Using large galaxy surveys to distinguish z ≃ 0.5 quiescent galaxy models

about

A 2.5 per cent measurement of the growth rate from small-scale redshift space clustering of SDSS-III CMASS galaxies Tidal stripping as a test of satellite quenching in redMaPPer clusters Mapping stellar content to dark matter haloes – II. Halo mass is the main driver of galaxy quenching

P2860

Q57630644-7B6EDA2E-9903-473B-BB68-822DE01FFD8C Q57686336-00BEF1D3-F1DF-4356-8A72-1D66BBBC4C23 Q58490049-FB1C1C6D-D981-49E8-B31E-78109642906E

P2860

Using large galaxy surveys to distinguish z ≃ 0.5 quiescent galaxy models

Item

http://www.wikidata.org/entity/Q57630669

description

im März 2014 veröffentlichter wissenschaftlicher Artikel

@de

wetenschappelijk artikel

@nl

наукова стаття, опублікована в березні 2014

@uk

name

Using large galaxy surveys to distinguish z ≃ 0.5 quiescent galaxy models

@en

Using large galaxy surveys to distinguish z ≃ 0.5 quiescent galaxy models

@nl

type

Item

label

Using large galaxy surveys to distinguish z ≃ 0.5 quiescent galaxy models

@en

Using large galaxy surveys to distinguish z ≃ 0.5 quiescent galaxy models

@nl

prefLabel

Using large galaxy surveys to distinguish z ≃ 0.5 quiescent galaxy models

@en

Using large galaxy surveys to distinguish z ≃ 0.5 quiescent galaxy models

@nl

P1476

Using large galaxy surveys to distinguish z ≃ 0.5 quiescent galaxy models

@en

P2093

J. D. Cohn

http://www.w3.org/2001/XMLSchema#string

P2860

GADGET: a code for collisionless and gasdynamical cosmological simulations

The Structure of Cold Dark Matter Halos

Galaxy Zoo: disentangling the environmental dependence of morphology and colour

The evolution of large-scale structure in a universe dominated by cold dark matter

Baryon Dynamics, Dark Matter Substructure, and Galaxies

Numerical simulations of the dark universe: State of the art and the next decade

Galaxy Luminosity Functions toz∼1 from DEEP2 and COMBO‐17: Implications for Red Galaxy Formation

Modeling Luminosity‐dependent Galaxy Clustering through Cosmic Time

A Wide‐FieldHubble Space TelescopeStudy of the Cluster Cl 0024+16 atz= 0.4. I. Morphological Distributions to 5 Mpc Radius

Evolution sincez= 0.5 of the Morphology‐Density Relation for Clusters of Galaxies

P304

1712–1729

http://www.w3.org/2001/XMLSchema#string

P31

scholarly article

P356

10.1093/MNRAS/STU367

http://www.w3.org/2001/XMLSchema#string

P407

English

P433

http://www.w3.org/2001/XMLSchema#string

P478

440

http://www.w3.org/2001/XMLSchema#string

P50

Martin White

P577

2014-03-26T00:00:00Z

http://www.w3.org/2001/XMLSchema#dateTime

P818

1311.0850

http://www.w3.org/2001/XMLSchema#string

P819

2014MNRAS.440.1712C

http://www.w3.org/2001/XMLSchema#string

Using large galaxy surveys to distinguish z ≃ 0.5 quiescent galaxy models

about

P2860

P2860

Using large galaxy surveys to distinguish z ≃ 0.5 quiescent galaxy models

description

name

type

label

prefLabel

P1433

P1476

P2093

P2860

P304

P31

P356

P407

P433

P478

P50

P577

P818

P819

P356

P1433

P1476

P2093

P2860

P304

P31

P356

P407

P433

P478

P50

P577

P818

P819