about
The need for speed: escape velocity and dynamical mass measurements of the Andromeda galaxyHerschel ★ -ATLAS: properties of dusty massive galaxies at low and high redshiftsGalaxy And Mass Assembly (GAMA): linking star formation histories and stellar mass growthGalaxy And Mass Assembly (GAMA): galaxy radial alignments in GAMA groupsHerschel★-ATLAS: rapid evolution of dust in galaxies over the last 5 billion yearsGAMA: towards a physical understanding of galaxy formationHerschel-ATLAS: Dust temperature and redshift distribution of SPIRE and PACS detected sources using submillimetre coloursHerschel-ATLAS: Evolution of the 250 µm luminosity function out to z=0.54MOST: 4-metre Multi-Object Spectroscopic TelescopeGalaxy And Mass Assembly (GAMA): understanding the wavelength dependence of galaxy structure with bulge-disc decompositionsGalaxy And Mass Assembly (GAMA): the wavelength-dependent sizes and profiles of galaxies revealed by MegaMorphGalaxy And Mass Assembly (GAMA): trends in galaxy colours, morphology, and stellar populations with large-scale structure, group, and pair environmentsHerschel-ATLAS/GAMA: spatial clustering of low-redshift submm galaxiesGalaxy And Mass Assembly (GAMA): galaxy environments and star formation rate variationsGAMA/H-ATLAS: the ultraviolet spectral slope and obscuration in galaxiesWhich haloes host Herschel-ATLAS galaxies in the local Universe?Galaxy and mass assembly (GAMA): dust obscuration in galaxies and their recent star formation historiesSubstructure analysis of selected low-richness 2dFGRS clusters of galaxiesNew Upper Limit on the Total Neutrino Mass from the 2 Degree Field Galaxy Redshift SurveyH-ATLAS/GAMA: the nature and characteristics of optically red galaxies detected at submillimetre wavelengthsGalaxy And Mass Assembly (GAMA): testing galaxy formation models through the most massive galaxies in the UniverseThe 2dF-SDSS LRG and QSO (2SLAQ) Luminous Red Galaxy SurveyH-ATLAS/GAMA: quantifying the morphological evolution of the galaxy population using cosmic calorimetryThe environment and characteristics of low-redshift galaxies detected by the Herschel-ATLASThe Herschel ATLASThe SAMI Galaxy Survey: spatially resolving the main sequence of star formationThe SAMI Galaxy Survey: Data Release One with emission-line physics value-added productsGalaxy and Mass Assembly (GAMA): probing the merger histories of massive galaxies via stellar populationsGalaxy and Mass Assembly (GAMA): Exploring the WISE Web in G12Galaxy And Mass Assembly (GAMA): deconstructing bimodality – I. Red ones and blue onesThe SAMI Galaxy Survey: cubism and covariance, putting round pegs into square holesHerschel-ATLAS/GAMA: a difference between star formation rates in strong-line and weak-line radio galaxies★The infrared properties of sources matched in the WISE all-sky and Herschel ATLAS surveysThe SAMI Galaxy Survey: Data Release Two with absorption-line physics value-added productsGalaxy And Mass Assembly (GAMA): the large-scale structure of galaxies and comparison to mock universesGalaxy And Mass Assembly (GAMA): a deeper view of the mass, metallicity and SFR relationshipsGalaxy And Mass Assembly (GAMA): the connection between metals, specific SFR and H i gas in galaxies: the Z–SSFR relationGalaxy And Mass Assembly (GAMA): blue spheroids within 87 MpcGalaxy And Mass Assembly: automatic morphological classification of galaxies using statistical learningGAMA/G10-COSMOS/3D-HST: the 0 < z < 5 cosmic star formation history, stellar-mass, and dust-mass densities
P50
Q56112705-5C8FF4AC-D7C5-4471-99CA-345610349967Q56550399-3DC5DC80-5B5F-48ED-995C-EB69B2E78310Q56814771-6087AC46-3BFB-4469-819D-66B0B28B02B9Q56908179-79DD13BE-F605-48DE-A8EA-C31B8E67C173Q57088410-2F4CF2C8-520F-4EC2-A69E-CF396AF7708CQ57533457-BFE5C02E-ED3C-4D71-AE02-788B1A6A49C1Q58217322-DA6F2D6F-9CF5-4111-A246-AF2A95E58E0FQ58217326-DE00B203-C4A1-4B3C-A0C6-CBA69885AA08Q58489149-11F8AC90-7C06-48F3-B62B-2E69FBDE89A2Q58492562-E16D7921-D915-48E1-AB7C-DABA037111E9Q58492574-A086152B-6BD6-4600-A162-0A1E6C81F9AEQ58831047-09FD99CA-34C1-494B-8514-60F74193E11EQ58831088-05836C41-DA41-4D78-98C3-0D37FAC0BF3BQ58831096-26EB7A9B-E353-40D7-AD04-8779BB6E74FAQ58831112-B7778230-B957-4479-8527-8181FA6EDFE4Q58831123-7BB96B62-3AB3-42E3-97C7-D119F4221DD6Q58831126-2372071C-1E95-47BF-B924-2F80268D56B8Q58910170-FD3C5EB6-F745-4A54-9E02-1EA40AC57304Q58910240-AE3DCEC7-2A8F-4EAB-99B4-37CEE1A605F1Q58912890-F40744D4-1262-486E-A8E9-C205F3CB0274Q58915519-7DA343CD-AE16-4457-949E-E8234A731F09Q58915651-FA64EC29-C6F1-438B-81ED-AEC3F4F6DFA0Q58916242-82283A56-3CCA-4A7A-A37F-1C7CB824AE76Q58916381-94A85BC6-3AB7-4646-B390-1601DF7C98C3Q58916437-C29B9A78-8FD7-40C6-9DEC-1DAC80111675Q59718386-96602660-E861-43F3-A7E0-6FF8269E0819Q59718399-E61A0840-F0D4-43A9-B1FD-D1C74FB3ED1CQ59718464-F150C43D-1D3B-4954-9CF6-BC059C779A74Q59718476-FDBDD6CE-EEDB-41FB-8AF4-90278691EB38Q59718585-7DF35266-33AB-4A8D-BB11-65617FC561E7Q59718593-183DD738-9843-4FEC-9B82-9D8C75C2EA05Q59718709-A8D8171A-C0BE-45EC-BF17-99666E8D29E6Q59720045-AC1C88B0-2245-460B-AC85-CF8BAE777C84Q59743420-CC68FA54-248E-42E3-84EF-6060F2B5C5B7Q59756692-BF5229E1-F307-4C65-A017-C858C0B94DE9Q59756701-40BBD177-EC79-41A9-9C66-16F7C182D7F3Q59756705-CF6257BA-8E84-4E9F-809B-2A19DA5C0A90Q59807151-09B485D4-E507-47BD-B584-17C63EC48A1EQ59807157-F38DA5CD-5325-4C33-9867-A4DDFAF3A541Q59807202-46DF14AB-DF86-43DA-B8ED-4D6172A9D8E1
P50
description
onderzoeker
@nl
researcher
@en
հետազոտող
@hy
name
Simon Driver
@ast
Simon Driver
@en
Simon Driver
@es
Simon Driver
@fr
Simon Driver
@nl
type
label
Simon Driver
@ast
Simon Driver
@en
Simon Driver
@es
Simon Driver
@fr
Simon Driver
@nl
altLabel
S. Driver
@en
prefLabel
Simon Driver
@ast
Simon Driver
@en
Simon Driver
@es
Simon Driver
@fr
Simon Driver
@nl
P106
P1412
P21
P31
P496
0000-0001-9491-7327