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most citedThe Rise of Faint, Red AGN at : A Sample of Little Red Dots in the JWST Extragalactic Legacy Fields

23 citations · 124 across the 25 of their papers we have counts for

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astro-ph.GA2024★ 10 cited

PICZL: Image-based Photometric Redshifts for AGN

William Roster, Mara Salvato, Sven Krippendorf +14

Computing photo-z for AGN is challenging, primarily due to the interplay of relative emissions associated with the SMBH and its host galaxy. SED fitting methods, effective in penci…

astro-ph.HE2024★ 1 cited

Systematic Collapse of the Accretion Disc Across the Supermassive Black Hole Population

Scott Hagen, Chris Done, John D. Silverman +7

The structure of the accretion flow onto supermassive black holes (SMBH) is not well understood. Standard disc models match to zeroth order in predicting substantial energy dissipa…

astro-ph.GA2024★ 20 cited

Genuine Retrieval of the AGN Host Stellar Population (GRAHSP)

Johannes Buchner, Hattie Starck, Mara Salvato +11

The assembly and co-evolution of supermassive black holes (SMBH) and their host galaxy stellar population is a key open questions in galaxy evolution. Stellar mass () and…

astro-ph.GA2024★ 7 cited

Morphological Evidence for the eROSITA Bubbles Being Giant and Distant Structures

Teng Liu, Andrea Merloni, Jeremy Sanders +13

There are two contradictory views of the eROSITA bubbles: either a 10 kpc-scale pair of giant bubbles blown by the Galactic center (GC), or a 100 pc-scale local structure coinciden…

astro-ph.GA2024★ 23 cited

The Rise of Faint, Red AGN at : A Sample of Little Red Dots in the JWST Extragalactic Legacy Fields

Dale D. Kocevski, Steven L. Finkelstein, Guillermo Barro +54

We present a sample of 341 "little red dots" (LRDs) spanning the redshift range using data from the CEERS, PRIMER, JADES, UNCOVER and NGDEEP surveys. Unlike past use of…

astro-ph.GA2024★ 18 cited

Accretion properties of X-ray AGN: Evidence for radiation-regulated obscuration with redshift-dependent host galaxy contribution

Brivael Laloux, Antonis Georgakakis, David M. Alexander +12

We adopt a Bayesian X-ray spectral approach to investigate the accretion properties of unobscured () and obscured ($22< \log(N_{\rm H}/{\rm cm}^…