Search Results - "Croton, D."
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Statistical analysis of galaxy surveys – I. Robust error estimation for two-point clustering statistics
Published in Monthly notices of the Royal Astronomical Society (11-06-2009)“…We present a test of different error estimators for two-point clustering statistics, appropriate for present and future large galaxy redshift surveys. Using an…”
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The growth of discs and bulges during hierarchical galaxy formation – I. Fast evolution versus secular processes
Published in Monthly notices of the Royal Astronomical Society (11-07-2016)“…We present a theoretical model for the evolution of mass, angular momentum and size of galaxy discs and bulges, and we implement it into the semi-analytic…”
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Simulation of the Cosmic Evolution of Atomic and Molecular Hydrogen in Galaxies
Published in The Astrophysical journal (20-06-2009)“…We present a simulation of the cosmic evolution of the atomic and molecular phases of the cold hydrogen gas in about 3 X 107 galaxies, obtained by…”
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Evidence for Merger-driven Growth in Luminous, High-z, Obscured AGNs in the CANDELS/COSMOS Field
Published in The Astrophysical journal (20-01-2018)“…While major mergers have long been proposed as a driver of both active galactic nucleus (AGN) activity and the relation, studies of moderate to high-redshift…”
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The formation history of elliptical galaxies
Published in Monthly notices of the Royal Astronomical Society (01-02-2006)“…ABSTRACT We take advantage of the largest high‐resolution simulation of cosmic structure growth ever carried out – the Millennium Simulation of the concordance…”
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The morphologies of massive galaxies at 1 < z < 3 in the CANDELS-UDS field: compact bulges, and the rise and fall of massive discs
Published in Monthly notices of the Royal Astronomical Society (01-12-2012)“…We have used high-resolution, Hubble Space Telescope, near-infrared imaging to conduct a detailed analysis of the morphological properties of the most massive…”
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[O ii] emitters in MultiDark-Galaxies and DEEP2
Published in Monthly notices of the Royal Astronomical Society (01-10-2020)“…ABSTRACT We use three semi-analytical models (SAMs) of galaxy formation and evolution run on the same 1 h−1 Gpc MultiDark Planck2 cosmological simulation to…”
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Galaxy Cluster Mass Reconstruction Project – IV. Understanding the effects of imperfect membership on cluster mass estimation
Published in Monthly notices of the Royal Astronomical Society (21-11-2018)“…The primary difficulty in measuring dynamical masses of galaxy clusters from galaxy data lies in the separation between true cluster members from interloping…”
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Interactive 3D visualization for theoretical virtual observatories
Published in Monthly notices of the Royal Astronomical Society (21-06-2018)“…Abstract Virtual observatories (VOs) are online hubs of scientific knowledge. They encompass a collection of platforms dedicated to the storage and…”
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Galaxy cluster mass reconstruction project – I. Methods and first results on galaxy-based techniques
Published in Monthly notices of the Royal Astronomical Society (21-06-2014)“…This paper is the first in a series in which we perform an extensive comparison of various galaxy-based cluster mass estimation techniques that utilize the…”
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Morphologies of z ∼ 0.7 AGN host galaxies in CANDELS: no trend of merger incidence with AGN luminosity
Published in Monthly notices of the Royal Astronomical Society (21-04-2014)“…The processes that trigger active galactic nuclei (AGN) remain poorly understood. While lower luminosity AGN may be triggered by minor disturbances to the host…”
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Galaxy Cluster Mass Reconstruction Project – II. Quantifying scatter and bias using contrasting mock catalogues
Published in Monthly notices of the Royal Astronomical Society (11-05-2015)“…This paper is the second in a series in which we perform an extensive comparison of various galaxy-based cluster mass estimation techniques that utilize the…”
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AEGIS: The Color-Magnitude Relation for X-Ray-selected Active Galactic Nuclei
Published in The Astrophysical journal (01-05-2007)“…We discuss the relationship between rest-frame color and optical luminosity for X-ray sources in the range 0.6< z <1.4 selected from the Chandra survey of the…”
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Galaxy Cluster Mass Reconstruction Project – III. The impact of dynamical substructure on cluster mass estimates
Published in Monthly notices of the Royal Astronomical Society (21-03-2018)“…Abstract With the advent of wide-field cosmological surveys, we are approaching samples of hundreds of thousands of galaxy clusters. While such large numbers…”
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Statistical analysis of galaxy surveys — II. The three-point galaxy correlation function measured from the 2dFGRS
Published in Monthly notices of the Royal Astronomical Society (01-12-2005)“…We present new results for the three-point correlation function, ζ, measured as a function of scale, luminosity and colour from the final version of the 2dF…”
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The role of dissipation in the scaling relations of cosmological merger remnants
Published in Monthly notices of the Royal Astronomical Society (01-08-2011)“…There are strong correlations between the three structural properties of elliptical galaxies - stellar mass, velocity dispersion and size - in the form of a…”
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The All-Wavelength Extended Groth Strip International Survey (AEGIS) Data Sets
Published in The Astrophysical journal (01-05-2007)“…In this the first of a series of Letters, we present a panchromatic data set in the Extended Groth Strip region of the sky. Our survey, the All-Wavelength…”
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The growth of discs and bulges during hierarchical galaxy formation – II. Metallicity, stellar populations and dynamical evolution
Published in Monthly notices of the Royal Astronomical Society (11-03-2017)“…We investigate the properties of the stellar populations of model galaxies as a function of galaxy evolutionary history and angular momentum content. We use…”
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Statistical analysis of galaxy surveys - IV. An objective way to quantify the impact of superstructures on galaxy clustering statistics
Published in Monthly notices of the Royal Astronomical Society (01-12-2011)“…For galaxy clustering to provide robust constraints on cosmological parameters and galaxy formation models, it is essential to make reliable estimates of the…”
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Galaxy And Mass Assembly (GAMA): the bright void galaxy population in the optical and mid-IR
Published in Monthly notices of the Royal Astronomical Society (11-11-2015)“…We examine the properties of galaxies in the Galaxies and Mass Assembly (GAMA) survey located in voids with radii >10 h −1 Mpc. Utilizing the GAMA equatorial…”
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