The VVDS Data‐Reduction Pipeline: Introducing VIPGI, the VIMOS Interactive Pipeline and Graphical Interface
about
A mature cluster with X-ray emission atz= 2.07The VIMOS Ultra-Deep Survey: ~10 000 galaxies with spectroscopic redshifts to study galaxy assembly at early epochs 2 < z ≃ 6The VIMOS Ultra-Deep Survey (VUDS): fast increase in the fraction of strong Lyman-α emitters from z = 2 to z = 6Discovery of a rich proto-cluster atz= 2.9 and associated diffuse cold gas in the VIMOS Ultra-Deep Survey (VUDS)Evidence for major mergers of galaxies at 2 ≲z< 4 in the VVDS and VUDS surveysThe VIMOS Public Extragalactic Redshift Survey (VIPERS): A quiescent formation of massive red-sequence galaxies over the past 9 GyrSpot the differenceThe VIMOS Public Extragalactic Redshift Survey (VIPERS)Obscured AGN at z ~ 1 from the zCOSMOS-Bright SurveyThe dominant role of mergers in the size evolution of massive early-type galaxies sincez ~ 1The VIMOS VLT Deep SurveyThe VIMOS VLT Deep Survey: star formation rate density of Lyαemitters from a sample of 217 galaxies with spectroscopic redshifts 2 ≤ z ≤ 6.6Tracking the impact of environment on the galaxy stellar mass function up toz ~ 1 in the 10 k zCOSMOS sampleThe zCOSMOS survey: the role of the environment in the evolution of the luminosity function of different galaxy typesThe zCOSMOS redshift survey: the role of environment and stellar mass in shaping the rise of the morphology-density relation from z ~ 1The 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 zCOSMOS redshift survey: the three-dimensional classification cube and bimodality in galaxy physical propertiesThe VIMOS VLT Deep Survey. Tracing the galaxy stellar mass assembly history over the last 8 GyrThe VIMOS VLT Deep SurveyThe VIMOS-VLT deep survey. Color bimodality and the mix of galaxy populations up to z~2The VIMOS VLT deep surveyCLASH-VLT: spectroscopic confirmation of az= 6.11 quintuply lensed galaxy in the Frontier Fields cluster RXC J2248.7-4431CLASH-VLT: The mass, velocity-anisotropy, and pseudo-phase-space density profiles of thez= 0.44 galaxy cluster MACS J1206.2-0847Integral field spectroscopy of four lensed quasars: analysis of their neighborhood and evidence for microlensingTelescope search for decaying relic axionsVIMOS-IFU survey of z~0.2 massive galaxy clusters. I. Observations of the strong lensing cluster Abell 2667F-VIPGI: a new adapted version of VIPGI for FORS2 spectroscopyThe 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 = dataSize evolution of star-forming galaxies with 2 < z < 4.5 in the VIMOS Ultra-Deep SurveyOn the connection between the metal-enriched intergalactic medium and galaxies: an O vi–galaxy cross-correlation study atz< 1CLASH-VLT: Substructure in the galaxy cluster MACS J1206.2-0847 from kinematics of galaxy populationsCLASH-VLT: The stellar mass function and stellar mass density profile of thez= 0.44 cluster of galaxies MACS J1206.2-0847An extragalactic spectroscopic survey of the SSA22 fieldThe VIMOS Public Extragalactic Redshift Survey (VIPERS)VIMOS Ultra-Deep Survey (VUDS): IGM transmission towards galaxies with 2.5 <z< 5.5 and the colour selection of high-redshift galaxiesA high definition view of the COSMOS Wall atz ~ 0.73
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The VVDS Data‐Reduction Pipeline: Introducing VIPGI, the VIMOS Interactive Pipeline and Graphical Interface
description
im November 2005 veröffentlichter wissenschaftlicher Artikel
@de
wetenschappelijk artikel
@nl
наукова стаття, опублікована в листопаді 2005
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name
The VVDS Data‐Reduction Pipeli ...... peline and Graphical Interface
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The VVDS Data‐Reduction Pipeli ...... peline and Graphical Interface
@nl
type
label
The VVDS Data‐Reduction Pipeli ...... peline and Graphical Interface
@en
The VVDS Data‐Reduction Pipeli ...... peline and Graphical Interface
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prefLabel
The VVDS Data‐Reduction Pipeli ...... peline and Graphical Interface
@en
The VVDS Data‐Reduction Pipeli ...... peline and Graphical Interface
@nl
P2093
P50
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P1476
The VVDS Data‐Reduction Pipeli ...... peline and Graphical Interface
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C. Marinoni
D. Bottini
D. Maccagni
P304
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10.1086/496937
P407
P50
P577
2005-11-01T00:00:00Z
P818
astro-ph/0409248
P819
2005PASP..117.1284S