Eight low-redshift Little Red Dots identified in DESI DR1 exhibit broad Balmer lines, steep decrements, compact shapes, and negligible variability, with a number density roughly 10,000 times lower than at z>4.
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Spectrophotometry of 11 low-mass galaxies with extreme O32 ratios yields helium and oxygen abundances plus line-specific velocity dispersions that differ between inner and outer HII-region zones.
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A new sample of Little Red Dots at $z<0.45$ in DESI DR1: Broad Balmer lines, low ionization spectrum and no variability
Eight low-redshift Little Red Dots identified in DESI DR1 exhibit broad Balmer lines, steep decrements, compact shapes, and negligible variability, with a number density roughly 10,000 times lower than at z>4.
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Chemical composition and kinematics of ionised gas in low-mass star-forming galaxies with extremely high [OIII]/[OII] ratios
Spectrophotometry of 11 low-mass galaxies with extreme O32 ratios yields helium and oxygen abundances plus line-specific velocity dispersions that differ between inner and outer HII-region zones.