about
Hexabundles: imaging fiber arrays for low-light astronomical applications.Near‐Infrared Spectroscopy of High‐Redshift Active Galactic Nuclei. I. A Metallicity–Accretion Rate RelationshipThe WiggleZ Dark Energy Survey: the transition to large-scale cosmic homogeneityA pilot survey for KX QSOs in the UKIDSS Ultra Deep Survey FieldGalaxy And Mass Assembly (GAMA): linking star formation histories and stellar mass growthGalaxy And Mass Assembly (GAMA): Panchromatic Data Release (far-UV–far-IR) and the low-zenergy budgetGalaxy And Mass Assembly (GAMA): spectroscopic analysisErratum: 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< 1WiggleZ 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: the selection function and z= 0.6 galaxy power spectrumThe WiggleZ Dark Energy Survey: small-scale clustering of Lyman-break galaxies atz< 1The WiggleZ Dark Energy SurveyHerschel-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=0.5Galaxy And Mass Assembly: evolution of the Hα luminosity function and star formation rate density up to z < 0.35Herschel-ATLAS/GAMA: spatial clustering of low-redshift submm galaxiesGalaxy And Mass Assembly (GAMA): galaxy environments and star formation rate variationsHerschel-ATLAS: counterparts from the ultraviolet-near-infrared in the science demonstration phase catalogue★GAMA/H-ATLAS: the ultraviolet spectral slope and obscuration in galaxiesGalaxy and Mass Assembly (GAMA): the star formation rate dependence of the stellar initial mass functionWhich haloes host Herschel-ATLAS galaxies in the local Universe?Galaxy and mass assembly (GAMA): dust obscuration in galaxies and their recent star formation historiesMegaZ-LRG: a photometric redshift catalogue of one million SDSS luminous red galaxiesThe 2dF-SDSS LRG and QSO (2SLAQ) Luminous Red Galaxy SurveyNear‐Infrared Spectroscopy of High‐Redshift Active Galactic Nuclei. II. Disappearing Narrow‐Line Regions and the Role of AccretionKOALA: a wide-field 1000 element integral-field unit for the Anglo-Australian Telescope
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P50
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onderzoeker
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հետազոտող
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Scott Croom
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Scott M. Croom
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Scott M. Croom
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S M Croom
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S.M. Croom
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Scott Croom
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Scott Croom
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Scott M. Croom
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Scott M. Croom
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P106
P31
P496
0000-0003-2880-9197