The SWIRE-VVDS-CFHTLS surveys: stellar mass assembly over the last 10 Gyr. Evidence for a major build up of the red sequence between z = 2 and z = 1
about
Evolution of the H β + [O iii] and [O ii] luminosity functions and the [O ii] star formation history of the Universe up toz ∼ 5 from HiZELSCFHTLenS: the relation between galaxy dark matter haloes and baryons from weak gravitational lensingGOODS-Herschel: dust attenuation properties of UV selected high redshift galaxiesThe stellar masses of ∼ 40 000 UV selected Galaxies from the WiggleZ survey at 0.3<z<1.0: analogues of Lyman break galaxies?MASSIV: Mass Assembly Survey with SINFONI in VVDSMASSIV: Mass Assembly Survey with SINFONI in VVDSIntegral field spectroscopy with SINFONI of VVDS galaxiesThe VIMOS Ultra-Deep Survey: ~10 000 galaxies with spectroscopic redshifts to study galaxy assembly at early epochs 2 < z ≃ 6VIMOS Ultra-Deep Survey (VUDS): Witnessing the assembly of a massive cluster atz~ 3.3The VIMOS Public Extragalactic Redshift Survey (VIPERS): A quiescent formation of massive red-sequence galaxies over the past 9 GyrMass assembly in quiescent and star-forming galaxies since z ≃ 4 from UltraVISTAThe dominant role of mergers in the size evolution of massive early-type galaxies sincez ~ 1The evolution of quiescent galaxies at high redshifts (z≥ 1.4)The VIMOS VLT Deep SurveyComparison of the VIMOS-VLT Deep Survey with the Munich semi-analytical modelThe zCOSMOS survey. The dependence of clustering on luminosity and stellar mass at $z=0.2$–1Integral field spectroscopy with SINFONI of VVDS galaxies. I. Galaxy dynamics and mass assembly at 1.2 < z < 1.6The VIMOS VLT Deep Survey. Evolution of the major merger rate since z ~ 1 from spectroscopically confirmed galaxy pairsThe VVDS-SWIRE-GALEX-CFHTLS surveys: physical properties of galaxies at z below 1.2 from photometric dataThe VIMOS VLT Deep Survey. Tracing the galaxy stellar mass assembly history over the last 8 GyrGalaxy Zoo: evidence for diverse star formation histories through the green valleyThe WIRCam Deep Survey II. Mass selected clusteringThe WIRCam Deep Survey I. Counts, colours, and mass-functions derived from near-infrared imaging in the CFHTLS deep fieldsHubble Frontier Fields: the geometry and dynamics of the massive galaxy cluster merger MACSJ0416.1-2403A weak lensing mass reconstruction of the large-scale filament feeding the massive galaxy cluster MACS J0717.5+3745The fraction of quiescent massive galaxies in the early UniverseEvidence for two modes of black hole accretion in massive galaxies at z∼2COMMISSION 47: COSMOLOGYExtragalactic background light inferred from AEGIS galaxy-SED-type fractionsA high definition view of the COSMOS Wall atz ~ 0.73Hidden starbursts and active galactic nuclei at 0 < z < 4 from theHerschel-VVDS-CFHTLS-D1 field: Inferences on coevolution and feedbackGMASS ultradeep spectroscopy of galaxies at z ~ 2 II. Superdense passive galaxies: how did they form and evolve?The KMOS Redshift One Spectroscopic Survey (KROSS): the Tully–Fisher relation atz∼ 1The Atacama Cosmology Telescope: the stellar content of galaxy clusters selected using the Sunyaev–Zel'dovich effectThe VIMOS Public Extragalactic Redshift Survey (VIPERS)The VIMOS Public Extragalactic Redshift Survey (VIPERS)AKs-band-selected catalogue of objects in the ALHAMBRA surveyRevealing X-ray obscured quasars in SWIRE sources with extreme mid-IR/optical flux ratiosPolycyclic aromatic hydrocarbon feature deficit of starburst galaxies in the AKARI North Ecliptic Pole Deep fieldStar Formation and AGN Activity in Galaxies Classified Using the 1.6 μm Bump and PAH Features atz= 0.4–2
P2860
Q56550141-AF76C32E-EB54-40A2-A543-209FD5BF9056Q57651659-AD0FD692-1A51-4A4A-8275-4B8AE6968C85Q57710892-6B6A0C87-57ED-4059-8F84-7646649033DCQ57769623-F1CCE94C-1EED-44E1-9803-5CF88065B45AQ57854319-BE07D091-22C8-4EFC-A0B3-181ADA675C9BQ57854385-A73EDAEB-10D1-456E-BCFD-7FD0B9672017Q57854861-FEA5EB29-E608-44FA-9316-6E08CAF6AA69Q58035346-7833AC3B-ED5A-44DE-98D6-28B2F9D3DF69Q58035359-B4BD27FE-C03D-4CB2-9E43-B2AE48C4205AQ58035417-E166F3C6-2435-4BB4-A95B-C5CCA82F7E02Q58035460-09906572-FFC9-4E0C-AE0D-9CEFA4ED20DCQ58035492-8CB2F480-6B9E-4B93-B930-15A34BC3E94FQ58035564-0ACF944B-B01A-41A3-B568-FB7FA9F16A8CQ58035567-0AF6F451-430E-42B8-9AE1-2AF16570DDB6Q58035583-35C41DB8-FEC2-4B8B-A2CD-09EFDA768464Q58035661-23894B9A-52E2-4A83-AA2E-F26B59A5D3E0Q58035664-AE4CE313-D895-493C-AF5B-A0F1861B751CQ58035677-3AFD5F83-FEB8-4831-AD9C-280F6D8B2B31Q58035707-F70437C6-4264-4A79-A658-867680CAEFE7Q58035711-6ABF8E26-B4A5-4E3D-8E96-A4E1910462A3Q58245916-460973C4-1A16-4E11-841F-58155B979B72Q58246868-52E3FF70-C15B-40DC-BD71-5074382F9708Q58246897-21246EB9-4069-439A-BC8E-77FA45EB2399Q58489673-324B1BD1-7914-4966-AF33-29F6AAA706B5Q58489726-8CA9599A-8889-462E-AEED-844C13BE2352Q58907880-08C83CD8-DF82-4FF9-BF55-03E356B33929Q58908416-678C5E78-1D2E-4B6F-A455-5B7737B1F280Q58908637-2BABCD82-6AE5-406B-B37A-366860B010B6Q58909855-D2C39AA3-AE0E-4420-8EB7-C84D9A99E09EQ58910619-96E16EB5-88F0-4EA4-A838-0C0F93FC1DECQ58910679-C0736B2A-0D75-48EA-A57D-662825A336A0Q58910766-5B4393EA-E465-4B1B-90EC-43D76165B1D9Q58916861-00F21C38-9CCD-45BB-94A9-F363D8E783CEQ58919238-43A59D03-6287-40A2-A0F1-E4DB5F7D1DE2Q58922646-B3EF237D-20C3-4C44-B0C5-926B4D580832Q58922667-010EC182-CF64-430F-89C6-A77282597EFBQ58982193-F4210FE1-5B82-4E8B-A02E-CF91598EA094Q58982437-CA125E0C-DF7C-4E51-BF20-0FBAE668E3F6Q58983352-1A53EA40-F55D-4F63-BB47-1EE85CA630EFQ58983375-1FFE5153-D92F-4ABA-B037-66842EBBD448
P2860
The SWIRE-VVDS-CFHTLS surveys: stellar mass assembly over the last 10 Gyr. Evidence for a major build up of the red sequence between z = 2 and z = 1
description
article publié dans la revue scientifique Astronomy and Astrophysics
@fr
im September 2007 veröffentlichter wissenschaftlicher Artikel
@de
scientific article published in Astronomy and Astrophysics
@en
wetenschappelijk artikel
@nl
наукова стаття, опублікована у вересні 2007
@uk
name
The SWIRE-VVDS-CFHTLS surveys: ...... quence between z = 2 and z = 1
@en
The SWIRE-VVDS-CFHTLS surveys: ...... quence between z = 2 and z = 1
@nl
type
label
The SWIRE-VVDS-CFHTLS surveys: ...... quence between z = 2 and z = 1
@en
The SWIRE-VVDS-CFHTLS surveys: ...... quence between z = 2 and z = 1
@nl
prefLabel
The SWIRE-VVDS-CFHTLS surveys: ...... quence between z = 2 and z = 1
@en
The SWIRE-VVDS-CFHTLS surveys: ...... quence between z = 2 and z = 1
@nl
P2093
P2860
P50
P1476
The SWIRE-VVDS-CFHTLS surveys: ...... quence between z = 2 and z = 1
@en
P2093
C. J. Walcher
C. Lonsdale
C. Marinoni
D. Bottini
D. Maccagni
P2860
P304
P356
10.1051/0004-6361:20077632
P407
P50
P577
2007-09-24T00:00:00Z
P818
P819
2007A&A...476..137A