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The epoch of galaxy formationGalaxies at redshifts 5 to 6 with systematically low dust content and high [C II] emission.Galaxy evolution. Evidence for mature bulges and an inside-out quenching phase 3 billion years after the Big Bang.zCOSMOS: A Large VLT/VIMOS Redshift Survey Covering 0 <z< 3 in the COSMOS FieldThe Cosmic Evolution Survey (COSMOS): OverviewCOSMOS: Hubble Space Telescope ObservationsProto-groups at 1.8 < z < 3 in the zCOSMOS-deep sampleSpace-quality data from balloon-borne telescopes: The High Altitude Lensing Observatory (HALO)PHIBSS: Unified Scaling Relations of Gas Depletion Time and Molecular Gas FractionsCombined CO and dust scaling relations of depletion time and molecular gas fractions with cosmic time, specific star-formation rate, and stellar massCommission 28: GalaxiesDivision VIII: Galaxies and the UniverseThe second-generation VLT instrument MUSE: science drivers and instrument designA massive, distant proto-cluster at z = 2.47 caught in a phase of rapid formation?Connection between Stellar Mass Distributions within Galaxies and Quenching Sincez= 2Extreme emission-line galaxies out toz~ 1 in zCOSMOSThe dependence of galactic outflows on the properties and orientation of zCOSMOS galaxies at z ~ 1THE SINS/zC-SINF SURVEY OFz∼ 2 GALAXY KINEMATICS: EVIDENCE FOR POWERFUL ACTIVE GALACTIC NUCLEUS-DRIVEN NUCLEAR OUTFLOWS IN MASSIVE STAR-FORMING GALAXIESTHE SINS/zC-SINF SURVEY OFz∼ 2 GALAXY KINEMATICS: EVIDENCE FOR GRAVITATIONAL QUENCHINGThe zCOSMOS redshift survey: evolution of the light in bulges and discs since z ~ 0.8zCOSMOS 20k: satellite galaxies are the main drivers of environmental effects in the galaxy population at least to z ∼ 0.7Spot the differenceInvestigating the relationship between AGN activity and stellar mass in zCOSMOS galaxies at 0 < z < 1 using emission-line diagnostic diagramsMass assembly in quiescent and star-forming galaxies since z ≃ 4 from UltraVISTAObscured AGN at z ~ 1 from the zCOSMOS-Bright SurveyThe colors of central and satellite galaxies in zCOSMOS out to z =~ 0.8 and implications for quenchingEnvironmental effects in the interaction and merging of galaxies in zCOSMOSThe cosmic evolution of oxygen and nitrogen abundances in star-forming galaxies over the past 10 GyrThe dominant role of mergers in the size evolution of massive early-type galaxies sincez ~ 1Comparison of star formation rates from Hα and infrared luminosity as seen byHerschelA group-galaxy cross-correlation function analysis in zCOSMOSThe COSMOS density field: a reconstruction using both weak lensing and galaxy distributionsTHE zCOSMOS 20k GROUP CATALOGPhoto-zperformance for precision cosmology - II. Empirical verification1★A journey from the outskirts to the cores of groupsThe impact of galaxy interactions on active galactic nucleus activity in zCOSMOSThe radial and azimuthal profiles of Mg II absorption around 0.5 < z < 0.9 zCOSMOS galaxies of different colors, masses, and environmentsTHE zCOSMOS-SINFONI PROJECT. I. SAMPLE SELECTION AND NATURAL-SEEING OBSERVATIONSBlack hole accretion and host galaxies of obscured quasars in XMM-COSMOSThe bimodality of the 10k zCOSMOS-bright galaxies up toz ~ 1: a new statistical and portable classification based on optical galaxy properties
P50
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P50
description
Professor at the Institute for Astronomy in the Department of Physics at ETH Zürich
@en
astrofysicus
@nl
britisch-kanadischer Astrophysiker
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name
Simon Lilly
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Simon Lilly
@de
Simon Lilly
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Simon Lilly
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Simon Lilly
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Simon Lilly
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Simon Lilly
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西蒙·利利
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type
label
Simon Lilly
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Simon Lilly
@de
Simon Lilly
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Simon Lilly
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Simon Lilly
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Simon Lilly
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Simon Lilly
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西蒙·利利
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Simon J. Lilly
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Simon John Lilly
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prefLabel
Simon Lilly
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Simon Lilly
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Simon Lilly
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Simon Lilly
@es
Simon Lilly
@fr
Simon Lilly
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Simon Lilly
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西蒙·利利
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P1006
P214
P1006
P1153
35242659800
P166
P184
P19
P2070
simon-lilly-11819
P21
P214
P31
P463
P496
0000-0002-6423-3597
P549
P569
1959-01-01T00:00:00Z