Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at z < 0.35
Lasse Seyberlich, Sarah E. I. Bosman
astro-ph.GA
Submitted: 2026-08-05
Comments: 15 pages, 6 figures. Submitted to A&A
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Origins of the UV continuum and Balmer emission lines in Little Red Dots: observational validation of dense gas envelope models enshrouding the AGN
- From "The Cliff" to "Virgil": Mapping the Spectral Diversity of Little Red Dots with JWST/NIRSpec
- Do little red dots really form a distinct class of astronomical objects?
- A close look at the black hole masses and hot dusty toruses of the first quasars with MIRI-MRS
- Too Quiet for Comfort: Local Little Red Dots Lack Variability over Decades
- A Population of Little Red Dot-like Quasars in SDSS
- Little Red Dots as Globular Clusters in Formation
- Three Hundred Quasars from the Couch: A first look at high-redshift quasar discovery with SPHEREx
- Little Red Dots host Black Hole Stars: A unified family of gas-reddened AGN revealed by JWST/NIRSpec spectroscopy
- The DESI Experiment Part I: Science,Targeting, and Survey Design
- Discovery of low-redshift analogues to "Little Red Dots" in DESI: A later evolutionary stage of compact LRDs?
- Cosmology with the SPHEREX All-Sky Spectral Survey
- Euclid Quick Data Release (Q1). Extending the quest for little red dots to z<4
- Discovery of two little red dots transitioning into quasars
- The GlimmIr: Spectroscopic Variability in a z~7 LRD Indicates Rapid Changes in Both the Narrow and Broad Line Regions
- Local Analogs of Little Red Dots: Optical Variability and Evidence for an Active Galatic Nucleus Origin
- (LRDs)$^2$: The Low-ReDshift Little Red Dots Survey. II. DESI DR1 Sample
- The Balmer Break and Optical Continuum of Little Red Dots from Super-Eddington Accretion
- How I Wonder What You Are -- JWST's Little Red Dots do not TWINKLE
- The Engine and its Flows: Little Red Dot spectra are shaped by the column densities of their gas envelopes
Related papers
- Apparent Stability in Self-Gravitating Turbulence and the Evolution of Molecular Clouds
- Two sets of potential-density basis pairs for the study of radial perturbations in collisionless spherical stellar systems
- Constraining reionization-era Ly alpha escape with JELS-MUSE: a highly complete H alpha-selected sample at z about6.1
- Deriving volume density profiles of filaments from observed surface densities
- Little Red Dots and Supermassive Black Hole Seed Formation in Ultralight Dark Matter Halos
- MEGATRON: how the first stars can create an iron metallicity plateau in the smallest dwarf galaxies