about
Strongly baryon-dominated disk galaxies at the peak of galaxy formation ten billion years ago.The WiggleZ Dark Energy Survey: the transition to large-scale cosmic homogeneityIonized and Molecular Gas Kinematics in a z = 1.4 Star-forming GalaxyGAMA/WiggleZ: the 1.4 GHz radio luminosity functions of high- and low-excitation radio galaxies and their redshift evolution toz= 0.75Erratum: The stellar masses of ∼40 000 UV-selected galaxies from the WiggleZ survey at 0.3 < z < 1.0: analogues of Lyman break galaxies?The WiggleZ Dark Energy Survey: improved distance measurements to z = 1 with reconstruction of the baryonic acoustic featureThe WiggleZ Dark Energy Survey: probing the epoch of radiation domination using large-scale structureThe stellar masses of ∼ 40 000 UV selected Galaxies from the WiggleZ survey at 0.3<z<1.0: analogues of Lyman break galaxies?The WiggleZ Dark Energy Survey: measuring the cosmic growth rate with the two-point galaxy correlation functionThe WiggleZ Dark Energy Survey: constraining galaxy bias and cosmic growth with three-point correlation functionsThe WiggleZ Dark Energy Survey: star formation in UV-luminous galaxies from their luminosity functionsThe WiggleZ Dark Energy Survey: Final data release and cosmological resultsThe WiggleZ Dark Energy Survey: joint measurements of the expansion and growth history atz< 1THE WiggleZ DARK ENERGY SURVEY: GALAXY EVOLUTION AT 0.25 ⩽z⩽ 0.75 USING THE SECOND RED-SEQUENCE CLUSTER SURVEYWiggleZ Dark Energy Survey: Cosmological neutrino mass constraint from blue high-redshift galaxiesThe WiggleZ Dark Energy Survey: direct constraints on blue galaxy intrinsic alignments at intermediate redshiftsThe WiggleZ Dark Energy Survey: high-resolution kinematics of luminous star-forming galaxiesThe WiggleZ Dark Energy Survey: mapping the distance-redshift relation with baryon acoustic oscillationsThe WiggleZ Dark Energy Survey: measuring the cosmic expansion history using the Alcock-Paczynski test and distant supernovaeThe WiggleZ Dark Energy Survey: testing the cosmological model with baryon acoustic oscillations at z= 0.6The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9The WiggleZ Dark Energy Survey: survey design and first data releaseThe WiggleZ Dark Energy Survey: the selection function and z= 0.6 galaxy power spectrumTHE SINS/zC-SINF SURVEY OFz∼ 2 GALAXY KINEMATICS: EVIDENCE FOR POWERFUL ACTIVE GALACTIC NUCLEUS-DRIVEN NUCLEAR OUTFLOWS IN MASSIVE STAR-FORMING GALAXIESA consistent study of metallicity evolution at 0.8 < z < 2.6DYNAMO – I. A sample of Hα-luminous galaxies with resolved kinematicsThe WiggleZ Dark Energy Survey: final data release and the metallicity of UV-luminous galaxiesKMOS3D Reveals Low-level Star Formation Activity in Massive Quiescent Galaxies at 0.7 < z < 2.7Falling Outer Rotation Curves of Star-forming Galaxies at 0.6 ≲ z ≲ 2.6 Probed with KMOS3D and SINS/zC-SINFKMOS3D: dynamical constraints on the mass budget in early star-forming disksThe KMOS3D Survey: Rotating Compact Star-forming Galaxies and the Decomposition of Integrated Line WidthsRotating Starburst Cores in Massive Galaxies at z = 2.5The Evolution of the Tully–Fisher Relation between z ∼ 2.3 and z ∼ 0.9 with KMOS3DBulge-forming galaxies with an extended rotating disk at z ~ 2The evolution of metallicity and metallicity gradients from z = 2.7 to 0.6 with KMOS3D
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description
onderzoeker
@nl
researcher ORCID ID = 0000-0003-1657-7878
@en
name
Emily Wisnioski
@ast
Emily Wisnioski
@en
Emily Wisnioski
@es
Emily Wisnioski
@nl
type
label
Emily Wisnioski
@ast
Emily Wisnioski
@en
Emily Wisnioski
@es
Emily Wisnioski
@nl
prefLabel
Emily Wisnioski
@ast
Emily Wisnioski
@en
Emily Wisnioski
@es
Emily Wisnioski
@nl
P106
P1153
35301157800
P21
P31
P496
0000-0003-1657-7878