JADES-GN+189.26978+62.19421 , the SIMBAD biblio

JADES-GN+189.26978+62.19421 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST17:46:09


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Title First 3 Authors
2023ApJS..269...16R viz 17       D               1 2653 ~ JADES Initial Data Release for the Hubble Ultra Deep Field: Revealing the Faint Infrared Sky with Deep JWST NIRCam Imaging. RIEKE M.J., ROBERTSON B., TACCHELLA S., et al.
2024AJ....167..251L 18       D               1 20 ~ Radio Emission from High-redshift Active Galactic Nuclei in the JADES and CEERS Surveys. LATIF M.A., AFTAB A. and WHALEN D.J.
2024ApJ...974L..26Y 18       D               3 17 ~ Stacking X-Ray Observations of “Little Red Dots”: Implications for Their Active Galactic Nucleus Properties. YUE M., EILERS A.-C., ANANNA T.T., et al.
2024A&A...691A.145M 18       D               3 17 ~ JADES The diverse population of infant black holes at 4 < z < 11: Merging, tiny, poor, but mighty. MAIOLINO R., SCHOLTZ J., CURTIS-LAKE E., et al.
2025ApJ...981...19L 19       D               1 23 ~ Tip of the Iceberg: Overmassive Black Holes at 4 < z < 7 Found by JWST Are Not Inconsistent with the Local ${{ \mathcal M }}_{\mathrm{BH}}-{{ \mathcal M }}_{\star }$ Relation. LI J., SILVERMAN J.D., SHEN Y., et al.
2025MNRAS.538.1921M 19       D               1 79 ~ JWST meets Chandra: a large population of Compton thick, feedback-free, and intrinsically X-ray weak AGN, with a sprinkle of SNe. MAIOLINO R., RISALITI G., SIGNORINI M., et al.
2025ApJ...986..177B 159       D     X         4 19 ~ Here There Be (Dusty) Monsters: High-redshift Active Galactic Nuclei Are Dustier than Their Hosts. BROOKS M., SIMONS R.C., TRUMP J.R., et al.
2025ApJ...988L..61C 19       D               1 30 ~ Evidence for Evolutionary Pathway-dependent Black Hole Scaling Relations. COHN J.H., DURODOLA E., CASEY Q.O., et al.
2025ApJ...991..217T 19       D               1 32 ~ JWST/NIRSpec Observations of High-ionization Emission Lines in Galaxies at High Redshift. TANG M., STARK D.P., PLAT A., et al.
2026ApJ..1000..100D 20       D               1 13 ~ Causal Reversal in the M•-σ0 Relation: Implications for High-redshift Supermassive Black Hole Mass Estimates. DAVIS B.L., MORE S., JIN Z., et al.

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