Paper Citation Record · LEDGER

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots

As of 7 August 2026, this Paper Citation Record lists 87 of 87 outbound references and 16 inbound Pith citation observations for arXiv:2509.05434.

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

pith.paper-citation-record.v1
2509.05434 v1

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Outbound references

Observation 0fc565e8-8360-4996-a506-05acccca3447 · outbound

This paper cites COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly

Reference 1

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Observation 6667839f-ea39-4348-8b5d-40a3cb33babc · outbound

This paper cites 2019, MNRAS, 485, 2694, doi: 10.1093/mnras/stz551.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots 2019, MNRAS, 485, 2694, doi: 10.1093/mnras/stz551

Reference 2

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Observation bef06466-f501-4a71-902e-447b06d91aac · outbound

This paper cites T., Bogd´ an,´A., Kov´ acs, O.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots T., Bogd´ an,´A., Kov´ acs, O

Reference 3

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Observation 57377696-d7e9-4afa-9934-e23e4b2623b5 · outbound

This paper cites The Small Sizes and High Implied Densities of `Little Red Dots' with Balmer Breaks Could Explain Their Broad Emission Lines Without an AGN.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots The Small Sizes and High Implied Densities of `Little Red Dots' with Balmer Breaks Could Explain Their Broad Emission Lines Without an AGN

Reference 4

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Observation 92ff4e77-ba3f-4a33-8ee6-e65e91c539aa · outbound

This paper cites G., Kocevski, D.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots G., Kocevski, D

Reference 5

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Observation 9cc16c70-9fb3-4ae5-8ab9-f80f59296028 · outbound

This paper cites A Comprehensive Photometric Selection of `Little Red Dots' in MIRI Fields: An IR-Bright LRD at $z=3.1386$ with Warm Dust Emission.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots A Comprehensive Photometric Selection of `Little Red Dots' in MIRI Fields: An IR-Bright LRD at $z=3.1386$ with Warm Dust Emission

Reference 6

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Observation 93e0bd72-2035-4bb5-98f7-b3df9d200556 · outbound

This paper cites C., & Dexter, J.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots C., & Dexter, J

Reference 7

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Observation 7383ad2a-2034-47c4-80fd-f90f66d3a8ff · outbound

This paper cites C., Rossi, E.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots C., Rossi, E

Reference 8

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Observation 5731ef8a-8583-4315-a561-7f42c0a55ec9 · outbound

This paper cites E., et al.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots E., et al

Reference 9

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Observation b0558b33-bdac-4cf9-ba66-c548e1e08cf8 · outbound

This paper cites An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots An upper limit of 10$^6$ M$_\odot$ in dust from ALMA observations in 60 Little Red Dots

Reference 10

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Observation 027f0d70-fdb0-43e0-b7b9-b4dbf6ee8eed · outbound

This paper cites The Physical Nature of the Off-centered Extended Emission Associated with the Little Red Dots.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots The Physical Nature of the Off-centered Extended Emission Associated with the Little Red Dots

Reference 11

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Observation a8521c4d-09b2-4775-a7e2-6f5f2283251e · outbound

This paper cites The Host Galaxy (If Any) of the Little Red Dots.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots The Host Galaxy (If Any) of the Little Red Dots

Reference 12

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Observation 6829e6f9-66b4-41af-9da0-2026d68e3d78 · outbound

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What you see is what you get: empirically measured bolometric luminosities of Little Red Dots Unresolved cited work

Reference 13

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Observation 3a5da92a-9e1a-4b80-a036-42e54c7b0ee2 · outbound

This paper cites M., Rhook, K., Corbett, E.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots M., Rhook, K., Corbett, E

Reference 14

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Observation 976fde38-d71d-45c2-ac14-df6ea6e2ab32 · outbound

This paper cites RUBIES: a complete census of the bright and red distant Universe with JWST/NIRSpec.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots RUBIES: a complete census of the bright and red distant Universe with JWST/NIRSpec

Reference 15

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Observation f9cc8dcf-2589-4e42-981b-70c49123e336 · outbound

This paper cites 2003, in The Mass of Galaxies at Low and High Redshift, ed.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots 2003, in The Mass of Galaxies at Low and High Redshift, ed

Reference 16

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Observation 6febd40b-d467-49c0-83aa-4cb31975cd50 · outbound

This paper cites D., et al.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots D., et al

Reference 17

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Observation b23625e2-166d-4278-ad45-0845c3c3aa0d · outbound

This paper cites J., McDowell, J.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots J., McDowell, J

Reference 18

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Observation c14eab54-452a-417b-9349-fca2aae4552f · outbound

This paper cites DUALZ: Deep UNCOVER-ALMA Legacy High-Z Survey.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots DUALZ: Deep UNCOVER-ALMA Legacy High-Z Survey

Reference 19

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This paper cites J., Zitrin, A., Plat, A., et al.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots J., Zitrin, A., Plat, A., et al

Reference 20

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Observation 7bc1c9c1-3ca5-4208-a8b8-d4bc434bb38b · outbound

This paper cites J., Zitrin, A., Weaver, J.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots J., Zitrin, A., Weaver, J

Reference 21

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Observation af5db91c-2487-4da2-8d1a-8a4ada758086 · outbound

This paper cites J., Labb´ e, I., Zitrin, A., et al.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots J., Labb´ e, I., Zitrin, A., et al

Reference 22

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Observation 518cbef4-1846-472a-b6ce-b29465d0c87a · outbound

This paper cites Another piece to the puzzle: radio detection of a JWST detected AGN candidate.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots Another piece to the puzzle: radio detection of a JWST detected AGN candidate

Reference 23

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Observation 3592b037-f6d6-404e-b885-86db3094b40f · outbound

This paper cites E., & Ho, L.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots E., & Ho, L

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Observation e996cae8-fe5f-4a60-a2f5-a652a77d52f7 · outbound

This paper cites E., Strader, J., & Ho, L.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots E., Strader, J., & Ho, L

Reference 25

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Observation c85a7198-6e61-4f1a-be57-f55312653649 · outbound

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

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots E., Labbe, I., Goulding, A

Reference 26

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Observation 4633c18c-1e5a-40c9-b73f-5ea2339d9028 · outbound

This paper cites S., Li, Y., et al.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots S., Li, Y., et al

Reference 27

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This paper cites A JWST/NIRSpec First Census of Broad-Line AGNs at z=4-7: Detection of 10 Faint AGNs with M_BH~10^6-10^8 M_sun and Their Host Galaxy Properties.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots A JWST/NIRSpec First Census of Broad-Line AGNs at z=4-7: Detection of 10 Faint AGNs with M_BH~10^6-10^8 M_sun and Their Host Galaxy Properties

Reference 28

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This paper cites Periodic subvarieties of semiabelian varieties and annihilators of irreducible representations.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots Periodic subvarieties of semiabelian varieties and annihilators of irreducible representations

Reference 29

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

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots E., de Graaff, A., Miller, T

Reference 31

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

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots 2024, ApJL, 973, L49, doi: 10.3847/2041-8213/ad74e2

Reference 32

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Observation d7874a2d-7dc4-494b-94d0-d7f4f4d5be44 · outbound

This paper cites Extremely Dense Gas around Little Red Dots and High-redshift Active Galactic Nuclei: A Non-stellar Origin of the Balmer Break and Absorption Features.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots Extremely Dense Gas around Little Red Dots and High-redshift Active Galactic Nuclei: A Non-stellar Origin of the Balmer Break and Absorption Features

Reference 33

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This paper cites 2025, arXiv e-prints, arXiv:2501.13082, doi: 10.48550/arXiv.2501.13082 Juodˇ zbalis, I., Maiolino, R., Baker, W.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots 2025, arXiv e-prints, arXiv:2501.13082, doi: 10.48550/arXiv.2501.13082 Juodˇ zbalis, I., Maiolino, R., Baker, W

Reference 34

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Observation e63160d1-21c3-4309-96a5-3844f284a21d · outbound

This paper cites S., Netzer, H., et al.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots S., Netzer, H., et al

Reference 35

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Reference 36

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This paper cites 2024, A&A, 691, A52, doi: 10.1051/0004-6361/202348857.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots 2024, A&A, 691, A52, doi: 10.1051/0004-6361/202348857

Reference 37

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Observation 944211e3-bd67-4bdb-8e91-a577aef77199 · outbound

This paper cites The Rise of Faint, Red AGN at $z>4$: A Sample of Little Red Dots in the JWST Extragalactic Legacy Fields.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots The Rise of Faint, Red AGN at $z>4$: A Sample of Little Red Dots in the JWST Extragalactic Legacy Fields

Reference 38

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What you see is what you get: empirically measured bolometric luminosities of Little Red Dots 2023, ApJL, 957, L7, doi: 10.3847/2041-8213/ad037a

Reference 39

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Observation 0708be37-1d95-493d-960f-eede59954988 · outbound

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What you see is what you get: empirically measured bolometric luminosities of Little Red Dots I., Greene, J

Reference 40

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This paper cites 2019, MNRAS, 489, 524, doi: 10.1093/mnras/stz2140 Labb´ e, I., van Dokkum, P., Nelson, E., et al.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots 2019, MNRAS, 489, 524, doi: 10.1093/mnras/stz2140 Labb´ e, I., van Dokkum, P., Nelson, E., et al

Reference 41

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Observation 34f52ef8-bddb-4ea8-b8c1-eb49817a6e8c · 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.

What you see is what you get: empirically measured bolometric luminosities of 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

Reference 42

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Observation 4a0f5a4a-dbfe-4f03-bb63-e744cf453e86 · outbound

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What you see is what you get: empirically measured bolometric luminosities of Little Red Dots E., Bezanson, R., et al

Reference 43

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This paper cites The case for super-Eddington accretion in JWST broad-line AGN during the first billion years.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots The case for super-Eddington accretion in JWST broad-line AGN during the first billion years

Reference 44

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What you see is what you get: empirically measured bolometric luminosities of Little Red Dots 2024, ApJ, 974, 147, doi: 10.3847/1538-4357/ad6565

Reference 45

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This paper cites 2025a, arXiv e-prints, arXiv:2505.02896, doi: 10.48550/arXiv.2505.02896.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots 2025a, arXiv e-prints, arXiv:2505.02896, doi: 10.48550/arXiv.2505.02896

Reference 46

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This paper cites 2025b, arXiv e-prints, arXiv:2507.10659.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots 2025b, arXiv e-prints, arXiv:2507.10659

Reference 47

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What you see is what you get: empirically measured bolometric luminosities of Little Red Dots E., & Ma, Y

Reference 48

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What you see is what you get: empirically measured bolometric luminosities of Little Red Dots L., Greene, J

Reference 49

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This paper cites 2024, A&A, 689, A128, doi: 10.1051/0004-6361/202451249.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots 2024, A&A, 689, A128, doi: 10.1051/0004-6361/202451249

Reference 50

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This paper cites UNCOVER: 404 Error -- Models Not Found for the Triply Imaged Little Red Dot A2744-QSO1.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots UNCOVER: 404 Error -- Models Not Found for the Triply Imaged Little Red Dot A2744-QSO1

Reference 51

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Observation 3324af72-b6cd-4ba3-bcde-f614d0d448a4 · outbound

This paper cites JADES. The diverse population of infant Black Holes at 4<z<11: merging, tiny, poor, but mighty.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots JADES. The diverse population of infant Black Holes at 4<z<11: merging, tiny, poor, but mighty

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:30.094026Z

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Observation cf04c2b2-c0ab-4d45-a90b-5ad095e54d52 · outbound

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

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots P., Brammer, G., et al

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:30.103627Z

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Unavailable: canonical work link unavailable.

Observation dc8b1906-2fec-49d6-b149-9a5f8d5952f6 · outbound

This paper cites Environmental Evidence for Overly Massive Black Holes in Low Mass Galaxies and a Black Hole - Halo Mass Relation at $z \sim 5$.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots Environmental Evidence for Overly Massive Black Holes in Low Mass Galaxies and a Black Hole - Halo Mass Relation at $z \sim 5$

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:30.108545Z

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Observation 14c87702-185c-47d9-8e5a-c7e4fb7cb780 · outbound

This paper cites All the Little Things in Abell 2744: $>$1000 Gravitationally Lensed Dwarf Galaxies at $z=0-9$ from JWST NIRCam Grism Spectroscopy.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots All the Little Things in Abell 2744: $>$1000 Gravitationally Lensed Dwarf Galaxies at $z=0-9$ from JWST NIRCam Grism Spectroscopy

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:30.114057Z

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Observation fd1380f5-684d-4b1a-89c8-d9d44357f87d · outbound

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

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots A "Black Hole Star" Reveals the Remarkable Gas-Enshrouded Hearts of the Little Red Dots

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:30.119834Z

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Unavailable: canonical work link unavailable.

Observation b49f522c-f705-497f-8fe0-4a48857604c8 · outbound

This paper cites 2025, A&A, 693, L2, doi: 10.1051/0004-6361/202452422.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots 2025, A&A, 693, L2, doi: 10.1051/0004-6361/202452422

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:30.125211Z

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Unavailable: canonical work link unavailable.

Observation 8e387bce-dba2-4e19-9b60-834cd4e3baa4 · outbound

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

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots F., Schaye, J., et al

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:30.130676Z

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Observation 9febfa37-3c14-40f1-8e94-36da3aa2633a · outbound

This paper cites The UNCOVER Survey: First Release of Ultradeep JWST/NIRSpec PRISM spectra for ~700 galaxies from z~0.3-13 in Abell 2744.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots The UNCOVER Survey: First Release of Ultradeep JWST/NIRSpec PRISM spectra for ~700 galaxies from z~0.3-13 in Abell 2744

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:30.135108Z

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Unavailable: canonical work link unavailable.

Observation d70af4b7-c0c1-48b0-81cf-ccef37ff2863 · outbound

This paper cites E., & Volonteri, M.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots E., & Volonteri, M

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:30.140031Z

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Unavailable: canonical work link unavailable.

Observation 39a7eb29-a911-418e-abbc-e04fa4bf4407 · outbound

This paper cites T., Lacy, M., Storrie-Lombardi, L.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots T., Lacy, M., Storrie-Lombardi, L

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:30.145127Z

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Unavailable: canonical work link unavailable.

Observation b09e5992-ad81-4abf-ba1f-724fae81d2b5 · outbound

This paper cites 2004, in Astrophysics and Space Science Library, Vol.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots 2004, in Astrophysics and Space Science Library, Vol

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:30.149400Z

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Unavailable: canonical work link unavailable.

Observation 85da8e48-bdb1-4c1a-aef7-fafb09484b1c · outbound

This paper cites P., et al.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots P., et al

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:30.154189Z

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Unavailable: canonical work link unavailable.

Observation 47c2c039-b64c-45c1-b0f4-289e3b001856 · outbound

This paper cites P., Opitsch, M., Erwin, P., et al.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots P., Opitsch, M., Erwin, P., et al

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:30.158645Z

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Unavailable: canonical work link unavailable.

Observation aaf3585e-da56-446a-810d-56c986338eac · outbound

This paper cites JADES: A large population of obscured, narrow line AGN at high redshift.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots JADES: A large population of obscured, narrow line AGN at high redshift

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:30.163491Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fe5e67a9-b503-4d60-a089-142f603e7e90 · outbound

This paper cites an unresolved cited work.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots Unresolved cited work

Reference 67

Resolution: verified exact; doi, observed 2026-08-05T05:29:30.846077Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 94f4386c-0cc5-4e5f-b21b-d500084cd082 · outbound

This paper cites Little Red Dots at an Inflection Point: Ubiquitous "V-Shaped" Turnover Consistently Occurs at the Balmer Limit.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots Little Red Dots at an Inflection Point: Ubiquitous "V-Shaped" Turnover Consistently Occurs at the Balmer Limit

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:30.178527Z

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Unavailable: canonical work link unavailable.

Observation 59b653b3-e742-4b90-ac93-7e3cff5cbd37 · outbound

This paper cites A confirmed deficit of hot and cold dust emission in the most luminous Little Red Dots.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots A confirmed deficit of hot and cold dust emission in the most luminous Little Red Dots

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:30.183520Z

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Unavailable: canonical work link unavailable.

Observation cb23ae2e-11bf-48c1-9fae-dcf379416b74 · outbound

This paper cites F., Faucher-Gigu` ere, C.-A., et al.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots F., Faucher-Gigu` ere, C.-A., et al

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:30.188146Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1a15da45-0974-4ddd-9b0e-95e1bad10673 · outbound

This paper cites an unresolved cited work.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots Unresolved cited work

Reference 71

Resolution: verified exact; doi, observed 2026-08-05T05:29:30.796311Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 8847092f-0ad7-4457-a762-100e94c9b859 · outbound

This paper cites 2012, MNRAS, 423, 600, doi: 10.1111/j.1365-2966.2012.20901.x.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots 2012, MNRAS, 423, 600, doi: 10.1111/j.1365-2966.2012.20901.x

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:30.196952Z

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Unavailable: canonical work link unavailable.

Observation 38018b8a-6cd8-4f08-9020-4a14b7a0a686 · outbound

This paper cites A., Weaver, J.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots A., Weaver, J

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:30.201527Z

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Unavailable: canonical work link unavailable.

Observation 67d76277-61cd-4673-bc41-54ee32717c86 · outbound

This paper cites JWST/NIRSpec Observations of High Ionization Emission Lines in Galaxies at High Redshift.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots JWST/NIRSpec Observations of High Ionization Emission Lines in Galaxies at High Redshift

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:30.206090Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 14fcc6ed-affc-4b64-84ec-9ab380455967 · outbound

This paper cites CAPERS-LRD-z9: A Gas Enshrouded Little Red Dot Hosting a Broad-line AGN at z=9.288.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots CAPERS-LRD-z9: A Gas Enshrouded Little Red Dot Hosting a Broad-line AGN at z=9.288

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:30.211213Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4fbbf18a-838a-4d29-98e2-2aa5dd64c0a6 · outbound

This paper cites 2025, arXiv e-prints, arXiv:2505.09542, doi: 10.48550/arXiv.2505.09542.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots 2025, arXiv e-prints, arXiv:2505.09542, doi: 10.48550/arXiv.2505.09542

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:30.216757Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7e5c8a39-6697-4800-9cca-e44ab2ca6238 · outbound

This paper cites UNCOVERing the High-redshift AGN Population among Extreme UV Line Emitters.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots UNCOVERing the High-redshift AGN Population among Extreme UV Line Emitters

Reference 77

Resolution: verified exact; local_arxiv, observed 2026-08-05T05:29:30.475481Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation ac7b1aef-cc77-46c8-90f8-187dd5620d01 · outbound

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

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots Episodic super-Eddington accretion as a clue to Overmassive Black Holes in the early Universe

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:30.226321Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 51854def-766e-499d-a794-f26d7b37ea4f · outbound

This paper cites V., & Fabian, A.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots V., & Fabian, A

Reference 79

Resolution: verified exact; arxiv_id_nonexistent, observed 2026-08-05T05:29:33.099543Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 62d9cd4e-a677-4de5-9626-45765d4e1fe0 · outbound

This paper cites an unresolved cited work.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots Unresolved cited work

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:30.237449Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bcf5751b-2cef-46ae-86c3-8699efcab9be · outbound

This paper cites 2010, A&A Rv, 18, 279, doi: 10.1007/s00159-010-0029-x.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots 2010, A&A Rv, 18, 279, doi: 10.1007/s00159-010-0029-x

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:30.244372Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fb10ca30-f173-4225-b27a-15d0ac3d8ca2 · outbound

This paper cites 2017, ApJ, 849, 155, doi: 10.3847/1538-4357/aa93f1.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots 2017, ApJ, 849, 155, doi: 10.3847/1538-4357/aa93f1

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:30.249249Z

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Unavailable: canonical work link unavailable.

Observation 85c00b8c-64d4-4021-ac54-9ac0c1a5cd9a · outbound

This paper cites RUBIES: JWST/NIRSpec Confirmation of an Infrared-luminous, Broad-line Little Red Dot with an Ionized Outflow.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots RUBIES: JWST/NIRSpec Confirmation of an Infrared-luminous, Broad-line Little Red Dot with an Ionized Outflow

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:30.254240Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 352ed1da-290c-487c-b218-3a887c025d05 · outbound

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

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots 2024b, ApJL, 969, L13, doi: 10.3847/2041-8213/ad55f7

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:30.259528Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1396a51b-9efa-49e8-b071-97cfcf08748e · outbound

This paper cites C., Alberts, S., Ji, Z., et al.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots C., Alberts, S., Ji, Z., et al

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:30.264455Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2474a039-777c-4d92-b18a-76373d9edd0d · outbound

This paper cites No [CII] or dust detection in two Little Red Dots at z$_{\rm spec}$ > 7.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots No [CII] or dust detection in two Little Red Dots at z$_{\rm spec}$ > 7

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:30.269648Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation eb9ece49-f990-4533-8c0a-c64c80e7485f · outbound

This paper cites an unresolved cited work.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots Unresolved cited work

Reference 87

Resolution: verified exact; doi, observed 2026-08-05T05:29:30.342335Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 10b11528-060f-44a6-b62d-56eb1325b8b0 · outbound

This paper cites T., et al.

What you see is what you get: empirically measured bolometric luminosities of Little Red Dots T., et al

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-05T05:29:30.278562Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Pith citing papers

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The mechanism for creating "dynamical gravastar" black hole mimickers also explains formation of "little red dots" What you see is what you get: empirically measured bolometric luminosities of Little Red Dots

Reference 6

Resolution: metadata mismatch; arxiv_id, observed 2026-05-21T21:20:38.833481Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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A first look at quasar-galaxy clustering at $z\simeq7.3$ What you see is what you get: empirically measured bolometric luminosities of Little Red Dots

Reference 41

Resolution: verified exact; arxiv_id, observed 2026-05-18T08:31:07.014280Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Little Red Dots as Hidden Neutrino Sources What you see is what you get: empirically measured bolometric luminosities of Little Red Dots

Reference 100

Resolution: verified exact; arxiv_id, observed 2026-05-16T13:42:56.343818Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Little Red Dots on FIRE: The Ability of Bursty Galaxies to Host an Abundant Population of High-Redshift AGN What you see is what you get: empirically measured bolometric luminosities of Little Red Dots

Reference 17

Resolution: verified exact; arxiv_id, observed 2026-05-16T09:27:40.575386Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Spectral Appearance of Self-gravitating Disks Powered by Stellar Objects: Universal Effective Temperature in the Optical Continuum and Application to Little Red Dots What you see is what you get: empirically measured bolometric luminosities of Little Red Dots

Reference 33

Resolution: verified exact; arxiv_id, observed 2026-05-16T06:22:26.956951Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-02T20:51:00.800152Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Hidden Monsters with SPHEREx I: A goldmine for heavily reddened quasars at cosmic noon What you see is what you get: empirically measured bolometric luminosities of Little Red Dots

Reference 26

Resolution: metadata mismatch; arxiv_id, observed 2026-05-11T01:10:53.393091Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Non-LTE atmosphere models of very luminous sources and their applicability to Little Red Dots, quasi-stars, and similar objects What you see is what you get: empirically measured bolometric luminosities of Little Red Dots

Reference 36

Resolution: metadata mismatch; arxiv_id, observed 2026-05-13T04:47:16.530524Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-02T13:59:31.117437Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Reference 45

Resolution: verified exact; arxiv_id, observed 2026-05-22T09:46:22.154612Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Reference 34

Resolution: metadata mismatch; arxiv_id, observed 2026-06-27T21:01:15.480229Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Reference 19

Resolution: verified exact; arxiv_id, observed 2026-06-27T16:21:01.732955Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 05ff2b4f-9c52-4609-9ae9-3500221b87a0 · inbound

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Resolution: verified exact; arxiv_id, observed 2026-06-27T07:00:40.181542Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Resolution: verified exact; arxiv_id, observed 2026-07-01T12:15:43.997975Z

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No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation f50a9719-d664-4892-b852-242d27f3137c · inbound

Unveil the nature of JWST-AGN and Little Red Dots with SKAO continuum surveys cites this paper.

Unveil the nature of JWST-AGN and Little Red Dots with SKAO continuum surveys What you see is what you get: empirically measured bolometric luminosities of Little Red Dots

Reference 59

Resolution: metadata mismatch; arxiv_id, observed 2026-07-01T06:25:27.974412Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 5a18e3f4-4c23-44bb-a186-70245f6b08e2 · inbound

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs cites this paper.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs What you see is what you get: empirically measured bolometric luminosities of Little Red Dots

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-01T00:25:31.840857Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.