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The James Webb Space Telescope (JWST) has uncovered many compact galaxies at high redshift with broad hydrogen and helium lines, including the enigmatic population of little red dots (LRDs).
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Nature Methods
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“Spectroscopic follow-up of ultra-high-z candidates in CEERS: Characterizing true z ¿ 12 galaxies and z 4-7 interlopers in preparation for JWST Cycle 2”
Arrabal Haro, P., Dickinson, M., Bagley, M., Burgarella, D. et al · 2022
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Eisenstein, D. J., Willott, C., Alberts, S., Arribas, S. et al., “Overview of the JWST Advanced Deep Extragalactic Survey (JADES)” · 2023
Cited alongside, same era.
Eisenstein, D. J., Johnson, B. D., Robertson, B., Tacchella, S. et al., “The JADES Origins Field: A New JWST Deep Field in the JADES Second NIRCam Data Release” · 2023
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“Extremely massive galaxies in the early universe: a challenge to Lambda-CDM?”
Nelson, E., Labbe, I., Benton, C., Bezanson, R. et al · 2023
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“JWST NIRSpec/NIRCam Follow-Up of the High-Redshift Transients Discovered in the GOODS-S JADES-Deep Field”
Lambrides, E., Garofali, K., Larson, R., Ptak, A. et al., “The Case for Super-Eddington Accretion: Connecting Weak X-ray and UV Line Emission in JWST Broad-Line AGN During the First Gyr of Cosmic Time” · 2024
Later among the works it cites.
Ji, X., Maiolino, R., Übler, H., Scholtz, J. et al., “BlackTHUNDER – A non-stellar Balmer break in a black hole-dominated little red dot at z = 7.04 z=7.04 ” · 2025
Closest in time.
Akins, H. B., Casey, C. M., Chisholm, J., Berg, D. A. et al., “Tentative detection of neutral gas in a Little Red Dot at z = 4.46 z=4.46 ” · 2025
Closest in time.
The Open Journal of Astrophysics
Katz, H., Cameron, A. J., Saxena, A., Barrufet, L. et al., “21 Balmer Jump Street: The Nebular Continuum at High Redshift and Implications for the Bright Galaxy Problem, UV Continuum Slopes, and Early Stellar Populations” · 2025
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Egami, E., Bonaventura, N., Charlot, S., Curti, M. et al · 2023
Cited alongside, same era.
“ msaexp
Brammer, G · 2023
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Advances in Space Research
Dojčinović, I., Kovačević-Dojčinović, J. and Popović, L. Č., “The flux ratio of the [N II] λ \lambda λ \lambda 6548, 6583 Å lines in sample of Active Galactic Nuclei Type 2” · 2023
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Egami, E., Sun, F., Alberts, S., Baum, S. A. et al · 2023
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Brammer, G · 2023
Cited alongside, same era.
Kokubo, M. and Harikane, Y., “Challenging the AGN scenario for JWST/NIRSpec broad H α \alpha emitters/Little Red Dots in light of non-detection of NIRCam photometric variability and X-ray” · 2024
Cited alongside, same era.
Mazzolari, G., Gilli, R., Maiolino, R., Prandoni, I. et al., “The radio properties of the JWST-discovered AGN” · 2024
Cited alongside, same era.
Setton, D. J., Greene, J. E., de Graaff, A., Ma, Y. et al., “Little Red Dots at an Inflection Point: Ubiquitous “V-Shaped” Turnover Consistently Occurs at the Balmer Limit” · 2024
Cited alongside, same era.
Naidu, R. P., Matthee, J., Katz, H., de Graaff, A. et al., “A “Black Hole Star” Reveals the Remarkable Gas-Enshrouded Hearts of the Little Red Dots” · 2025
Closest in time.
Juodžbalis, I., Maiolino, R., Baker, W. M., Lake, E. C. et al., “JADES: comprehensive census of broad-line AGN from Reionization to Cosmic Noon revealed by JWST” · 2025
Closest in time.
Nikopoulos, G. P., Watson, D., Sneppen, A., Rusakov, V. et al., “Evidence of violation of Case B recombination in Little Red Dots” · 2025
Closest in time.
D’Eugenio, F., Nelson, E., Ji, X., Baggen, J. et al., “Irony at z=6.68: a bright AGN with forbidden Fe emission and multi-component Balmer absorption” · 2025
Closest in time.
Hviding, R. E., de Graaff, A., Miller, T. B., Setton, D. J. et al., “RUBIES: A Spectroscopic Census of Little Red Dots; All V-Shaped Point Sources Have Broad Lines” · 2025
Closest in time.
D’Eugenio, F., Maiolino, R., Perna, M., Uebler, H. et al., “BlackTHUNDER strikes twice: rest-frame Balmer-line absorption and high Eddington accretion rate in a Little Red Dot at z = 7.04 z=7.04 ” · 2025
Closest in time.
Juodžbalis, I., Maiolino, R., Baker, W. M., Lake, E. C. et al., “JADES: comprehensive census of broad-line AGN from Reionization to Cosmic Noon revealed by JWST” · 2025
Closest in time.