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Since the launch of James Webb Space Telescope (JWST) in late 2021, our understanding of high-redshift objects has faced several upheavals. JWST has discovered much more massive galaxies and supermassive black holes (SMBH) than cosmological…

Astrophysics of Galaxies · Physics 2026-01-05 David D Vaida , Ryan Jeffrey Farber

The James Webb Space Telescope (JWST) observations have identified a class of compact galaxies at high redshifts ($4 \lesssim z \lesssim 11$), dubbed "little red dots" (LRDs). The supermassive black holes (SMBHs) of…

Cosmology and Nongalactic Astrophysics · Physics 2025-07-24 Borui Zhang , Wei-Xiang Feng , Haipeng An

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). The nature of these galaxies is debated and is…

The discovery of Little Red Dots (LRDs) -- a population of compact, high-redshift, dust-reddened galaxies -- is one of the most surprising results from JWST. However, the nature of LRDs is still debated: does the near-infrared emission…

Astrophysics of Galaxies · Physics 2024-06-14 Tonima Tasnim Ananna , Ákos Bogdán , Orsolya E. Kovács , Priyamvada Natarajan , Ryan C. Hickox

The James Webb Space Telescope has detected massive black holes (BHs) with masses of $\sim 10^{6-8}~M_\odot$ within the first billion years of the universe. One of the remarkable findings is the identification of "Little Red Dots" (LRDs), a…

Astrophysics of Galaxies · Physics 2025-07-17 Kohei Inayoshi

The James Webb Space Telescope (JWST) has discovered a new population of objects, the Little Red Dots (LRDs), characterized by V-shaped spectra indicative of strong breaks around the Balmer limit and compact morphology that gave them their…

One of the most puzzling discoveries by JWST is the population of high-redshift, red, and compact galaxies dubbed little red dots (LRDs). Based on broad-line diagnostics, these galaxies have been argued to host accreting $10^7-10^8$…

Astrophysics of Galaxies · Physics 2025-07-30 Andrea Sacchi , Akos Bogdan

The James Webb Space Telescope (JWST) has uncovered a population of compact, high-redshift sources, the Little Red Dots (LRDs), which may host supermassive black holes (BHs) significantly heavier than their stellar content compared with…

Cosmology and Nongalactic Astrophysics · Physics 2025-12-23 Valerio De Luca , Loris Del Grosso , Gabriele Franciolini , Konstantinos Kritos , Emanuele Berti , Daniel D'Orazio , Joseph Silk

The advent of the James Webb Space Telescope has revolutionised our understanding of the high-redshift Universe through its detection of bright, massive galaxies up to $z\gtrsim 10$ and its identification of peculiar sources called `little…

Astrophysics of Galaxies · Physics 2026-01-14 Giada Quadri , Alessandro Trinca , Alessandro Lupi , Monica Colpi , Marta Volonteri

JWST has revealed a population of low-luminosity AGN at $z>4$ in compact, red hosts (the "Little Red Dots", or LRDs), which are largely undetected in X-rays. We investigate this phenomenon using GRRMHD simulations of super-Eddington…

High Energy Astrophysical Phenomena · Physics 2024-11-15 Fabio Pacucci , Ramesh Narayan

Little Red Dots (LRDs) are a newly identified class of active galactic nuclei (AGNs) uncovered by JWST deep surveys. Their enigmatic properties challenge the canonical AGN paradigm and have stimulated ideas on early massive black hole (BH)…

Astrophysics of Galaxies · Physics 2025-12-04 Kohei Inayoshi , Luis C. Ho

JWST is revolutionizing our view of the early Universe by pushing the boundaries of detectable galaxies and black holes in redshift (upward) and mass (downward). The Little Red Dots (LRDs), detected by several surveys at $z > 4$, present a…

Astrophysics of Galaxies · Physics 2025-05-23 Emmanuel Durodola , Fabio Pacucci , Ryan C. Hickox

Little Red Dots (LRDs), among the most enigmatic high-redshift discoveries by JWST, are commonly believed to be powered by accreting supermassive black holes. Here, we explore the possibility that these sources are globular clusters in…

Little Red Dots (LRDs), newly identified compact and dusty galaxies with an unexpectedly high number density observed by JWST, have an unusual "V-shaped" rest-frame UV to near-infrared spectral energy distribution (SED). A group of…

We investigate the possibility that the recently identified population of high-redshift, obscured quasars - known as "Little Red Dots" (LRDs) - originates from early black hole seed formation driven by ultra-strongly self-interacting dark…

Astrophysics of Galaxies · Physics 2026-03-10 M. Grant Roberts , Lila Braff , Aarna Garg , Stefano Profumo , Tesla Jeltema

Recent observations by the James Webb Space Telescope (JWST) have revealed a previously hidden population of extremely bright and compact objects between redshifts of $z \sim 4$ and $z \sim 10$. Given their extreme red colouring in the…

Astrophysics of Galaxies · Physics 2024-09-23 Jake Feeney , Patrick Kavanagh , John A. Regan

As an unprecedented large population in the early universe, the JWST-discovered little red dots (LRDs) have garnered much attention for formation of massive black holes and galaxies, but their nature remains a mystery. The LRDs appearing as…

Astrophysics of Galaxies · Physics 2025-11-13 Jian-Min Wang , Yi-Lin Wang , Yong-Jie Chen , Jun-Rong Liu , Yu-Yang Songsheng , Cheng Cheng , Yan-Rong Li , Pu Du , Hao Zhang , Yu Zhao

JWST has revealed an abundant population of compact, low-metallicity "Little Red Dots" (LRDs) at high redshift, challenging conventional scenarios in which supermassive black holes (SMBHs) grow from stellar-mass seeds. We consider a…

High Energy Physics - Phenomenology · Physics 2026-04-03 Jinhui Guo , Jia Liu , Masanori Tanaka , Xiao-Ping Wang , Huangyu Xiao

Little Red Dots (LRDs) are enigmatic, compact, red galaxies at high redshift, $z\sim 4$-$7$, discovered by the James Webb Space Telescope. Broad emission lines in the absence of X-ray and radio counterparts suggest that they host accreting…

High Energy Astrophysical Phenomena · Physics 2026-04-29 Riku Kuze , Kunihito Ioka , Kohta Murase , Shigeo S. Kimura , Kohei Inayoshi
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