Little red dots as obscured little blue dots: relative abundances, luminosities, and black-hole masses
astro-ph.GA, astro-ph.HE
Submitted: 2026-05-06
Updated: 2026-09-08
Comments: revised version, submitted to A&A
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Connecting the Dots: UV-Bright Companions of Little Red Dots as Lyman-Werner Sources Enabling Direct Collapse Black Hole Formation
- Do little red dots really form a distinct class of astronomical objects?
- The Little Blue and Red Dots Rosetta Stones: Non-Gaussian broad lines, hot dust, and X-ray weakness
- Little Red Dots host Black Hole Stars: A unified family of gas-reddened AGN revealed by JWST/NIRSpec spectroscopy
- BlackTHUNDER strikes twice: rest-frame Balmer-line absorption and high Eddington accretion rate in a Little Red Dot at $z=7.04$
- Irony at z=6.68: a bright AGN with forbidden Fe emission and multi-component Balmer absorption
- Holes in the BH$^\star$? AGN signatures in the FUV spectrum of a black-hole dominated Little Red Dot at $z=7.04$
- 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
- Little Red Dots as Obscured Little Blue Dots: A Super-Eddington Unification Model
- A "Black Hole Star" Reveals the Remarkable Gas-Enshrouded Hearts of the Little Red Dots
- The Little Red Dots Are Direct Collapse Black Holes
- SPURS: Evidence for Clumpy Neutral Envelopes and Ionized IGM Surrounding Little Red Dots in Abell 2744 from Ultra-Deep Rest-UV Spectroscopy
- You can't see me: Super-Eddington growth hindering X-ray detection in high-z broad-line active galactic nuclei
- Balmer Transition Signatures from Gas-Enshrouded, Dust-Poor Active Galactic Nuclei
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