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Modelling the galaxy bimodality: shutdown above a critical halo mass
We reproduce the blue and red sequences in the observed joint distribution of colour and magnitude for galaxies at low and high redshifts using hybrid N-body/semi-analytic simulations of galaxyExpand
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Comparing climate and cost impacts of reference levels for reducing emissions from deforestation
The climate benefit and economic cost of an international mechanism for reducing emissions from deforestation and degradation (REDD) will depend on the design of reference levels for creditingExpand
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Climate Smart Agriculture? Assessing the Adaptation Implications in Zambia
We examine a set of potentially climate smart agricultural practices, including reduced tillage, crop rotation and legume intercropping, combined with the use of improved seeds and inorganicExpand
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AGN self-regulation in cooling flow clusters
We use three-dimensional high-resolution adaptive-mesh-refinement simulations to investigate if mechanical feedback from active galactic nucleus jets can halt a massive cooling flow in a galaxyExpand
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The role of black holes in galaxy formation and evolution
Virtually all massive galaxies, including our own, host central black holes ranging in mass from millions to billions of solar masses. The growth of these black holes releases vast amounts of energyExpand
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Accuracy Evaluation of Three Modelling Tools for Occupational Exposure Assessment
Objectives The objective of this study is to evaluate the accuracy and robustness of three exposure-modelling tools [STOFFENMANAGER® v.6, European Centre for Ecotoxicology and Toxicology of ChemicalExpand
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Review of Agri-Environment Indexes and Stewardship Payments
Agri-environment programs aim to secure environmental and social stewardship services through payments to farmers. A critical component of many agri-environment programs is an agri-environment indexExpand
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THE MORPHOLOGIES OF MASSIVE GALAXIES FROM z ∼ 3—WITNESSING THE TWO CHANNELS OF BULGE GROWTH
We quantify the morphological evolution of z ~ 0 massive galaxies (M_*/M_∼ ∼10^11.2 +/- 0.3) from z ~ 3 in the 5 CANDELS fields. The progenitors are selected using abundance matching techniques toExpand
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Downsizing by shutdown in red galaxies
We address the origin of the 'downsizing' of elliptical galaxies, according to which the stars in more massive galaxies formed earlier and over a shorter period than those in less massive galaxies.Expand
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Galaxy luminosity function and Tully-Fisher relation: reconciled through rotation-curve studies
The relation between galaxy luminosity L and halo virial velocity v vir required to fit the galaxy luminosity function differs from the observed Tully-Fisher relation between L and disk speed v rot.Expand
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