763

Reference 14

Resolution
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Source-reported events for the cited work

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Observation 65ffcde6-8b1c-4a3e-8f55-d10228b9a531 · outbound

This paper cites P., Whitaker, K.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff P., Whitaker, K

Reference 15

Resolution
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Source-reported events for the cited work

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Observation 8d8baedc-83a5-473b-a65f-4b369b1f79de · outbound

This paper cites J., Chatzikos, M., Guzmán, F., et al.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff J., Chatzikos, M., Guzmán, F., et al

Reference 16

Resolution
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Source-reported events for the cited work

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Observation 2d9ed624-d8c1-4815-bea4-5a32583151c9 · outbound

This paper cites 2024, A&A, 684, A207.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff 2024, A&A, 684, A207

Reference 17

Resolution
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Observation b7813b6c-6469-4c11-8c87-178974be791b · outbound

This paper cites J., Secunda, A.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff J., Secunda, A

Reference 18

Resolution
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Observation c30b990f-dddd-4db3-ae88-afcd0b808e10 · outbound

This paper cites D., Clayton, G.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff D., Clayton, G

Reference 19

Resolution
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Observation 1efb6051-e5d6-492c-90de-ce053ef05909 · outbound

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Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff Unresolved cited work

Reference 20

Resolution
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Source-reported events for the cited work

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Observation 490da211-150c-4ad5-8289-834bde987e4a · outbound

This paper cites E., Labbe, I., Goulding, A.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff E., Labbe, I., Goulding, A

Reference 21

Resolution
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Observation 52925120-cd64-440d-92f4-45f08c17ca68 · outbound

This paper cites A., Pacucci, F., & Kocevski, D.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff A., Pacucci, F., & Kocevski, D

Reference 22

Resolution
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Observation d6de1353-f31a-45b0-bc1f-d4dee8b60d70 · outbound

This paper cites E., de Graaff, A., Miller, T.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff E., de Graaff, A., Miller, T

Reference 23

Resolution
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Source-reported events for the cited work

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Observation 61020cbd-8b3c-42bc-aa46-f33ecd9331a0 · outbound

This paper cites 2025, ApJ, 988, L22.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff 2025, ApJ, 988, L22

Reference 24

Resolution
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Observation bd175d8e-8a8d-4574-b6a6-b7423115f581 · outbound

This paper cites & Maiolino, R.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff & Maiolino, R

Reference 25

Resolution
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Observation 6c6dfb14-3e64-41e6-8a2f-ed078b88a2f3 · outbound

This paper cites 2026, ApJ, 1000, 90.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff 2026, ApJ, 1000, 90

Reference 26

Resolution
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Observation f972b9ad-78ea-461d-8300-4f7b08b66948 · outbound

This paper cites The Emergence of Little Red Dots from Binary Massive Black Holes.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff The Emergence of Little Red Dots from Binary Massive Black Holes

Reference 27

Resolution
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Source-reported events for the cited work

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Observation 6d320a91-22b0-463f-8c04-6e8a110d7815 · outbound

This paper cites 2022, A&A, 661, A80.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff 2022, A&A, 661, A80

Reference 28

Resolution
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

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Observation 25e65925-52d4-4318-b2e1-6b85d8c5e9ab · outbound

This paper cites 2026, MNRAS, 545, staf2235.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff 2026, MNRAS, 545, staf2235

Reference 29

Resolution
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Observation 32248349-18ec-4b97-be14-f7b5e2dd9134 · outbound

This paper cites 2025, MNRAS, 544.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff 2025, MNRAS, 544

Reference 30

Resolution
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Observation f693dcfa-2eff-45ba-8329-2be55a884cb9 · outbound

This paper cites A direct black hole mass measurement in a Little Red Dot at the Epoch of Reionization.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff A direct black hole mass measurement in a Little Red Dot at the Epoch of Reionization

Reference 31

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Observation 89d1e9a4-d5e9-46e2-a038-fdfc2a9d25d5 · outbound

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Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff Unresolved cited work

Reference 32

Resolution
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

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Observation cd96beee-c11c-40c3-97b6-b16e0c9e144f · outbound

This paper cites an unresolved cited work.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff Unresolved cited work

Reference 33

Resolution
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

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Observation 6fafad7d-379b-4a72-8407-8abf833d53eb · outbound

This paper cites D., Finkelstein, S.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff D., Finkelstein, S

Reference 34

Resolution
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raw_fallback, observed 2026-05-14T10:54:13.662135Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T03:11:10.401986Z digest=sha256:2301d4e77db9979a2d8c3b8b8961373ce609223aa20b1496e2c788a4d7652812

Observation b589eb7b-8a86-41b8-a33b-5e464f237344 · outbound

This paper cites & Harikane, Y.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff & Harikane, Y

Reference 35

Resolution
verified fuzzy
raw_fallback, observed 2026-05-14T10:59:15.447461Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T03:11:10.401986Z digest=sha256:43f4aa089232a99ebb77bb95def5285473b68ba8760ca86e5a57194c65f5c1be

Observation 42f19a4b-a052-432d-ab63-ab1609882a63 · outbound

This paper cites GLIMPSED: Direct evidence for a fast AGN-driven outflow from a z=6.64 Little Red Dot host galaxy.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff GLIMPSED: Direct evidence for a fast AGN-driven outflow from a z=6.64 Little Red Dot host galaxy

Reference 36

Resolution
metadata mismatch
local_arxiv, observed 2026-05-11T03:15:55.118062Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T03:11:10.401986Z digest=sha256:d96042f3f5e1bd8b526ae072d9b04d6bb71340a108f9866e0352e5231f3c03ca

Observation 8707d830-1b04-4c19-9390-e99c996cc557 · outbound

This paper cites E., Bezanson, R., et al.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff E., Bezanson, R., et al

Reference 37

Resolution
verified fuzzy
raw_fallback, observed 2026-05-14T10:54:13.663565Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T03:11:10.401986Z digest=sha256:45ee4fbccfb448d31015d4625aa933fd637cbe3c8b95f6fde04893d3604d2414

Observation dbc2ae48-aba8-4e93-9cbd-f5d4b6e46ab8 · outbound

This paper cites An unambiguous AGN and a Balmer break in an Ultraluminous Little Red Dot at z=4.47 from Ultradeep UNCOVER and All the Little Things Spectroscopy.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff An unambiguous AGN and a Balmer break in an Ultraluminous Little Red Dot at z=4.47 from Ultradeep UNCOVER and All the Little Things Spectroscopy

Reference 38

Resolution
verified exact
arxiv_id, observed 2026-05-11T03:15:55.106282Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T03:11:10.401986Z digest=sha256:ed745cfeb8161eb04752d88e298c469832a419c29303d39c5f423406b5e78c4e

Observation 1e858bf4-90eb-4818-9fa8-404a8c63490c · outbound

This paper cites C., Johnson, B.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff C., Johnson, B

Reference 39

Resolution
verified fuzzy
raw_fallback, observed 2026-05-14T10:54:13.665061Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T03:11:10.401986Z digest=sha256:66bc0a5f0fd2db3185044940abdc95da11aa10f3706f8976b0c35d7d69195252

Observation 9c551d92-d0d3-4dfd-b03b-71b5ebddf3fa · outbound

This paper cites 2023, ApJ, 950, 85.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff 2023, ApJ, 950, 85

Reference 40

Resolution
verified fuzzy
raw_fallback, observed 2026-05-14T10:59:15.449534Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T03:11:10.401986Z digest=sha256:bd443e632cbff2b9244186c023a7f2d87394cde9822b99cfe41a19876e1108e5

Observation e5d0b37e-3e6c-4278-b708-1089b129ae8c · outbound

This paper cites 2025, ApJ, 980, L34.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff 2025, ApJ, 980, L34

Reference 41

Resolution
verified fuzzy
raw_fallback, observed 2026-05-14T10:59:15.436275Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T03:11:10.401986Z digest=sha256:e6d4d4efdac97b3df3106ac02a60783ee0167e208a6ead2e6dc34319e2419c80

Observation b4dcb9e7-2986-4b93-9184-86d559e5f6fa · outbound

This paper cites 2024, A&A, 689, A128.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff 2024, A&A, 689, A128

Reference 42

Resolution
verified fuzzy
raw_fallback, observed 2026-05-14T10:59:15.433324Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T03:11:10.401986Z digest=sha256:46fc3fce3056c53338d7997aad0223e7bf8534665a823af3537e981e6fc163af

Observation 2e32c8f8-89cb-4416-9a5c-992d47d2b8ce · outbound

This paper cites E., Setton, D.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff E., Setton, D

Reference 43

Resolution
verified fuzzy
raw_fallback, observed 2026-05-14T10:59:15.461186Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T03:11:10.401986Z digest=sha256:a3ba4b4b2d5e78d21441a6290434343fe26af0878e4001f4e1cbed2f7d836a06

Observation 1d6ef0ff-2191-4130-9178-f1b7df5f8ff8 · outbound

This paper cites 2014, ApJ, 784, L38.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff 2014, ApJ, 784, L38

Reference 44

Resolution
verified fuzzy
raw_fallback, observed 2026-05-14T10:59:15.445380Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T03:11:10.401986Z digest=sha256:a0f034542e5d3c10181a7bcd7794a346b7cfa501e267d9bec84cc8c9913ce420

Observation d69bd229-65a3-4b00-ab68-ecf092ffac6f · outbound

This paper cites Little Red Dots as Obscured Little Blue Dots: A Super-Eddington Unification Model.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff Little Red Dots as Obscured Little Blue Dots: A Super-Eddington Unification Model

Reference 45

Resolution
verified exact
arxiv_id, observed 2026-07-20T03:19:15.500417Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T03:11:10.401986Z digest=sha256:8445d3db237211c0063c3c87a42949194286be02c1ff1dac7447466399d9659a

Observation ad575e11-c164-4bdb-a301-7b124b99813f · outbound

This paper cites 2024, A&A, 691, A145 Matthee , J., Naidu, R.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff 2024, A&A, 691, A145 Matthee , J., Naidu, R

Reference 46

Resolution
verified fuzzy
raw_fallback, observed 2026-05-14T10:59:15.443100Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T03:11:10.401986Z digest=sha256:90fd86c9dfcb02fc88c0419582573c5e9c5f330459c410fdbcc8cb5f0f514d2f

Observation 6d371ba6-c0a5-453c-9425-ba2e88a054c6 · outbound

This paper cites P., Kotiwale, G., et al.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff P., Kotiwale, G., et al

Reference 47

Resolution
verified fuzzy
raw_fallback, observed 2026-05-14T10:59:15.453368Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T03:11:10.401986Z digest=sha256:6fe5fb43b75b731f80be0b5ce479c7a2824fbc698508eaf277fd97af545c4d8e

Observation e4f10479-9ef8-4928-a49b-11278b14d674 · outbound

This paper cites A "Black Hole Star" Reveals the Remarkable Gas-Enshrouded Hearts of the Little Red Dots.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff A "Black Hole Star" Reveals the Remarkable Gas-Enshrouded Hearts of the Little Red Dots

Reference 48

Resolution
metadata mismatch
arxiv_id, observed 2026-05-16T08:53:14.890938Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T03:11:10.401986Z digest=sha256:d70f8f6cceea25dd785ec88ef3e9dbed7d306324c0a2db104c4b344fc838db95

Observation 61824f68-eb49-4a37-9b77-72314fce2cbe · outbound

This paper cites Pacucci, A.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff Pacucci, A

Reference 49

Resolution
verified exact
arxiv_id, observed 2026-05-11T03:15:55.081049Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T03:11:10.401986Z digest=sha256:ea26d32d192612c655680c99d506046c79e0308829011ba35541957107b22f80

Observation d0ce5a91-f6e5-41c4-941e-0eab4088e427 · outbound

This paper cites an unresolved cited work.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff Unresolved cited work

Reference 50

Resolution
unresolved
raw_fallback, observed 2026-05-14T10:59:15.424928Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T03:11:10.401986Z digest=sha256:a8e1665996e4909d0c2c507ea8e963b6503b1cc17645785e666c6ea9c2617263

Observation 3df1c0b4-8745-41e6-9e87-90514b8b801c · outbound

This paper cites F., Schaye, J., et al.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff F., Schaye, J., et al

Reference 51

Resolution
verified fuzzy
raw_fallback, observed 2026-05-14T10:59:15.417370Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T03:11:10.401986Z digest=sha256:4b0deb394d41998644e084c920ec7a299af395b1a0971411252d728a8ac1ef02

Observation dc242ea2-1e20-4abe-8c5b-4663c30333ee · outbound

This paper cites 2025, A&A, 704, A248.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff 2025, A&A, 704, A248

Reference 52

Resolution
verified fuzzy
raw_fallback, observed 2026-05-14T10:59:15.441061Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T03:11:10.401986Z digest=sha256:ab466c97866de52bc17e760992e07d29bf90ec9e8dd8dc89bb364c73c3872c4c

Observation 7842b5c0-9f90-43dd-8c55-4b9133b1678d · outbound

This paper cites an unresolved cited work.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff Unresolved cited work

Reference 53

Resolution
unresolved
raw_fallback, observed 2026-05-14T10:59:15.463062Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T03:11:10.401986Z digest=sha256:06d805cfbe0b35ddb5022dfc22403f79d4a7d8973a686f249f76e88c8268174f

Observation ea831b52-d23a-4522-8990-b1b2d6025e87 · outbound

This paper cites H., et al.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff H., et al

Reference 54

Resolution
verified fuzzy
raw_fallback, observed 2026-05-14T10:59:15.427667Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T03:11:10.401986Z digest=sha256:caeecb09b06e5e08f561e2263535943c75074e44a4632ba93938e948419943cb

Observation c3e7862b-7552-420a-b274-59ed8f972ad1 · outbound

This paper cites P., et al.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff P., et al

Reference 55

Resolution
verified fuzzy
raw_fallback, observed 2026-05-14T10:59:15.464892Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T03:11:10.401986Z digest=sha256:745c57d33f5be321c5c3855033a2fd65d3b7270dd77ad479183ce450026a72b0

Observation 4705d13f-10ca-4dcb-b830-97f6a1e7fa05 · outbound

This paper cites 2026, arXiv e-prints, arXiv:2603.22277, doi: 10.48550/arXiv.2603.22277.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff 2026, arXiv e-prints, arXiv:2603.22277, doi: 10.48550/arXiv.2603.22277

Reference 56

Resolution
verified exact
arxiv_id, observed 2026-05-11T03:15:55.076236Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T03:11:10.401986Z digest=sha256:3c1a5e694d1312d0636b750b1af4ca0d91ff0e851079ea488f4b42d20ccc173a

Observation 5e3a303b-d13c-45be-af0d-12c3a72afb6c · outbound

This paper cites J., Greene, J.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff J., Greene, J

Reference 57

Resolution
verified fuzzy
raw_fallback, observed 2026-05-14T10:59:15.457420Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T03:11:10.401986Z digest=sha256:225f584d4f849143e6e103bdc2b9cc20ef8d4f8f8a98452b5d83d700fba0a17e

Observation c084ec9b-4aff-4012-88c8-ca11133f73cb · outbound

This paper cites F., Faucher-Giguère, C.-A., et al.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff F., Faucher-Giguère, C.-A., et al

Reference 58

Resolution
verified fuzzy
raw_fallback, observed 2026-05-14T10:59:15.422163Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T03:11:10.401986Z digest=sha256:0c77a8c071c52f343d2822703771c91c2e0f4aea4246a7d6b2ae74789f367a28

Observation ae0c192d-091d-497b-a26e-3e67a92c70c1 · outbound

This paper cites Little Red Dot $-$ Host Galaxy $=$ Black Hole Star: A Gas-Enshrouded Heart at the Center of Every Little Red Dot.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff Little Red Dot $-$ Host Galaxy $=$ Black Hole Star: A Gas-Enshrouded Heart at the Center of Every Little Red Dot

Reference 59

Resolution
verified exact
arxiv_id, observed 2026-05-25T03:01:11.256109Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T03:11:10.401986Z digest=sha256:2e96b534d5ad04044cafb066c69e284be57c3a2a94cd6b05dcff41ffaa5a8363

Observation 8faeabfc-a3d3-44a5-b2fc-dc0e00b124fb · outbound

This paper cites P., Plat, A., et al.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff P., Plat, A., et al

Reference 60

Resolution
verified fuzzy
raw_fallback, observed 2026-05-14T10:54:13.657507Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T03:11:10.401986Z digest=sha256:16b782dc9fc3f2d5d9eef7c392ff6cec9717b8efc235df4224ab9a9d62530a7d

Observation 0e231a86-9ea9-4449-ab6d-8ab2cff0a48b · outbound

This paper cites J., Kokorev, V ., Kocevski, D.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff J., Kokorev, V ., Kocevski, D

Reference 61

Resolution
verified fuzzy
raw_fallback, observed 2026-05-14T10:54:13.659099Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T03:11:10.401986Z digest=sha256:dd5f218b3bbd723d4f9f78737a732afc85d9eefa54c6ecd5c2c5e7ca4c319af0

Observation 859db90f-6bc1-44f1-8f06-10f302d63fe5 · outbound

This paper cites E., Weaver, J.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff E., Weaver, J

Reference 62

Resolution
verified fuzzy
raw_fallback, observed 2026-05-14T10:54:13.660649Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T03:11:10.401986Z digest=sha256:cbf9e1299fb3eddc2da00508af72a344302c12ab43bb76fd03b3422be7bc132c

Observation 63988257-e28d-43eb-a4ba-8650143e3c8a · outbound

This paper cites Episodic super-Eddington accretion as a clue to Overmassive Black Holes in the early Universe.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff Episodic super-Eddington accretion as a clue to Overmassive Black Holes in the early Universe

Reference 63

Resolution
verified exact
arxiv_id, observed 2026-05-11T03:15:55.063054Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T03:11:10.401986Z digest=sha256:6353e140d016673ca80775325b70cfef60b478229fda87f95b025831d7474edd

Observation df450592-348e-490b-82d2-99af28ba0ebb · outbound

This paper cites 2026, ApJ, 999, 183.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff 2026, ApJ, 999, 183

Reference 64

Resolution
verified fuzzy
raw_fallback, observed 2026-05-14T10:54:13.656032Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T03:11:10.401986Z digest=sha256:264738190b71c8450c03aea35b6e0f730b5bc0cc8fbf49853410a5b65200f3e3

Observation e678a7eb-5954-495e-8b76-a968e9e74805 · outbound

This paper cites L., et al.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff L., et al

Reference 65

Resolution
verified fuzzy
raw_fallback, observed 2026-05-14T10:54:13.651265Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T03:11:10.401986Z digest=sha256:a8e726ed7a47fea2d2003aae7f7541a1d55a8691729c2dc5d0217ca7828b91ba

Observation 01310997-18fe-4646-a8f2-616a3ef96b1a · outbound

This paper cites an unresolved cited work.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff Unresolved cited work

Reference 66

Resolution
unresolved
raw_fallback, observed 2026-05-14T10:54:13.652763Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T03:11:10.401986Z digest=sha256:49641091a40f41488ac9435c3b7f652eb44765f8ba6aae61f789581059362ef8

Observation 6ff0fef4-8ed5-4da1-a1df-573ddf28a0af · outbound

This paper cites 2026, ApJ, 999, 31.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff 2026, ApJ, 999, 31

Reference 67

Resolution
verified fuzzy
raw_fallback, observed 2026-05-14T10:54:13.654231Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T03:11:10.401986Z digest=sha256:a7c5e298c6483dc6f78f21bc482fb93cfa5131c26a5f38b4230db3f91472d230

Observation 367e593c-d1f6-4049-95cc-cf543f0e9817 · outbound

This paper cites & King, A.

Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff & King, A

Reference 68

Resolution
verified fuzzy
raw_fallback, observed 2026-05-14T10:54:13.649590Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-11T03:11:10.401986Z digest=sha256:bafb04ac17ce3a3050329740576cfe6f2354f70371b730b04a5d2e2b8d96bdf2

Pith citing papers

Observation 161a7b93-e3ba-498a-9f15-dde972878e78 · inbound

A Population of Red Galaxies with Very Strong Emission Lines at $z > 5$ Revealed by the NIRCam Medium Bands: ''Classic'' LRDs, Dusty Star-Forming Galaxies, and a Missing Population of LRDs cites this paper.

A Population of Red Galaxies with Very Strong Emission Lines at $z > 5$ Revealed by the NIRCam Medium Bands: ''Classic'' LRDs, Dusty Star-Forming Galaxies, and a Missing Population of LRDs Testing the BH$^*$ Model: a UV-to-Optical Spectral Fitting of The Cliff

Reference 120

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local_arxiv, observed 2026-06-28T01:41:30.082582Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-06-28T00:23:19.443839Z digest=sha256:f20ab7e6d3ce80a2061a6706aa2aa1a5021f55244f0967956f0743454da8d17a