about
sameAs
A test of the nature of cosmic acceleration using galaxy redshift distortions.The 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 ≤ 24.75Comparison of the VIMOS-VLT Deep Survey with the Munich semi-analytical modelThe 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 SurveyThe 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 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 functionThe VIMOS-VLT deep survey. Color bimodality and the mix of galaxy populations up to z~2The VIMOS VLT deep surveyAccurate photometric redshifts for the CFHT legacy survey calibrated using the VIMOS VLT deep surveyThe VIMOS VLT Deep Survey: the build-up of the colour–density relationThe VIMOS VLT Deep Survey: the faint type-1 AGN sampleThe GALEXVIMOS-VLT Deep Survey Measurement of the Evolution of the 1500 Å Luminosity FunctionThe cosmic star formation rate evolution from z = 5 to z = 0 from the VIMOS VLT deep surveyThe VIMOS VLT Deep Survey. Evolution of the luminosity functions by galaxy type up to z = 1.5 from first /session define format EPOCH1 = dataThe VIMOS-VLT Deep Survey Galaxy luminosity function per morphological type up to z = 1.2The VIMOS-VLT Deep Survey. The evolution of galaxy clustering per spectral type to z=~1.5The VIMOS-VLT Deep Survey. Luminosity dependence of clustering at z =~1A large population of galaxies 9 to 12 billion years back in the history of the UniverseThe VIMOS Integral Field Unit: Data‐Reduction Methods and Quality AssessmentThe VIMOS VLT Deep SurveyThe VIMOS VLT deep surveyThe VIMOS VLT deep survey. First epoch VVDS-deep survey: 11564 spectra with 17.5<=I_AB_<=24, and the redshift distribution over 0<=z<=5The VIMOS VLT deep surveyThe VIMOS-VLT deep survey Evolution of the galaxy luminosity function up to z = 2 in first epoch dataThe VIRMOS deep imaging survey. IV. Near-infrared observationsThe VVDS Data‐Reduction Pipeline: Introducing VIPGI, the VIMOS Interactive Pipeline and Graphical Interface
P50
Q34743650-AD44F34E-F39E-4A92-B723-F68CE6CE3BC5Q58035436-7AE4B28D-4310-4DB0-AEC3-7A5683165E6AQ58035583-DE2E5F7B-F987-4911-89A1-5370840E1DF1Q58035609-35402411-A0DB-4D87-A1F3-A62D7670A791Q58035614-518BADEE-E088-4DD1-9E81-2695969AFFEFQ58035668-7CE8C697-6840-41D4-8B04-1FCC0B522032Q58035677-F9BF7FE0-426A-4F38-AB8F-763ECA6826A6Q58035685-815EC964-CF6F-4A55-800A-A1DC8DAE6527Q58035688-7B3A3C9A-50A3-4428-89AA-5F187C5F5DA5Q58035689-0A171490-01AF-4503-BF7F-2E7443A80919Q58035704-C2E9D2D9-5512-435F-9161-17BC3379CE45Q58035707-5ACCAD1B-1182-40FD-A10A-0BC7E990454BQ58035709-7F934C7D-8E31-44C0-B3D3-1A1F45D5DB22Q58035711-42BA1527-849D-452D-AC51-F340BA0AF9EAQ58035714-A586B81E-913A-44BC-90FD-B8E69BD527C5Q58035722-CBD4D267-90EB-4235-AC31-B3A8F476C4FBQ58035736-87393C49-07C4-46AF-BDF8-7AACE0F3C77AQ58035739-D8BB6746-5226-463E-9542-98041B2AC66AQ58035744-AF3A6BC7-4F0E-4A99-B55E-846122A6B366Q58035751-DA539AD5-4FC0-48FB-9BAC-37B145F1265DQ58035764-39E3988C-14AA-469C-93BF-E625607BF762Q58035772-730E0747-43F8-488D-8AF1-AC1455EB211FQ58035786-7FA2E722-85EC-4D70-8E39-93A7D240F2A6Q58035789-4FE7189D-290F-428C-9F50-A4643B2751F9Q58035790-7C1C78B8-D702-42DF-AC32-9BAFFD81E03DQ58470251-FB884F16-24D2-4A5F-ABB0-F2727CF63903Q58908064-8C2A26E7-C8DD-4025-A59D-921AD923877AQ58908072-2DAC4CAE-4AD9-4FFE-9811-CE718872D332Q58908074-015EF436-3E72-4C8C-8BA4-7CFB060D1F4EQ58908077-1D645D01-CC49-4488-A659-95037A4FD911Q58908080-3126C2FA-677F-40F7-812C-ACD87F981229Q58908089-19E02EAE-47E3-4889-AFAD-227038C18F01Q58908094-DB1A0574-F614-455D-BEB7-70E3B7052681Q58908096-2AFA7BE6-3CE2-4901-A2A6-07B010A7FAE5Q58908098-B4449034-7548-4EFA-800B-26F74A03B924Q58908100-6FD4CA2C-2A53-44B0-829C-E1180D5DB3DDQ58908102-4DD1E351-5957-4577-A4C0-AEAA27375FC1Q58908105-F7568403-5BC9-4113-9623-8F85B10DBE63Q58908109-412D56AB-6E3C-4CB2-A3D4-A24F3787C5D5Q58908112-5D957535-1C5A-40E1-98FE-E001BAD4FE9B
P50
description
Italiaans onderzoeker
@nl
forsker
@nb
researcher ORCID ID = 0000-0003-2490-1834
@en
name
R. Merighi
@ast
R. Merighi
@nl
R. Merighi
@sl
Roberto Merighi
@en
Roberto Merighi
@es
Roberto Merighi
@nb
Roberto Merighi
@sq
type
label
R. Merighi
@ast
R. Merighi
@nl
R. Merighi
@sl
Roberto Merighi
@en
Roberto Merighi
@es
Roberto Merighi
@nb
Roberto Merighi
@sq
altLabel
R. Merighi
@en
prefLabel
R. Merighi
@ast
R. Merighi
@nl
R. Merighi
@sl
Roberto Merighi
@en
Roberto Merighi
@es
Roberto Merighi
@nb
Roberto Merighi
@sq
P106
P1153
6602870715
P27
P31
P496
0000-0003-2490-1834