about
A test of the nature of cosmic acceleration using galaxy redshift distortions.A 20 GHz bright sample for δ > 72° – II. Multifrequency follow-upzCOSMOS: A Large VLT/VIMOS Redshift Survey Covering 0 <z< 3 in the COSMOS FieldThe VIMOS Public Extragalactic Redshift Survey. Reconstruction of the redshift-space galaxy density fieldThe VIMOS Public Extragalactic Redshift Survey (VIPERS)The VIMOS Public Extragalactic Redshift Survey. Searching for cosmic voidsThe VIMOS Public Extragalactic Redshift Survey (VIPERS)The VIMOS Public Extragalactic Redshift Survey (VIPERS)The VIMOS Public Extragalactic Redshift Survey (VIPERS) - from the galaxy clustering ratio measured at z ~1The VIMOS Public Extragalactic Redshift Survey (VIPERS): A quiescent formation of massive red-sequence galaxies over the past 9 GyrThe VIMOS Public Extragalactic Survey (VIPERS)Radio-optical properties of extragalactic populations in the VIPERS SurveyThe VIMOS VLT Deep Survey final data release: a spectroscopic sample of 35 016 galaxies and AGN out to z ~ 6.7 selected with 17.5 ≤ iAB ≤ 24.75The VIMOS Public Extragalactic Redshift Survey (VIPERS)The VIMOS Public Extragalactic Redshift Survey (VIPERS)The VIMOS Public Extragalactic Redshift Survey (VIPERS)The VIMOS Public Extragalactic Redshift Survey (VIPERS)He II emitters in the VIMOS VLT Deep Survey: Population III star formation or peculiar stellar populations in galaxies at 2 <z< 4.6?The VIMOS Public Extragalactic Redshift Survey (VIPERS): spectral classification through principal component analysis★The power spectrum from the angular distribution of galaxies in the CFHTLS-Wide fields at redshift ∼0.7The star formation rate density and dust attenuation evolution over 12 Gyr with the VVDS surveysComparison of the VIMOS-VLT Deep Survey with the Munich semi-analytical modelThe VIMOS VLT Deep Survey: star formation rate density of Lyαemitters from a sample of 217 galaxies with spectroscopic redshifts 2 ≤ z ≤ 6.6The VIMOS-VLT deep survey: the group catalogueThe VIMOS-VLT Deep Survey: evolution in the halo occupation number since z∼ 1★The Vimos VLT deep survey. Stellar mass segregation and large-scale galaxy environment in the redshift range 0.2 < z < 1.4The VIMOS VLT Deep Survey. Evolution of the major merger rate since z ~ 1 from spectroscopically confirmed galaxy pairsPhysical properties of galaxies and their evolution in the VIMOS VLT Deep SurveyPhysical properties of galaxies and their evolution in the VIMOS VLT Deep SurveyThe VVDS-VLA deep field. IV. Radio-optical propertiesEddington ratios of faint AGN at intermediate redshift: evidence for a population of half-starved black holesThe 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 GyrThe Vimos VLT deep surveyThe VIMOS VLT deep survey. The K-band follow-up in the 0226-04 fieldThe VIMOS-VLT Deep Survey (VVDS). The dependence of clustering on galaxy stellar mass at z ~ 1The 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 = 1The VIMOS VLT Deep SurveyVVDS-SWIRE. Clustering evolution from a spectroscopic sample of galaxies with redshift 0.2 < z < 2.1 selected from Spitzer IRAC 3.6 {mu}m and 4.5 {mu}m photometryThe VVDS type-1 AGN sample: the faint end of the luminosity function
P50
Q34743650-A488DB56-1874-455D-8A56-47829A4F8442Q55672548-F52FA931-8C4B-401D-8DD3-FE3ED9B71AB8Q56556487-02319A06-2696-4E5E-A0E4-4F5A9F294D5FQ58035329-1C8DD3B1-DFF0-4992-8F28-43C68637E4BDQ58035334-3478745E-C8B6-48CD-ADE9-421FE67F67A0Q58035372-15530448-259B-4CCD-BB0F-1CFA74ACECE9Q58035381-76AA0933-4B76-4052-A1D6-835D2ABF9CACQ58035394-99719215-DFEC-465A-9650-4390E9C345B3Q58035412-EEE5C363-7821-4DC8-9708-D50755B71545Q58035417-CF7D0588-4DCD-41D5-A69C-4E04C8037386Q58035419-658556A2-597F-4099-9635-85DED7747320Q58035432-35776D7B-CBDD-4D2C-9E8B-42347D3B0745Q58035436-C0CE8D2F-F6DD-41E3-BD73-A762941BA991Q58035440-12A8B006-3F73-41EC-AD5D-FC7374EAB395Q58035443-C38DB518-11C4-4CBD-9C99-11C762BD2568Q58035447-A5F419F1-86BB-42F5-B852-879F4D5C3CCBQ58035449-33317F59-6C30-4050-A31B-AC025EDA131EQ58035453-F084CD63-4BEE-4F65-9915-8E0328B30FB6Q58035479-A14BA552-1F8A-451D-864E-72C6923A5DD6Q58035537-5D7C58E0-8020-4055-8386-1B2266626885Q58035539-BBC00B7F-7088-4074-850B-913D70C9C6A5Q58035583-AE9A7259-5B7A-4B31-A990-5C57530B8A43Q58035585-8D2AAD3D-650D-45AB-A77C-A2896DC27D6FQ58035609-893D3FE8-0361-4A89-BA9A-FA82512D056EQ58035614-9CB19CE9-05E3-4CEF-9B9D-0DA5B1221A97Q58035668-91EA2A54-28BA-4C8E-98A8-973955AE577BQ58035677-BBBCD648-11C8-4492-9ACF-D2A15FCDED61Q58035685-74B0B7F3-0BD5-45F6-AE6C-C4FEF841A3BAQ58035688-47B00664-9793-4115-ABAF-51BC98BE11C0Q58035689-B0E3D4FD-6B90-4D9E-80FD-8085FBF2D250Q58035704-B7BE9169-49E3-495B-AA89-8FC5DD235C9CQ58035707-85EDC6ED-4EC4-47CB-B244-5292F70672ADQ58035711-9723131A-4165-448D-8D16-012642672ADFQ58035714-B20F8736-9440-46B6-B507-221550725A8EQ58035722-C689236E-FE60-42BD-B76C-64C956CA19C6Q58035725-F2AFCE64-3C55-489D-A440-4A29BCD66A1BQ58035736-53344DDF-7CCC-4ED6-81BE-201AA19AE40CQ58035739-0644ADB0-833B-488E-9656-4955D99D7FE4Q58035744-F932B2AC-7494-43FE-8F1E-4E2985BE3A09Q58035751-1E95F4E2-AC3E-4FA0-8CD3-C28333F8A2CC
P50
description
forsker
@nb
hulumtuese
@sq
researcher
@en
wetenschapper
@nl
հետազոտող
@hy
name
A. Zanichelli
@ast
A. Zanichelli
@nl
Alessandra Zanichelli
@en
Alessandra Zanichelli
@es
Alessandra Zanichelli
@nb
type
label
A. Zanichelli
@ast
A. Zanichelli
@nl
Alessandra Zanichelli
@en
Alessandra Zanichelli
@es
Alessandra Zanichelli
@nb
altLabel
A. Zanichelli
@en
prefLabel
A. Zanichelli
@ast
A. Zanichelli
@nl
Alessandra Zanichelli
@en
Alessandra Zanichelli
@es
Alessandra Zanichelli
@nb
P106
P21
P31
P496
0000-0002-2893-023X