activity
20122026
most citedOccupation of X-ray selected galaxy groups by X-ray AGN

76 citations · 269 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.GA2026

Common Excitation Patterns of Star Formation, Active Galactic Nuclei, and Shocks in Seyfert Galaxies

Peixin Zhu, Lisa J. Kewley, Dominika Ł. Król +6

The growth of galaxies and their central supermassive black holes is closely connected, yet the net effect of active galactic nuclei (AGN) feedback on host-galaxy star formation re…

astro-ph.GA2026

Local Heavily Obscured Active Galaxies Observed With Chandra (I): Spectral Properties of the Nuclear and Extended X-ray Emission

R. Middei, G. Fabbiano, A. Trindade Falcão +3

The Chandra X-ray Observatory has revealed that kiloparsec-scale extended X-ray emission is commonly associated with heavily absorbed (/cm) Active Gala…

astro-ph.GA2026

The Dyson Minds 2025 Workshop: SETI around Black Holes

Olivia Curtis, Van Hunter Adams, Daniel Angerhausen +9

The Dyson Minds 2025 Workshop, held at the Center for Brains, Minds & Machines at MIT and organized by Penn State, MIT, and The Ultraintelligence Foundation, brought together resea…

astro-ph.HE2025★ 2 cited

Probing AGN-ISM Feedback through Extended X-ray Emission in ESO 137-G034

D. Ł. Król, G. Fabbiano, M. Elvis +6

We present a detailed analysis of the X-ray emission of the Compton-thick (CT) AGN ESO\,137-G034 based on deep (\,ks) Chandra observations. As in other CT AGNs, the morpho…

astro-ph.GA2025

X-ray view of a massive node of the Cosmic Web at z=3 II. Discovery of extended X-ray emission around a hyperluminous QSO

Andrea Travascio, Sebastiano Cantalupo, Gabriele Pezzulli +17

While the warm, ionized gas in the CGM at z>3 is now routinely observed around bright QSOs in Lya emission, little is known about the CGM hot phase due to its expected faintness in…

astro-ph.GA2025★ 3 cited

Mapping the Excitation Mechanisms in the LINER I Active Galactic Nucleus NGC 5005: Positive Feedback and a Thin LINER Cocoon

Anna Trindade Falcão, G. Fabbiano, M. Elvis +5

We present a spatially resolved Baldwin-Phillips-Terlevich analysis of the narrow-line region (NLR) in the low-ionization nuclear emission-line region (LINER) I galaxy NGC 5005 usi…

astro-ph.HE2016★ 39 cited

The weak neutral Fe fluorescence line and long-term X-ray evolution of the Compton-thick AGN in NGC 7674

P. Gandhi, A. Annuar, G. B. Lansbury +26

We present X-ray observations of the active galactic nucleus (AGN) in NGC 7674. The source shows a flat X-ray spectrum, suggesting that it is obscured by Compton-thick gas…

astro-ph.GA2016★ 60 cited

A Distant Echo of Milky Way Central Activity closes the Galaxy's Baryon Census

F. Nicastro, F. Senatore, Y. Krongold +2

We report on the presence of large amounts of million-degree gas in the Milky Way's interstellar and circum-galactic medium. This gas (1) permeates both the Galactic plane and the…

astro-ph.GA2014★ 20 cited

Early-type galaxies in the Chandra COSMOS Survey

F. Civano, G. Fabbiano, S. Pellegrini +4

We study a sample of 69 X-ray detected Early Type Galaxies (ETGs), selected from the Chandra COSMOS survey, to explore the relation between the X-ray luminosity of hot gaseous halo…

astro-ph.HE2013★ 10 cited

The XMM-Newton spectrum of a candidate recoiling supermassive black hole: an elusive inverted P-Cygni profile

G. Lanzuisi, F. Civano, S. Marchesi +12

We present a detailed spectral analysis of new XMM-Newton data of the source CXOC J100043.1+020637, also known as CID-42, detected in the COSMOS survey at z = 0.359. Previous works…

astro-ph.CO2012★ 76 cited

Occupation of X-ray selected galaxy groups by X-ray AGN

V. Allevato, A. Finoguenov, G. Hasinger +12

We present the first direct measurement of the mean Halo Occupation Distribution (HOD) of X-ray selected AGN in the COSMOS field at z < 1, based on the association of 41 XMM and 17…

astro-ph.CO2012★ 59 cited

Chandra High resolution Observations of CID-42, a candidate recoiling SMBH

F. Civano, M. Elvis, G. Lanzuisi +15

We present Chandra High Resolution Camera observations of CID-42, a candidate recoiling supermassive black hole (SMBH) at z=0.359 in the COSMOS survey. CID-42 shows two optical com…