Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots | Paper Citation Record

Observation ed06d4ed-ada3-4f0e-ac43-e0a92c83e608 · outbound

This paper cites 1988, ApJ, 332, 646, doi: 10.1086/166683.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 1988, ApJ, 332, 646, doi: 10.1086/166683

Reference 1

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Observation 94804366-bfd8-46e9-bb7e-d7ba7d80176b · outbound

This paper cites B., Casey, C.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots B., Casey, C

Reference 2

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Observation 0705e835-54b3-44f1-838b-8b9baaf9339b · outbound

This paper cites C., & Dexter, J.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots C., & Dexter, J

Reference 3

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Observation d8fc5118-561b-40bd-9a92-74d1dee7abfa · outbound

This paper cites 2026, MNRAS, 545, staf2131, doi: 10.1093/mnras/staf2131.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 2026, MNRAS, 545, staf2131, doi: 10.1093/mnras/staf2131

Reference 4

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Observation 17699e12-3c57-487d-b4ba-f179217094b0 · outbound

This paper cites ABCD: The Nuclear Structure of the Little Red Dots Revealted through Absorption, Break, Continuum, and Decrement.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots ABCD: The Nuclear Structure of the Little Red Dots Revealted through Absorption, Break, Continuum, and Decrement

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:26.156486Z

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Observation f5594ae8-e0f9-4665-89eb-ccdc701b6ef8 · outbound

This paper cites Spectral Appearance of Self-gravitating Disks Powered by Stellar Objects: Universal Effective Temperature in the Optical Continuum and Application to Little Red Dots.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots Spectral Appearance of Self-gravitating Disks Powered by Stellar Objects: Universal Effective Temperature in the Optical Continuum and Application to Little Red Dots

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:26.344749Z

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Observation c3b9d24d-164a-4648-b673-9d4a0fa1c26d · outbound

This paper cites A., Boylan-Kolchin, M., et al.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots A., Boylan-Kolchin, M., et al

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Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:26.394835Z

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Observation 5f6b6ebf-415d-4f09-80d7-5dedf58aebb4 · outbound

This paper cites an unresolved cited work.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots Unresolved cited work

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:26.464311Z

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Observation c51011ac-ccae-4151-b9f5-5d1562de0e5d · outbound

This paper cites J., Duncan, K.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots J., Duncan, K

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:26.551919Z

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Observation 8eb7904a-15e8-4b36-ad15-e69fd8a1801d · outbound

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

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots E., Labbe, I., Goulding, A

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:26.663833Z

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Observation a9388241-170c-4cca-9fa5-df9e6ee788a7 · outbound

This paper cites 2006, MNRAS, 365, 345, doi: 10.1111/j.1365-2966.2005.09712.x.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 2006, MNRAS, 365, 345, doi: 10.1111/j.1365-2966.2005.09712.x

Reference 11

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Observation 9f4400ac-6846-4af8-98da-073f1471ec1e · outbound

This paper cites 2026, PASJ, doi: 10.1093/pasj/psag030.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 2026, PASJ, doi: 10.1093/pasj/psag030

Reference 12

Resolution: verified exact; doi, observed 2026-08-01T18:13:33.088298Z

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Observation ce330311-4142-41b6-9425-58fa88f69733 · outbound

This paper cites G., & Storey, P.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots G., & Storey, P

Reference 13

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Observation b68b85c5-0973-4b34-8d6c-02cb5fdccc7d · outbound

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

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots E., de Graaff, A., Miller, T

Reference 14

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Observation c27ddb9e-8187-481b-933e-e0c2e70a42a8 · outbound

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Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots Unresolved cited work

Reference 15

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Observation d62d785f-6147-4a5d-babf-9ad09e4e27b5 · outbound

This paper cites 2024, ApJL, 973, L49, doi: 10.3847/2041-8213/ad74e2.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 2024, ApJL, 973, L49, doi: 10.3847/2041-8213/ad74e2

Reference 16

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Observation 778b14e2-d75c-4f1d-a658-78e0ec732a74 · outbound

This paper cites S., & Noda, H.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots S., & Noda, H

Reference 17

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Observation a6b7088a-6306-4418-aae0-9fc8763dff1d · outbound

This paper cites 2025, ApJL, 980, L27, doi: 10.3847/2041-8213/adaebd.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 2025, ApJL, 980, L27, doi: 10.3847/2041-8213/adaebd

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:27.573311Z

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Observation 82f20962-06f5-4cfa-8088-398bc5672a6e · outbound

This paper cites 2026, ApJ, 998, 148, doi: 10.3847/1538-4357/ae3725.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 2026, ApJ, 998, 148, doi: 10.3847/1538-4357/ae3725

Reference 19

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Observation e822222e-76f4-43dd-8aa0-b254c7416d31 · outbound

This paper cites 2025, MNRAS, 544, 3900, doi: 10.1093/mnras/staf1867.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 2025, MNRAS, 544, 3900, doi: 10.1093/mnras/staf1867

Reference 20

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Observation f8526e29-8092-4919-b8f1-bd1e9e8b20f7 · outbound

This paper cites 2026, MNRAS, 545, staf2235, doi: 10.1093/mnras/staf2235.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 2026, MNRAS, 545, staf2235, doi: 10.1093/mnras/staf2235

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:27.933162Z

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Observation f4a9cbf7-7ba0-4ad9-a682-2223c06cffb3 · outbound

This paper cites 2026, ApJL, 996, L19, doi: 10.3847/2041-8213/ae247a.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 2026, ApJL, 996, L19, doi: 10.3847/2041-8213/ae247a

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:28.019559Z

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Observation 0871d9b2-195a-4a9d-9acd-1ccae7514f75 · outbound

This paper cites M., & Davis, S.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots M., & Davis, S

Reference 23

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Observation 7547ca26-33e2-4e95-9e80-42c8a2dd7a77 · outbound

This paper cites 2009, PASJ, 61, 769, doi: 10.1093/pasj/61.4.769 —.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 2009, PASJ, 61, 769, doi: 10.1093/pasj/61.4.769 —

Reference 24

Resolution: verified exact; doi, observed 2026-08-01T18:13:32.688519Z

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

Observation bec8a876-5f85-4fd0-aeb1-7abea300fb94 · outbound

This paper cites an unresolved cited work.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots Unresolved cited work

Reference 25

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Observation bd1c99b6-bd3a-4565-8330-85e636c273f4 · outbound

This paper cites 2001, ApJL, 552, L109, doi: 10.1086/320343.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 2001, ApJL, 552, L109, doi: 10.1086/320343

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Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:28.564663Z

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Observation a7661274-dcd5-4247-909d-861c43676cf4 · outbound

This paper cites R., & Pounds, K.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots R., & Pounds, K

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Observation 4c955901-d862-491f-811b-54ef5b029a63 · outbound

This paper cites 2013, Stellar Structure and Evolution, doi: 10.1007/978-3-642-30304-3.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 2013, Stellar Structure and Evolution, doi: 10.1007/978-3-642-30304-3

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:28.819538Z

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Observation 8b4b9753-c0c2-4d3d-bdc2-9bab7b2056fa · outbound

This paper cites 2017, PASJ, 69, 92, doi: 10.1093/pasj/psx101 —.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 2017, PASJ, 69, 92, doi: 10.1093/pasj/psx101 —

Reference 29

Resolution: verified exact; doi, observed 2026-08-01T18:13:32.472274Z

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Observation 354ac07e-5b25-4c92-9d07-80a1e3d9e461 · outbound

This paper cites D., Finkelstein, S.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots D., Finkelstein, S

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Observation 9a011a38-b263-424f-8008-0f1f604ad0fb · outbound

This paper cites I., Greene, J.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots I., Greene, J

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Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:29.225485Z

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Observation 0a166e13-d4b9-4db0-8e41-fd688778dd7a · 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.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 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

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Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:29.353280Z

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Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots E., Bezanson, R., et al

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Observation 3f54923c-3d7a-40dc-b495-bb3edc6a6312 · outbound

This paper cites The GlimmIr: Spectroscopic Variability in a z~7 LRD Indicates Rapid Changes in Both the Narrow and Broad Line Regions.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots The GlimmIr: Spectroscopic Variability in a z~7 LRD Indicates Rapid Changes in Both the Narrow and Broad Line Regions

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Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:29.585684Z

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Observation 2ee8fe58-8d45-4fcc-8d6a-3eb3a06618ea · outbound

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Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 2006, ApJ, 643, 112, doi: 10.1086/502798

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Observation 053bafeb-28bd-4901-b219-a41a7b62f5ce · outbound

This paper cites an unresolved cited work.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots Unresolved cited work

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Observation 7408b8ed-c120-4fde-9fbc-681c430385a4 · outbound

This paper cites 2026, ApJ, 997, 364, doi: 10.3847/1538-4357/ae2bdf.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 2026, ApJ, 997, 364, doi: 10.3847/1538-4357/ae2bdf

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Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:29.947856Z

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Observation 03e4955a-46eb-4360-8684-b72958048eda · outbound

This paper cites E., & Ma, Y.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots E., & Ma, Y

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Observation 43d5297e-eeb8-4642-bec8-121e841747e5 · outbound

This paper cites 2026, arXiv e-prints, arXiv:2603.02317, doi: 10.48550/arXiv.2603.02317.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 2026, arXiv e-prints, arXiv:2603.02317, doi: 10.48550/arXiv.2603.02317

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Observation a62dde79-3138-43f0-a249-6fa959d5c5ae · outbound

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Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 1997, ApJ, 489, 573, doi: 10.1086/304814

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Observation 9b214903-7f10-4e78-9efe-d9f3d133c3cc · outbound

This paper cites 2024, A&A, 691, A145, doi: 10.1051/0004-6361/202347640.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 2024, A&A, 691, A145, doi: 10.1051/0004-6361/202347640

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Observation ea38f061-91c4-49b0-b54b-4d234dea5a5b · outbound

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Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 2025, MNRAS, 538, 1921, doi: 10.1093/mnras/staf359

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Observation 5894661d-78ff-4183-a8e5-d4a35127bd83 · outbound

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Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots P., Brammer, G., et al

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Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:30.784703Z

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Observation 04f8519c-b367-429a-8d19-26c136d7a941 · outbound

This paper cites 2026, arXiv e-prints, arXiv:2603.17667, doi: 10.48550/arXiv.2603.17667.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 2026, arXiv e-prints, arXiv:2603.17667, doi: 10.48550/arXiv.2603.17667

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Observation 98a587f7-d57a-4864-a2f5-1764ac9cbfb9 · outbound

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Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 2026, A&A, 706, A372, doi: 10.1051/0004-6361/202453317

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Observation d2004158-379b-4370-b996-889ca169901d · outbound

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Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 2014, MNRAS, 441, 3177, doi: 10.1093/mnras/stu762

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Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:31.164942Z

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Observation 9403f486-b7ff-467f-86ec-b061ae6e0205 · outbound

This paper cites an unresolved cited work.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots Unresolved cited work

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Observation 1e35d5b8-9745-48a2-8f0b-32d98130d6d4 · outbound

This paper cites M., Kaastra, J.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots M., Kaastra, J

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Observation c165e745-9a20-4e65-a166-c94a172e38cd · outbound

This paper cites an unresolved cited work.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots Unresolved cited work

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Observation 86bbb791-4181-4987-9de0-c34c617e1eb6 · outbound

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

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots A "Black Hole Star" Reveals the Remarkable Gas-Enshrouded Hearts of the Little Red Dots

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Observation d552bf1f-edd2-4280-b085-f7cac498cbeb · outbound

This paper cites 2026, ApJ, 998, 124, doi: 10.3847/1538-4357/ae32f3.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 2026, ApJ, 998, 124, doi: 10.3847/1538-4357/ae32f3

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Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:31.840506Z

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This paper cites Evidence of violation of Case B recombination in Little Red Dots.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots Evidence of violation of Case B recombination in Little Red Dots

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Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:32.000164Z

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Observation 0144d00d-3fec-4031-97bd-15e4c820fccd · outbound

This paper cites Optical Counterparts of Ultraluminous X-Ray Sources.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots Optical Counterparts of Ultraluminous X-Ray Sources

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Observation 2739a74e-29a4-46fc-9c0c-c0d945f10a30 · outbound

This paper cites an unresolved cited work.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots Unresolved cited work

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Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:32.306636Z

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Observation 1a3f949c-aba5-467d-8a24-f19f0263993f · outbound

This paper cites G., & Abolmasov, P.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots G., & Abolmasov, P

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:32.374304Z

Source-reported events for the cited work

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Observation 7070785a-3fec-4239-8faa-355754c1bf19 · outbound

This paper cites 2021, ApJ, 906, 36, doi: 10.3847/1538-4357/abc959.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 2021, ApJ, 906, 36, doi: 10.3847/1538-4357/abc959

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:32.527798Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1a2d3113-4fb0-434f-afe3-146ecaa5251c · outbound

This paper cites P., et al.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots P., et al

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:32.638631Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ec1411d9-bfb9-4340-8d48-ea06100b3761 · outbound

This paper cites D., Farag, E., Bellinger, E.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots D., Farag, E., Bellinger, E

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:32.725155Z

Source-reported events for the cited work

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Observation 64625381-40df-4d98-9b23-5ce7562a1c0d · outbound

This paper cites I., & Sunyaev, R.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots I., & Sunyaev, R

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:32.796362Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7a3f68f9-cc53-4f6e-a570-16c3d6374e6e · outbound

This paper cites 2015, MNRAS, 447, L60, doi: 10.1093/mnrasl/slu183.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 2015, MNRAS, 447, L60, doi: 10.1093/mnrasl/slu183

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:32.879008Z

Source-reported events for the cited work

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Observation ea1ebcce-7c10-4dcf-b5b1-36ab077be7f4 · outbound

This paper cites 2016, MNRAS, 459, 171, doi: 10.1093/mnras/stw645 Sądowski, A., & Narayan, R.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 2016, MNRAS, 459, 171, doi: 10.1093/mnras/stw645 Sądowski, A., & Narayan, R

Reference 61

Resolution: verified exact; doi, observed 2026-08-01T18:13:31.998868Z

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.

Observation 4ce81885-8777-43c8-95e7-868425bfcd5e · outbound

This paper cites 2014, MNRAS, 439, 503, doi: 10.1093/mnras/stt2479.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 2014, MNRAS, 439, 503, doi: 10.1093/mnras/stt2479

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:33.006582Z

Source-reported events for the cited work

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Observation 7d8abad9-c826-4c1a-97f9-58aa8ed2a213 · outbound

This paper cites H., et al.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots H., et al

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:33.118525Z

Source-reported events for the cited work

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Observation 35a10b86-5604-488e-9585-3f5f9a889083 · outbound

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

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots Little Red Dot $-$ Host Galaxy $=$ Black Hole Star: A Gas-Enshrouded Heart at the Center of Every Little Red Dot

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:33.263750Z

Source-reported events for the cited work

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Observation da3dc03e-7bba-451f-bd08-2e7b0aa4a169 · outbound

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

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots J., Kokorev, V., Kocevski, D

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:33.411009Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 55c5cf4c-e340-4fd4-81d9-c15f721beec6 · outbound

This paper cites You can't see me: Super-Eddington growth hindering X-ray detection in high-z broad-line active galactic nuclei.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots You can't see me: Super-Eddington growth hindering X-ray detection in high-z broad-line active galactic nuclei

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:33.540677Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 34d77524-444f-493c-a36f-290f94a64185 · outbound

This paper cites 2026, ApJ, 999, 183, doi: 10.3847/1538-4357/ae4101.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 2026, ApJ, 999, 183, doi: 10.3847/1538-4357/ae4101

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:33.653692Z

Source-reported events for the cited work

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Observation 6dfb40e1-1a0f-4dee-8d6b-22b94295dbc1 · outbound

This paper cites 2024, ApJL, 969, L13, doi: 10.3847/2041-8213/ad55f7.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 2024, ApJL, 969, L13, doi: 10.3847/2041-8213/ad55f7

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:33.793722Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d5183357-a533-44ec-9ffc-1beae9b5fdb3 · outbound

This paper cites 2026, arXiv e-prints, arXiv:2602.06024, doi: 10.48550/arXiv.2602.06024.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 2026, arXiv e-prints, arXiv:2602.06024, doi: 10.48550/arXiv.2602.06024

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:33.934602Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9bb31f80-cdd7-4375-8f9e-54ba9d8fcc69 · outbound

This paper cites 2025, arXiv e-prints, arXiv:2511.09278, doi: 10.48550/arXiv.2511.09278.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 2025, arXiv e-prints, arXiv:2511.09278, doi: 10.48550/arXiv.2511.09278

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:34.044801Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 50bba6bd-5a4d-4cda-b9b5-e2b80c29e2a2 · outbound

This paper cites an unresolved cited work.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots Unresolved cited work

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:34.223336Z

Source-reported events for the cited work

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Observation 3ea166f8-1655-4684-bceb-5612b2a858a7 · outbound

This paper cites 2026, ApJ, 1002, 159, doi: 10.3847/1538-4357/ae5dbd.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 2026, ApJ, 1002, 159, doi: 10.3847/1538-4357/ae5dbd

Reference 72

Resolution: verified exact; doi, observed 2026-08-01T18:13:31.722245Z

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.

Observation a59927e9-0451-46de-9ab9-6a32ee6ef673 · outbound

This paper cites 2019, ApJL, 884, L3, doi: 10.3847/2041-8213/ab44c7.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 2019, ApJL, 884, L3, doi: 10.3847/2041-8213/ab44c7

Reference 73

Resolution: verified exact; doi, observed 2026-08-01T18:13:31.575753Z

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.

Observation 2a026fa2-157e-455d-ad24-71ac7f203ae2 · outbound

This paper cites T., et al.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots T., et al

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:34.551942Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2b278dc8-1102-41c7-8c54-1d0141085342 · outbound

This paper cites 2026, Nature Astronomy, doi: 10.1038/s41550-026-02785-x.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 2026, Nature Astronomy, doi: 10.1038/s41550-026-02785-x

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:34.711414Z

Source-reported events for the cited work

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Observation 688e3640-ee8f-472a-9ceb-626557336721 · outbound

This paper cites an unresolved cited work.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots Unresolved cited work

Reference 76

Resolution: verified exact; doi, observed 2026-08-01T18:13:31.403687Z

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.

Observation 9c191b43-873c-4a24-ba67-be5055e5197b · outbound

This paper cites C., & Yao, Y.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots C., & Yao, Y

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:34.993602Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation eb86e8ef-7086-4ecf-a3f9-08dd256c4a64 · outbound

This paper cites 2026, ApJ, 999, 31, doi: 10.3847/1538-4357/ae3612.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 2026, ApJ, 999, 31, doi: 10.3847/1538-4357/ae3612

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:35.081708Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0835160d-d859-47c0-90fa-07e5bd9166b4 · outbound

This paper cites 2025, arXiv e-prints, arXiv:2507.22014, doi: 10.48550/arXiv.2507.22014.

Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots 2025, arXiv e-prints, arXiv:2507.22014, doi: 10.48550/arXiv.2507.22014

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-01T18:08:35.202889Z

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Outbound references

Pith citing papers