activity
20192026
most citedH-X-ray Surface Brightness Correlation for Filaments in Cooling Flow Clusters

15 citations · 23 across the 16 of their papers we have counts for

collaborators

17 papers

astro-ph.HE2026

Multi-epoch Detection of an Ultra-fast Inflow in ESP 39607: Evidence for an Accretion Cascade

Alessandro Peca, Michael J. Koss, Roberto Serafinelli +10

We present simultaneous XRISM, XMM-Newton, and NuSTAR observations of ESP 39607, a Seyfert 2 galaxy at . XRISM/Resolve reveals two absorption features near 4.7 and 4.9 k…

astro-ph.HE2026

Dissecting the Nuclear Structure of NGC 5548 with XRISM. I. Physical Properties of the Highly Ionized Outflows

Missagh Mehdipour, Jon M. Miller, Jelle S. Kaastra +21

We present a detailed spectral analysis of an X-Ray Imaging and Spectroscopy Mission (XRISM) observation of the prototypical Seyfert 1 galaxy NGC 5548. XRISM's Resolve microcalorim…

astro-ph.GA2026

AGN Feeding & Feedback Over the Galactic Scales

Filippo M. Maccagni, Vincenzo Mainieri, Isabella Prandoni +8

Active Galactic Nuclei (AGN) are key drivers of galaxy evolution, triggered by cold gas accreting onto a super-massive black hole. However, the processes regulating this gas accret…

astro-ph.GA2025

A Deep Chandra View of Abell 2597: Bubbles, Shocks, Cold Fueling, and a Plasma Depletion Layer

Osase Omoruyi, Grant Tremblay, Stefi A. Baum +14

To examine how AGN feedback shapes the intracluster medium (ICM) and fuels black hole accretion in the cool-core galaxy cluster Abell 2597, we present deep (600 ks) Chandra X…

astro-ph.GA2025

The relationship between warm and hot gas-phase metallicity in massive elliptical galaxies and the influence of AGN feedback

Valeria Olivares, Yuanyuan Su, Pasquale Temi +10

Warm ionized gas is ubiquitous at the centers of X-ray bright elliptical galaxies. While it is believed to play a key role in the feeding and feedback processes of supermassive bla…

astro-ph.HE2025★ 3 cited

The Advanced X-ray Imaging Satellite (AXIS) Community Science Book

Michael Koss, Nafisa Aftab, Steven W. Allen +395

The AXIS Community Science Book represents the collective effort of 592 scientists worldwide to define the transformative science enabled by the Advanced X-ray Imaging Satellite (A…

astro-ph.GA2025

A century of change: new changing-look event in Mrk 1018's past

Thomas Dunn, Rebecca McElroy, Mirko Krumpe +7

We investigate the long-term variability of the known Changing Look Active Galactic Nuclei (CL AGN) Mrk 1018, whose second change we discovered as part of the Close AGN Reference S…

astro-ph.GA2025

The Close AGN Reference Survey (CARS): A comparison between sub-mm and optical AGN diagnostic diagrams

Jacob S. Elford, Timothy A. Davis, Ilaria Ruffa +9

The relation suggests that there is a tight connection between dense gas and star formation. We use data from the Close AGN Reference Survey (CARS) to inve…

astro-ph.GA2025

Constraining star formation in M87 using deep HST UV data

Prathamesh Tamhane, William Waldron, Ming Sun +11

We analyzed the deepest Hubble Space Telescope (HST) F275W ultraviolet (UV) imaging of M87 to obtain the most robust constraints on its star formation rate (SFR) and star formation…

astro-ph.CO2025

The Onset of Feedback in Abell 1885: Evidence for Large-Scale Quenching Despite a Young Central AGN

Laurel White, Michael McDonald, Francesco Ubertosi +4

We present a new 8.5 ks Chandra observation of Abell 1885, obtained as part of the Cluster Evolution Reference Ensemble At Low-z (CEREAL) survey of ~200 low-z galaxy groups and clu…

astro-ph.GA2025★ 5 cited

Directly Imaging the Cooling Flow in the Phoenix Cluster

Michael Reefe, Michael McDonald, Marios Chatzikos +14

In the centers of many galaxy clusters, the hot (10 K) intracluster medium (ICM) can become dense enough that it should cool on short timescales. However, the low measure…

astro-ph.GA2025★ 15 cited

H-X-ray Surface Brightness Correlation for Filaments in Cooling Flow Clusters

Valeria Olivares, Adrien Picquenot, Yuanyuan Su +4

Massive galaxies in cooling flow clusters display clear evidence of feedback from Active Galactic Nuclei (AGN). Joint X-ray and radio observations have shown that AGN radio jets pu…

astro-ph.GA2025

Cold Gas and Star Formation in the Phoenix Cluster with JWST

Michael Reefe, Michael McDonald, Marios Chatzikos +16

We present integral field unit observations of the Phoenix Cluster with the JWST Mid-infrared Instrument's Medium Resolution Spectrometer (MIRI/MRS). We focus this study on the mol…

astro-ph.CO2024

SZ-X-ray Surface Brightness Fluctuations in the SPT-XMM clusters

Charles Romero, Massimo Gaspari, Gerrit Schellenberger +10

The hot plasma in galaxy clusters, the intracluster medium (ICM), is expected to be shaped by subsonic turbulent motions, which are key for heating, cooling, and transport mechanis…

astro-ph.GA2024

X-ray Cool Core Remnants Heated by Strong Radio AGN Feedback

Wenhao Liu, Ming Sun, G. Mark Voit +6

Strong AGN heating provides an alternative means for the disruption of cluster cool cores (CCs) to cluster mergers. In this work we present a systematic Chandra study of a sample o…

astro-ph.CO2024

Surface Brightness Fluctuations in Two SPT clusters: a Pilot Study

Charles E. Romero, Massimo Gaspari, Gerrit Schellenberger +10

Studies of surface brightness fluctuations in the intracluster medium (ICM) present an indirect probe of turbulent properties such as the turbulent velocities, injection scales, an…

astro-ph.CO2019

Unveiling the Galaxy Cluster - Cosmic Web Connection with X-ray observations in the Next Decade

Stephen A. Walker, Daisuke Nagai, A. Simionescu +35

In recent years, the outskirts of galaxy clusters have emerged as one of the new frontiers and unique laboratories for studying the growth of large scale structure in the universe.…