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A deep kinematic survey of planetary nebulae in the Andromeda galaxy using the Planetary Nebula SpectrographIsolated Star Formation: A Compact H [CSC]ii[/CSC] Region in the Virgo ClusterThe edge of the M 87 halo and the kinematics of the diffuse light in the Virgo cluster coreThe build-up of the cD halo of M 87: evidence for accretion in the last GyrSloshing in its cD halo: MUSE kinematics of the central galaxy NGC 3311 in the Hydra I clusterIntracluster Planetary Nebulae in the Hydra I clusterStellar Kinematics for the Central Spheroid in the Polar Disk Galaxy NGC 4650APolar Ring Galaxies and the Tully‐Fisher Relation: Implications for the Dark Halo ShapeA 3D view of the Hydra I cluster core- II. Stellar populationsA 3D view of the Hydra I galaxy cluster core - I. Kinematic substructuresEddington ratios of faint AGN at intermediate redshift: evidence for a population of half-starved black holesThe VIMOS VLT Deep Survey: the build-up of the colour–density relationThe VIMOS VLT Deep Survey: the faint type-1 AGN sampleSpectroscopic monitoring of the BL Lac object AO 0235+164The Metallicity Distribution of Intracluster Stars in VirgoThe Resolved Stellar Populations of a Dwarf Spheroidal Galaxy in the Virgo ClusterVirgo’s Intracluster Globular Clusters as Seen by the Advanced Camera for SurveysThe GALEXVIMOS-VLT Deep Survey Measurement of the Evolution of the 1500 Å Luminosity FunctionThe GALEX-VVDS Measurement of the Evolution of the Far-Ultraviolet Luminosity Density and the Cosmic Star Formation RatePlanetary Nebula Spectrograph survey of S0 galaxy kinematics – II. Clues to the origins of S0 galaxiesThe Planetary Nebula Spectrograph survey of S0 galaxy kinematicsUnravelling the origins of S0 galaxies using maximum likelihood analysis of planetary nebulae kinematicsThe PN.S Elliptical Galaxy Survey: a standard ΛCDM halo around NGC 4374?★The 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. The evolution of galaxy clustering per spectral type to z=~1.5A 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 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 InterfaceThe VVDS-VLA deep field. II. Optical and near infrared identifications of VLA S_1.4GHz_>80{mu}Jy sources in the VIMOS VLT deep survey VVDS-02h fieldThe Vimos VLT deep survey: compact structures in the CDFSThe Very Large Telescope Visible Multi‐Object Spectrograph Mask Preparation SoftwareThe VIMOS VLT Deep SurveyThe VIRMOS deep imaging surveyVirmos-VLT deep survey (VVDS)The XMM-LSS survey
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description
hulumtuese
@sq
researcher
@en
wetenschapper
@nl
հետազոտող
@hy
name
Magda Arnaboldi
@ast
Magda Arnaboldi
@en
Magda Arnaboldi
@es
Magda Arnaboldi
@nl
Magda Arnaboldi
@sl
type
label
Magda Arnaboldi
@ast
Magda Arnaboldi
@en
Magda Arnaboldi
@es
Magda Arnaboldi
@nl
Magda Arnaboldi
@sl
prefLabel
Magda Arnaboldi
@ast
Magda Arnaboldi
@en
Magda Arnaboldi
@es
Magda Arnaboldi
@nl
Magda Arnaboldi
@sl
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P1153
56275157900
P21
P31
P496
0000-0001-7214-3009