Search Results - "Faber, M"
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Compaction and quenching of high-z galaxies in cosmological simulations: blue and red nuggets
Published in Monthly notices of the Royal Astronomical Society (01-07-2015)“…We use cosmological simulations to study a characteristic evolution pattern of high-redshift galaxies. Early, stream-fed, highly perturbed, gas-rich discs…”
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Structural and Star-forming Relations since z ∼ 3: Connecting Compact Star-forming and Quiescent Galaxies
Published in The Astrophysical journal (01-05-2017)“…We study the evolution of the scaling relations that compare the effective density ( ) and core density ( kpc) to the stellar masses of star-forming galaxies…”
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Effectiveness of behavioral techniques and physical exercise on psychosocial functioning and health-related quality of life in breast cancer patients and survivors-a meta-analysis
Published in Psycho-Oncology (01-02-2011)“…Objective: To evaluate the effect of behavioral techniques and physical exercise on psychosocial functioning and health‐related quality of life (HRQoL)…”
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Shellfish allergens: tropomyosin and beyond
Published in Allergy (Copenhagen) (01-06-2017)“…IgE‐mediated shellfish allergy constitutes an important cause of food‐related adverse reactions. Shellfish are classified into mollusks and crustaceans, the…”
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Steep rise in norovirus cases and emergence of a new recombinant strain GII.P16-GII.2, Germany, winter 2016
Published in Euro surveillance : bulletin européen sur les maladies transmissibles (26-01-2017)“…Since early November 2016, the number of laboratory-confirmed norovirus infections reported in Germany has been increasing steeply. Here, we report the…”
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What is Important? Morphological Asymmetries are Useful Predictors of Star Formation Rates of Star-forming Galaxies in SDSS Stripe 82
Published in The Astrophysical journal (01-12-2021)“…Abstract The morphology and structure of galaxies reflect their star formation and assembly histories. We use the framework of mutual information (MI) to…”
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Clumpy Galaxies in CANDELS. II. Physical Properties of UV-bright Clumps at 0.5 ≤ z < 3
Published in The Astrophysical journal (01-02-2018)“…Studying giant star-forming clumps in distant galaxies is important to understand galaxy formation and evolution. At present, however, observers and theorists…”
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Physical Drivers of Emission-line Diversity of SDSS Seyfert 2s and LINERs after Removal of Contributions from Star Formation
Published in The Astrophysical journal (01-12-2021)“…Abstract Ionization sources other than H ii regions give rise to the right-hand branch in the standard ([N ii ]) BPT diagram, populated by Seyfert 2s and…”
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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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z ∼ 2: An Epoch of Disk Assembly
Published in The Astrophysical journal (01-07-2017)“…We explore the evolution of the internal gas kinematics of star-forming galaxies from the peak of cosmic star formation at z ∼ 2 to today. Measurements of…”
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The Black Hole Mass in M87 from Gemini/NIFS Adaptive Optics Observations
Published in The Astrophysical journal (10-03-2011)“…We present the stellar kinematics in the central 2'' of the luminous elliptical galaxy M87 (NGC 4486), using laser adaptive optics to feed the Gemini telescope…”
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Extragalactic background light inferred from AEGIS galaxy-SED-type fractions
Published in Monthly notices of the Royal Astronomical Society (01-02-2011)“…The extragalactic background light (EBL) is of fundamental importance both for understanding the entire process of galaxy evolution and for γ-ray astronomy,…”
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The evolution of galaxy shapes in CANDELS: from prolate to discy
Published in Monthly notices of the Royal Astronomical Society (21-04-2019)“…Abstract We model the projected b/a–log a distributions of CANDELS star-forming main-sequence galaxies, where a (b) is the half-light semimajor (semiminor)…”
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Dissecting the Red sequence. III. Mass-to-Light Variations in Three-dimensional Fundamental Plane Space
Published in The Astrophysical journal (10-07-2010)“…The fundamental plane (FP) of early-type galaxies is observed to have finite thickness and to be tilted from the virial relation. Both of these represent…”
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Genetic studies of quantitative MCI and AD phenotypes in ADNI: Progress, opportunities, and plans
Published in Alzheimer's & dementia (01-07-2015)“…Abstract Introduction Genetic data from the Alzheimer's Disease Neuroimaging Initiative (ADNI) have been crucial in advancing the understanding of Alzheimer's…”
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Demographics of Star-forming Galaxies since z ∼ 2.5. I. The UVJ Diagram in CANDELS
Published in The Astrophysical journal (10-05-2018)“…This is the first in a series of papers examining the demographics of star-forming (SF) galaxies at 0.2 < z < 2.5 in CANDELS. We study 9100 galaxies from…”
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FROM STARBURST TO QUIESCENCE: TESTING ACTIVE GALACTIC NUCLEUS FEEDBACK IN RAPIDLY QUENCHING POST-STARBURST GALAXIES
Published in The Astrophysical journal (10-09-2014)“…Post-star-bursts are galaxies in transition from the blue cloud to the red sequence. This work uses Sloan Digital Sky Survey, the Galaxy Evolution Explorer,…”
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The DEEP3 Galaxy Redshift Survey: the impact of environment on the size evolution of massive early-type galaxies at intermediate redshift
Published in Monthly notices of the Royal Astronomical Society (01-02-2012)“…Using data drawn from the DEEP2 and DEEP3 Galaxy Redshift Surveys, we investigate the relationship between the environment and the structure of galaxies…”
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The M-σ and M-L Relations in Galactic Bulges, and Determinations of Their Intrinsic Scatter
Published in The Astrophysical journal (10-06-2009)“…We derive improved versions of the relations between supermassive black hole mass (M BH) and host-galaxy bulge velocity dispersion ( sigma ) and luminosity (L;…”
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Dissecting the Red Sequence. II. Star Formation Histories of Early-Type Galaxies Throughout the Fundamental Plane
Published in The Astrophysical journal (20-06-2009)“…This analysis uses spectra of ~16,000 nearby Sloan Digital Sky Survey quiescent galaxies to track variations in galaxy star formation histories (SFHs) along…”
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