UNCOVER DR1 28343 , the SIMBAD biblio

UNCOVER DR1 28343 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST03:17:42


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Title First 3 Authors
2024ApJ...964...39G 18       D               3 15 ~ UNCOVER Spectroscopy Confirms the Surprising Ubiquity of Active Galactic Nuclei in Red Sources at z > 5. GREENE J.E., LABBE I., GOULDING A.D., et al.
2024ApJ...969L..18A 18       D               1 24 ~ X-Ray View of Little Red Dots: Do They Host Supermassive Black Holes? ANANNA T.T., BOGDAN A., KOVACS O.E., et al.
2024A&A...690A.182D 18       D               1 31 ~ Exploring a primordial solution for early black holes detected with JWST. DAYAL P.
2025ApJ...978...92L 19       D               2 39 ~ UNCOVER: Candidate Red Active Galactic Nuclei at 3 < z < 7 with JWST and ALMA. LABBE I., GREENE J.E., BEZANSON R., et al.
2025ApJ...983...60C 467     A D     X C       10 9 ~ The Host Galaxy (If Any) of the Little Red Dots. CHEN C.-H., HO L.C., LI R., et al.
2025ApJ...986..126K 93           X         2 32 ~ The Rise of Faint, Red Active Galactic Nuclei at z > 4: A Sample of Little Red Dots in the JWST Extragalactic Legacy Fields. KOCEVSKI D.D., FINKELSTEIN S.L., BARRO G., et al.
2025A&A...698A.317M 47           X         1 2 ~ Possible environmental quenching in an interacting little red dot pair at z ∼ 7. MERIDA R.M., GASPAR G., SAWICKI M., et al.
2025ApJ...988..246M 299       D     X C       6 11 ~ Environmental Evidence for Overly Massive Black Holes in Low-mass Galaxies and a Black Hole-Halo Mass Relation at z ∼ 5. MATTHEE J., NAIDU R.P., KOTIWALE G., et al.
2025ApJ...995...24K 1931       D S   X C       40 18 ~ Challenging the Active Galactic Nucleus Scenario for JWST/NIRSpec Little Red Dot and Non-Little Red Dot Broad Hα Emitters in Light of Nondetection of NIRCam Photometric Variability and X-Ray. KOKUBO M. and HARIKANE Y.
2026ApJ...999...30C 20       D               1 8 ~ A z ≃ 0.4 Galaxy Reflecting the High-redshift Little Red Dots: An Extended Starburst with an Overmassive Black Hole. CHEN X., ICHIKAWA K., AKIYAMA M., et al.

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