---
DOAJ_listed: '1'
OA_place: publisher
OA_type: gold
PlanS_conform: '1'
_id: '21715'
abstract:
- lang: eng
  text: New populations of red active galactic nuclei (known as “little red dots”)
    discovered by JWST exhibit remarkable spectral energy distributions. Leveraging
    X-ray through far-infrared observations of two of the most luminous known little
    red dots, we directly measure their bolometric luminosities. We find evidence
    that more than half of the bolometric luminosity likely emerges in the rest-frame
    optical, with Lbol/L5100 = 5, roughly half the value for “standard” active galactic
    nuclei. Meanwhile, the X-ray emitting corona, UV-emitting blackbody, and reprocessed
    mid to far-infrared emission are all considerably subdominant, assuming that the
    far-infrared luminosity is well below current measured limits. We present new
    bolometric corrections that dramatically lower inferred bolometric luminosities
    by a factor of 10 compared to published values in the literature. These bolometric
    corrections are in accord with expectations from models in which gas absorption
    and reprocessing are responsible for the red rest-frame optical colors of little
    red dots. We discuss how this lowered luminosity scale suggests a lower mass scale
    for the population by at least an order of magnitude (e.g., ∼105–107 M⊙ black
    holes, and ∼108 M⊙ galaxies), alleviating tensions with clustering, overmassive
    black holes, and the integrated black hole mass density in the Universe.
acknowledgement: "We benefit from the following JWST programs: UNCOVER (JWST/GO #2561;
  Labbé & Bezanson); ALT (JWST-GO #3516; Naidu & Matthee); MegaScience (JWST-GO #4111;
  Suess); RUBIES (JWST-GO #4233; de Graaff & Brammer); PRIMER (JWST/GO #1837; Dunlop).\r\n\r\nWe
  acknowledge funding from NSF/AAG #2306950, JWST-GO-02561, JWST-GO-03516, and JWST-GO-04111,
  provided through a grant from the STScI under NASA contract NAS5-03127. I.L. acknowledges
  support from Australian Research Council Future Fellowship FT220100798. K.G. and
  T.N. acknowledge support from Australian Research Council Laureate Fellowship FL180100060.
  A.Z. acknowledges support by grant No. 2020750 from the United States-Israel Binational
  Science Foundation (BSF) and grant No. 2109066 from the United States National Science
  Foundation (NSF); by the Ministry of Science & Technology, Israel; and by the Israel
  Science Foundation grant No. 864/23. J.M. and I.K. are funded by the European Union
  (ERC, AGENTS, 101076224). Views and opinions expressed are, however, those of the
  author(s) only and do not necessarily reflect those of the European Union or the
  European Research Council. Neither the European Union nor the granting authority
  can be held responsible for them. Y.F. acknowledges support from JSPS KAKENHI grant
  No. JSPS KAKENHI grant Nos. JP22K21349 and JP23K13149. This work has received funding
  from the Swiss State Secretariat for Education, Research and Innovation (SERI) under
  contract No. MB22.00072, as well as from the Swiss National Science Foundation (SNSF)
  through project grant 200020_207349. The Cosmic Dawn Center (DAWN) is funded by
  the Danish National Research Foundation under grant DNRF140. Support for this work
  for RPN was provided by NASA through the NASA Hubble Fellowship grant HST-HF2-51515.001-A
  awarded by the Space Telescope Science Institute, which is operated by the Association
  of Universities for Research in Astronomy, Incorporated, under NASA contract NAS5-26555.
  The work of CCW is supported by NOIRLab, which is managed by the Association of
  Universities for Research in Astronomy (AURA) under a cooperative agreement with
  the National Science Foundation. J.M. acknowledges funding by the European Union
  (ERC, AGENTS, 101076224). R.E.H. acknowledges support by the German Aerospace Center
  (DLR) and the Federal Ministry for Economic Affairs and Energy (BMWi) through program
  50OR2403 “RUBIES.”"
article_number: '129'
article_processing_charge: Yes
article_type: original
arxiv: 1
author:
- first_name: Jenny E.
  full_name: Greene, Jenny E.
  last_name: Greene
- first_name: David J.
  full_name: Setton, David J.
  last_name: Setton
- first_name: Lukas J.
  full_name: Furtak, Lukas J.
  last_name: Furtak
- first_name: Rohan P.
  full_name: Naidu, Rohan P.
  last_name: Naidu
- first_name: Marta
  full_name: Volonteri, Marta
  last_name: Volonteri
- first_name: Pratika
  full_name: Dayal, Pratika
  last_name: Dayal
- first_name: Ivo
  full_name: Labbe, Ivo
  last_name: Labbe
- first_name: Pieter
  full_name: Van Dokkum, Pieter
  last_name: Van Dokkum
- first_name: Rachel
  full_name: Bezanson, Rachel
  last_name: Bezanson
- first_name: Gabriel
  full_name: Brammer, Gabriel
  last_name: Brammer
- first_name: Sam E.
  full_name: Cutler, Sam E.
  last_name: Cutler
- first_name: Karl
  full_name: Glazebrook, Karl
  last_name: Glazebrook
- first_name: Anna
  full_name: De Graaff, Anna
  last_name: De Graaff
- first_name: Michaela
  full_name: Hirschmann, Michaela
  last_name: Hirschmann
- first_name: Raphael E.
  full_name: Hviding, Raphael E.
  last_name: Hviding
- first_name: Vasily
  full_name: Kokorev, Vasily
  last_name: Kokorev
- first_name: Joel
  full_name: Leja, Joel
  last_name: Leja
- first_name: Hanpu
  full_name: Liu, Hanpu
  last_name: Liu
- first_name: Yilun
  full_name: Ma, Yilun
  last_name: Ma
- first_name: Jorryt J
  full_name: Matthee, Jorryt J
  id: 7439a258-f3c0-11ec-9501-9df22fe06720
  last_name: Matthee
  orcid: 0000-0003-2871-127X
- first_name: Themiya
  full_name: Nanayakkara, Themiya
  last_name: Nanayakkara
- first_name: Pascal A.
  full_name: Oesch, Pascal A.
  last_name: Oesch
- first_name: Richard
  full_name: Pan, Richard
  last_name: Pan
- first_name: Sedona H.
  full_name: Price, Sedona H.
  last_name: Price
- first_name: Justin S.
  full_name: Spilker, Justin S.
  last_name: Spilker
- first_name: Bingjie
  full_name: Wang, Bingjie
  last_name: Wang
- first_name: John R.
  full_name: Weaver, John R.
  last_name: Weaver
- first_name: Katherine E.
  full_name: Whitaker, Katherine E.
  last_name: Whitaker
- first_name: Christina C.
  full_name: Williams, Christina C.
  last_name: Williams
- first_name: Adi
  full_name: Zitrin, Adi
  last_name: Zitrin
citation:
  ama: 'Greene JE, Setton DJ, Furtak LJ, et al. What you see is what you get: Empirically
    measured bolometric luminosities of Little Red Dots. <i>The Astrophysical Journal</i>.
    2026;996(2). doi:<a href="https://doi.org/10.3847/1538-4357/ae1836">10.3847/1538-4357/ae1836</a>'
  apa: 'Greene, J. E., Setton, D. J., Furtak, L. J., Naidu, R. P., Volonteri, M.,
    Dayal, P., … Zitrin, A. (2026). What you see is what you get: Empirically measured
    bolometric luminosities of Little Red Dots. <i>The Astrophysical Journal</i>.
    IOP Publishing. <a href="https://doi.org/10.3847/1538-4357/ae1836">https://doi.org/10.3847/1538-4357/ae1836</a>'
  chicago: 'Greene, Jenny E., David J. Setton, Lukas J. Furtak, Rohan P. Naidu, Marta
    Volonteri, Pratika Dayal, Ivo Labbe, et al. “What You See Is What You Get: Empirically
    Measured Bolometric Luminosities of Little Red Dots.” <i>The Astrophysical Journal</i>.
    IOP Publishing, 2026. <a href="https://doi.org/10.3847/1538-4357/ae1836">https://doi.org/10.3847/1538-4357/ae1836</a>.'
  ieee: 'J. E. Greene <i>et al.</i>, “What you see is what you get: Empirically measured
    bolometric luminosities of Little Red Dots,” <i>The Astrophysical Journal</i>,
    vol. 996, no. 2. IOP Publishing, 2026.'
  ista: 'Greene JE, Setton DJ, Furtak LJ, Naidu RP, Volonteri M, Dayal P, Labbe I,
    Van Dokkum P, Bezanson R, Brammer G, Cutler SE, Glazebrook K, De Graaff A, Hirschmann
    M, Hviding RE, Kokorev V, Leja J, Liu H, Ma Y, Matthee JJ, Nanayakkara T, Oesch
    PA, Pan R, Price SH, Spilker JS, Wang B, Weaver JR, Whitaker KE, Williams CC,
    Zitrin A. 2026. What you see is what you get: Empirically measured bolometric
    luminosities of Little Red Dots. The Astrophysical Journal. 996(2), 129.'
  mla: 'Greene, Jenny E., et al. “What You See Is What You Get: Empirically Measured
    Bolometric Luminosities of Little Red Dots.” <i>The Astrophysical Journal</i>,
    vol. 996, no. 2, 129, IOP Publishing, 2026, doi:<a href="https://doi.org/10.3847/1538-4357/ae1836">10.3847/1538-4357/ae1836</a>.'
  short: J.E. Greene, D.J. Setton, L.J. Furtak, R.P. Naidu, M. Volonteri, P. Dayal,
    I. Labbe, P. Van Dokkum, R. Bezanson, G. Brammer, S.E. Cutler, K. Glazebrook,
    A. De Graaff, M. Hirschmann, R.E. Hviding, V. Kokorev, J. Leja, H. Liu, Y. Ma,
    J.J. Matthee, T. Nanayakkara, P.A. Oesch, R. Pan, S.H. Price, J.S. Spilker, B.
    Wang, J.R. Weaver, K.E. Whitaker, C.C. Williams, A. Zitrin, The Astrophysical
    Journal 996 (2026).
date_created: 2026-04-12T22:01:50Z
date_published: 2026-01-10T00:00:00Z
date_updated: 2026-05-04T11:20:42Z
day: '10'
ddc:
- '520'
department:
- _id: JoMa
doi: 10.3847/1538-4357/ae1836
external_id:
  arxiv:
  - '2509.05434'
file:
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has_accepted_license: '1'
intvolume: '       996'
issue: '2'
language:
- iso: eng
month: '01'
oa: 1
oa_version: Published Version
project:
- _id: bd9b2118-d553-11ed-ba76-db24564edfea
  grant_number: '101076224'
  name: Young galaxies as tracers and agents of cosmic reionization
publication: The Astrophysical Journal
publication_identifier:
  eissn:
  - 1538-4357
  issn:
  - 0004-637X
publication_status: published
publisher: IOP Publishing
quality_controlled: '1'
scopus_import: '1'
status: public
title: 'What you see is what you get: Empirically measured bolometric luminosities
  of Little Red Dots'
tmp:
  image: /images/cc_by.png
  legal_code_url: https://creativecommons.org/licenses/by/4.0/legalcode
  name: Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)
  short: CC BY (4.0)
type: journal_article
user_id: 2DF688A6-F248-11E8-B48F-1D18A9856A87
volume: 996
year: '2026'
...
