Search Results - "MULCHAEY, JOHN S"
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High-mass X-ray binaries in nearby metal-poor galaxies: on the contribution to nebular He ii emission
Published in Monthly notices of the Royal Astronomical Society (01-05-2020)“…ABSTRACT Despite significant progress both observationally and theoretically, the origin of high-ionization nebular He ii emission in galaxies dominated by…”
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The growth of brightest cluster galaxies and intracluster light over the past 10 billion years
Published in Monthly notices of the Royal Astronomical Society (01-01-2020)“…We constrain the evolution of the brightest cluster galaxy plus intracluster light (BCG + ICL) using an ensemble of 42 galaxy groups and clusters that span…”
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On the origin of excess cool gas in quasar host haloes
Published in Monthly notices of the Royal Astronomical Society (21-09-2015)“…Previous observations of quasar host haloes at z ≈ 2 have uncovered large quantities of cool gas that exceed what is found around inactive galaxies of both…”
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X-Ray Observations of a z ∼ 6.2 Quasar/Galaxy Merger
Published in The Astrophysical journal (20-12-2019)“…Quasars at early redshifts (z > 6) with companion galaxies offer unique insights into the growth and evolution of the first supermassive black holes. Here, we…”
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The Dawn of the Red: star formation histories of group galaxies over the past 5 billion years
Published in Monthly notices of the Royal Astronomical Society (01-05-2011)“…We examine the star formation properties of group and field galaxies in two surveys, Sloan Digital Sky Survey (at z∼ 0.08) and Group Environment Evolution…”
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THE SUPPRESSION OF STAR FORMATION AND THE EFFECT OF THE GALAXY ENVIRONMENT IN LOW-REDSHIFT GALAXY GROUPS
Published in The Astrophysical journal (01-10-2012)“…Understanding the interaction between galaxies and their surroundings is central to building a coherent picture of galaxy evolution. Here we use Galaxy…”
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A population of ultraviolet-dim protoclusters detected in absorption
Published in Nature (London) (16-06-2022)“…Galaxy protoclusters, which will eventually grow into the massive clusters we see in the local Universe, are usually traced by locating overdensities of…”
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The Cosmic Ultraviolet Baryon Survey (CUBS). VII. On the Warm-hot Circumgalactic Medium Probed by O vi and Ne viii at 0.4 ≲ z ≲ 0.7
Published in The Astrophysical journal (01-06-2024)“…This paper presents a newly established sample of 103 unique galaxies or galaxy groups at 0.4 ≲ z ≲ 0.7 from the Cosmic Ultraviolet Baryon Survey (CUBS) for…”
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The GEEC2 spectroscopic survey of Galaxy groups at 0.8 < z < 1
Published in Monthly notices of the Royal Astronomical Society (21-09-2014)“…We present the data release of the Gemini-South GMOS spectroscopy in the fields of 11 galaxy groups at 0.8 < z < 1, within the COSMOS field. This forms the…”
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Substructure in the most massive GEEC groups: field-like populations in dynamically active groups
Published in Monthly notices of the Royal Astronomical Society (01-04-2012)“…The presence of substructure in galaxy groups and clusters is believed to be a sign of recent galaxy accretion and can be used to probe not only the assembly…”
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Active Galactic Nuclei in Groups and Clusters of Galaxies: Detection and Host Morphology
Published in The Astrophysical journal (20-12-2009)“…The incidence and properties of active galactic nuclei (AGNs) in the field, groups, and clusters can provide new information about how these objects are…”
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Direct observational evidence for a large transient galaxy population in groups at 0.85 < z < 1
Published in Monthly notices of the Royal Astronomical Society (21-04-2011)“…We introduce our survey of galaxy groups at 0.85 < z < 1, as an extension of the Group Environment and Evolution Collaboration. Here we present the first…”
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The Distribution of Active Galactic Nuclei in Clusters of Galaxies
Published in The Astrophysical journal (01-08-2007)“…We present a study of the distribution of AGNs in clusters of galaxies with a uniformly selected, spectroscopically complete sample of 35 AGNs in eight…”
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X-RAY PROPERTIES OF GROUPS OF GALAXIES
Published in Annual review of astronomy and astrophysics (01-01-2000)“…ROSAT observations indicate that approximately half of all nearby groups of galaxies contain spatially extended X-ray emission. The radial extent of the X-ray…”
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The Properties of Poor Groups of Galaxies. I. Spectroscopic Survey and Results
Published in The Astrophysical journal (20-03-1998)Get full text
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Spectroscopic Confirmation of a Large Population of Active Galactic Nuclei in Clusters of Galaxies
Published in The Astrophysical journal (10-06-2006)“…We have completed a spectroscopic survey of X-ray point sources in eight low-redshift clusters of galaxies (0.05 < z < 0.31) and have identified 40 cluster…”
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On the possible environmental effect in distributing heavy elements beyond individual gaseous haloes
Published in Monthly notices of the Royal Astronomical Society (21-05-2015)“…We present a study of extended galaxy halo gas through H i and O vi absorption over two decades in projected distance at z ... 0.2. The study is based on a…”
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First Measurement of a Rapid Increase in the AGN Fraction in High-Redshift Clusters of Galaxies
Published in The Astrophysical journal (20-07-2007)“…We present the first measurement of the AGN fraction in high-redshift clusters of galaxies (z similar to 0.6) with spectroscopy of one cluster and archival…”
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Do group dynamics play a role in the evolution of member galaxies?
Published in Monthly notices of the Royal Astronomical Society (21-10-2013)“…We examine galaxy groups from the present epoch to z ∼ 1 to explore the impact of group dynamics on galaxy evolution. We use group catalogues from the Sloan…”
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Lost but not forgotten: intracluster light in galaxy groups and clusters
Published in Monthly notices of the Royal Astronomical Society (01-03-2018)“…AbstractWith Hubble Space Telescope imaging, we investigate the progenitor population and formation mechanisms of the intracluster light (ICL) for 23 galaxy…”
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