Search Results - "Hlavacek, J."
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Shaken Snow Globes: Kinematic Tracers of the Multiphase Condensation Cascade in Massive Galaxies, Groups, and Clusters
Published in The Astrophysical journal (20-02-2018)“…We propose a novel method to constrain turbulence and bulk motions in massive galaxies, galaxy groups, and clusters, exploring both simulations and…”
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The Remarkable Similarity of Massive Galaxy Clusters from z ∼ 0 to z ∼ 1.9
Published in The Astrophysical journal (01-07-2017)“…We present the results of a Chandra X-ray survey of the eight most massive galaxy clusters at z > 1.2 in the South Pole Telescope 2500 deg2 survey. We combine…”
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Revealing the velocity structure of the filamentary nebula in NGC 1275 in its entirety
Published in Monthly notices of the Royal Astronomical Society. Letters (01-09-2018)“…ABSTRACT We have produced for the first time a detailed velocity map of the giant filamentary nebula surrounding NGC 1275, the Perseus cluster’s brightest…”
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Alma Observations of Massive Molecular Gas Filaments Encasing Radio Bubbles in the Phoenix Cluster
Published in The Astrophysical journal (10-02-2017)“…We report new ALMA observations of the CO(3-2) line emission from the molecular gas reservoir in the central galaxy of the Phoenix cluster. The cold molecular…”
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A comprehensive study of the radio properties of brightest cluster galaxies
Published in Monthly notices of the Royal Astronomical Society (21-10-2015)“…We examine the radio properties of the brightest cluster galaxies (BCGs) in a large sample of X-ray selected galaxy clusters comprising the Brightest Cluster…”
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The Evolution of Environmental Quenching Timescales to z ∼ 1.6: Evidence for Dynamically Driven Quenching of the Cluster Galaxy Population
Published in The Astrophysical journal (20-10-2018)“…Using a sample of four galaxy clusters at 1.35 < z < 1.65 and 10 galaxy clusters at 0.85 < z < 1.35, we measure the environmental quenching timescale, tQ,…”
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A volume-limited sample of X-ray galaxy groups and clusters – II. X-ray cavity dynamics
Published in Monthly notices of the Royal Astronomical Society (21-10-2014)“…We present the results of our study of a volume-limited sample (z ≤ 0.071) of 101 X-ray galaxy groups and clusters, in which we explore the X-ray cavity…”
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Anatomy of a Cooling Flow: The Feedback Response to Pure Cooling in the Core of the Phoenix Cluster
Published in The Astrophysical journal (01-11-2019)“…We present new, deep observations of the Phoenix cluster from Chandra, the Hubble Space Telescope, and the Karl Jansky Very Large Array. These data provide an…”
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Baryon content in a sample of 91 galaxy clusters selected by the South Pole Telescope at 0.2 <z < 1.25
Published in Monthly notices of the Royal Astronomical Society (01-08-2018)“…We estimate total mass (M_500), intracluster medium (ICM) mass (M_ICM), and stellar mass (M_⋆) in a Sunyaev–Zel’dovich effect (SZE) selected sample of 91…”
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On the relation between mini-halos and AGN feedback in clusters of galaxies
Published in Monthly notices of the Royal Astronomical Society (01-12-2020)“…ABSTRACT A variety of large-scale diffuse radio structures have been identified in many clusters with the advent of new state-of-the-art facilities in radio…”
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Optical emission line nebulae in galaxy cluster cores 1: the morphological, kinematic and spectral properties of the sample
Published in Monthly notices of the Royal Astronomical Society (01-08-2016)“…We present an Integral Field Unit survey of 73 galaxy clusters and groups with the VIsible Multi Object Spectrograph on the Very Large Telescope. We exploit…”
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Extreme AGN feedback in the MAssive Cluster Survey: a detailed study of X-ray cavities at z>0.3
Published in Monthly notices of the Royal Astronomical Society (01-04-2012)“…We present the first statistical study of X-ray cavities in distant clusters of galaxies (z > 0.3). With the aim of providing further insight into how active…”
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Testing for X-Ray-SZ Differences and Redshift Evolution in the X-Ray Morphology of Galaxy Clusters
Published in The Astrophysical journal (20-05-2017)“…We present a quantitative study of the X-ray morphology of galaxy clusters, as a function of their detection method and redshift. We analyze two separate…”
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A wide Chandra view of the core of the Perseus cluster
Published in Monthly notices of the Royal Astronomical Society (21-12-2011)“…We present new Chandra images of the X-ray emission from the core of the Perseus cluster of galaxies. The total observation time is now 1.4 Ms. New depressions…”
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SIGNALS: I. Survey description
Published in Monthly notices of the Royal Astronomical Society (11-11-2019)“…ABSTRACT SIGNALS, the Star formation, Ionized Gas, and Nebular Abundances Legacy Survey, is a large observing programme designed to investigate massive star…”
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The First High-contrast Images of Near High-mass X-Ray Binaries with Keck/NIRC2
Published in The Astrophysical journal (01-05-2024)“…Abstract Although the study of X-ray binaries has led to major breakthroughs in high-energy astrophysics, their circumbinary environment at scales of…”
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Deep learning workflow to support in-flight processing of digital aerial imagery for wildlife population surveys
Published in PloS one (03-04-2024)“…Deep learning shows promise for automating detection and classification of wildlife from digital aerial imagery to support cost-efficient remote sensing…”
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Galaxy populations in the 26 most massive galaxy clusters in the South Pole Telescope SPT-SZ survey
Published in Monthly notices of the Royal Astronomical Society (11-10-2016)“…We present a study of the optical properties of the 26 most massive galaxy clusters within the South Pole Telescope Sunyaev-Zel'dovich (SPT-SZ) 2500 deg2…”
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Redshift Evolution of the Feedback–Cooling Equilibrium in the Core of 48 SPT Galaxy Clusters: A Joint Chandra–SPT–ATCA Analysis
Published in The Astrophysical journal (01-05-2023)“…Abstract We analyze the cooling and feedback properties of 48 galaxy clusters at redshifts 0.4 < z < 1.3 selected from the South Pole Telescope (SPT) catalogs…”
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The rapid evolution of AGN feedback in brightest cluster galaxies: switching from quasar-mode to radio-mode feedback
Published in Monthly notices of the Royal Astronomical Society (11-05-2013)“…We present an analysis of the 2-10 keV X-ray emission associated with the active galactic nuclei (AGN) in brightest cluster galaxies (BCGs). Our sample…”
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