Search Results - "VAN DER WEL, Arjen"
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Major Mergers Are Not the Dominant Trigger for High-accretion AGNs at z ∼ 2
Published in The Astrophysical journal (10-09-2019)“…Research over the past decade has shown diminishing evidence for major galaxy mergers being a dominant mechanism for the growth of supermassive black holes…”
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Fast and Slow Paths to Quiescence: Ages and Sizes of 400 Quiescent Galaxies from the LEGA-C Survey
Published in The Astrophysical journal (20-11-2018)“…We analyze the stellar age indicators (Dn4000 and EW(Hδ)) and sizes of 467 quiescent galaxies with M* ≥ 1010 M at z ∼ 0.7 drawn from DR2 of the LEGA-C survey…”
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The Mass Scale of High-redshift Galaxies: Virial Mass Estimates Calibrated with Stellar Dynamical Models from LEGA-C
Published in The Astrophysical journal (01-09-2022)“…Abstract Dynamical models for 673 galaxies at z = 0.6–1.0 with spatially resolved (long-slit) stellar kinematic data from LEGA-C are used to calibrate virial…”
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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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Extending the evolution of the stellar mass–size relation at z ≤ 2 to low stellar mass galaxies from HFF and CANDELS
Published in Monthly notices of the Royal Astronomical Society (10-09-2021)“…ABSTRACT We reliably extend the stellar mass–size relation over 0.2 ≤ z ≤ 2 to low stellar mass galaxies by combining the depth of Hubble Frontier Fields with…”
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The Colors and Sizes of Recently Quenched Galaxies: A Result of Compact Starburst before Quenching
Published in The Astrophysical journal (10-01-2020)“…We analyze the colors and sizes of 32 quiescent (UVJ-selected) galaxies with strong Balmer absorption (EW(Hδ) ≥ 4 ) at z ∼ 0.8 drawn from DR2 of the LEGA-C…”
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Rest-frame Near-infrared Sizes of Galaxies at Cosmic Noon: Objects in JWST's Mirror Are Smaller than They Appeared
Published in Astrophysical journal. Letters (01-10-2022)“…Abstract Galaxy sizes and their evolution over cosmic time have been studied for decades and serve as key tests of galaxy formation models. However, at z ≳ 1…”
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Molecular Gas Contents and Scaling Relations for Massive, Passive Galaxies at Intermediate Redshifts from the LEGA-C Survey
Published in The Astrophysical journal (20-06-2018)“…A decade of study has established that the molecular gas properties of star-forming galaxies follow coherent scaling relations out to z ∼ 3, suggesting…”
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A Significant Excess in Major Merger Rate for AGNs with the Highest Eddington Ratios at z < 0.2
Published in The Astrophysical journal (01-11-2020)“…Abstract Observational studies are increasingly finding evidence against major mergers being the dominant mechanism responsible for triggering an active…”
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THE ALMA SPECTROSCOPIC SURVEY IN THE HUBBLE ULTRA DEEP FIELD: MOLECULAR GAS RESERVOIRS IN HIGH-REDSHIFT GALAXIES
Published in The Astrophysical journal (10-12-2016)“…ABSTRACT We study the molecular gas properties of high-z galaxies observed in the ALMA Spectroscopic Survey (ASPECS) that targets an ∼1 arcmin2 region in the…”
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The redshift and mass dependence on the formation of the Hubble sequence at z > 1 from CANDELS/UDS
Published in Monthly notices of the Royal Astronomical Society (01-08-2013)“…In this paper we present a detailed study of the structures and morphologies of a sample of 1188 massive galaxies with M * ≥ 1010 M between redshifts z = 1 and…”
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The hyperplane of early-type galaxies: using stellar population properties to increase the precision and accuracy of the fundamental plane as a distance indicator
Published in Monthly notices of the Royal Astronomical Society (01-08-2024)“…ABSTRACT We use deep spectroscopy from the SAMI (Sydney-AAO Multi-object Integral) Galaxy Survey to explore the precision of the fundamental plane (FP) of…”
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Age and metal gradients in massive quiescent galaxies at 0.6 ≲ z ≲ 1.0: implications for quenching and assembly histories
Published in Monthly notices of the Royal Astronomical Society (01-08-2024)“…ABSTRACT We present spatially resolved, simple stellar population equivalent ages, stellar metallicities, and abundance ratios for 456 massive ($10.3\lesssim…”
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On the importance of using appropriate spectral models to derive physical properties of galaxies at 0.7 < z < 2.8
Published in Monthly notices of the Royal Astronomical Society (11-02-2015)“…Interpreting observations of distant galaxies in terms of constraints on physical parameters – such as stellar mass (M ★), star formation rate (SFR) and dust…”
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Galaxy kinematics and mass estimates at z ∼ 1 from ionized gas and stars
Published in Monthly notices of the Royal Astronomical Society (01-01-2024)“…ABSTRACT We compare ionized gas and stellar kinematics of 16 star-forming galaxies (log (M⋆/M⊙) = 9.7–11.2, SFR =6 − 86 M⊙ yr−1) at z ∼ 1 using near-infrared…”
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An over-massive black hole in the compact lenticular galaxy NGC 1277
Published in Nature (London) (29-11-2012)Get full text
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First results from the TNG50 simulation: the evolution of stellar and gaseous discs across cosmic time
Published in Monthly notices of the Royal Astronomical Society (01-12-2019)“…Abstract We present a new cosmological, magnetohydrodynamical simulation for galaxy formation: TNG50, the third and final instalment of the IllustrisTNG…”
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Observed structural parameters of EAGLE galaxies: reconciling the mass–size relation in simulations with local observations
Published in Monthly notices of the Royal Astronomical Society (15-02-2022)“…ABSTRACT We use mock images of z = 0.1 galaxies in the 100 Mpc EAGLE simulation to establish the differences between the sizes and morphologies inferred from…”
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Deprojecting Sérsic Profiles for Arbitrary Triaxial Shapes: Robust Measures of Intrinsic and Projected Galaxy Sizes
Published in The Astrophysical journal (01-06-2021)“…Abstract We present the analytical framework for converting projected light distributions with a Sérsic profile into three-dimensional light distributions for…”
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COSMOS-DASH: The Evolution of the Galaxy Size-Mass Relation since z ∼ 3 from New Wide-field WFC3 Imaging Combined with CANDELS/3D-HST
Published in The Astrophysical journal (20-07-2019)“…We present COSMOS-Drift And SHift (DASH), a Hubble Space Telescope (HST) Wide Field Camera 3 (WFC3) imaging survey of the COSMOS field in the H160 filter. The…”
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