Karl Glazebrook Australian astronomer
Glazebrook, Karl, 1965-
VIAF ID: 309870374 (Personal)
Permalink: http://viaf.org/viaf/309870374
Preferred Forms
4xx's: Alternate Name Forms (15)
Works
| Title | Sources |
|---|---|
| THE ABSENCE OF AN ENVIRONMENTAL DEPENDENCE IN THE MASS–METALLICITY RELATION ATz= 2 |
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| Afterglow observations of Fermi large area telescope gamma-ray bursts and the emerging class of hyper-energetic events |
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| Cold-mode accretion: driving the fundamental mass-metallicity relation at z ~ 2 |
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| DISCOVERY OF LYMAN BREAK GALAXIES ATz∼ 7 FROM THE zFourGE SURVEY |
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| EXTREME GAS FRACTIONS IN CLUMPY, TURBULENT DISK GALAXIES ATz∼ 0.1 |
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| THE FOURSTAR GALAXY EVOLUTION SURVEY (ZFOURGE): ULTRAVIOLET TO FAR-INFRARED CATALOGS, MEDIUM-BANDWIDTH PHOTOMETRIC REDSHIFTS WITH IMPROVED ACCURACY, STELLAR MASSES, AND CONFIRMATION OF QUIESCENT GALAXIES TOz∼ 3.5 |
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| THE HOST GALAXIES OFSWIFTDARK GAMMA-RAY BURSTS: OBSERVATIONAL CONSTRAINTS ON HIGHLY OBSCURED AND VERY HIGH REDSHIFT GRBs |
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| KECK/MOSFIRE SPECTROSCOPIC CONFIRMATION OF A VIRGO-LIKE CLUSTER ANCESTOR ATz= 2.095 |
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| The SAMI galaxy survey: toward a unified dynamical scaling relation for galaxies of all types |
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| Satellite quenching and galactic conformity at 0.3 < z < 2.5 |
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| Scaling relations of star-forming regions: from kpc-sized clumps to H ii regions |
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| Scheduled Discoveries of 7+ High-Redshift Supernovae:First Cosmology Results and Bounds on q 0 |
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| The Science Case for PILOT II: the Distant Universe |
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| Science Programs for a 2-m Class Telescope at Dome C, Antarctica: PILOT, the Pathfinder for an International Large Optical Telescope |
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| The SDSS Photometric Catalog, Release 6 |
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| Selection and Photometric Properties of K+A Galaxies |
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| The SFR-M* relation and empirical star-formation histories from ZFOURGE at 0.5 < z < 4 |
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| THE SIZES OF MASSIVE QUIESCENT AND STAR-FORMING GALAXIES ATz∼ 4 WITH ZFOURGE AND CANDELS |
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| The Sloan Digital Sky Survey: The Cosmic Spectrum and Star Formation History |
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| A small-area faint KX redshift survey for QSOs in the ESO Imaging SurveyChandraDeep Field South |
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| Spectroscopic Classifications of DES transients by OzDES |
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| A spectroscopic measure of the star formation rate density in dwarf galaxies atz∼ 1 |
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| A spectroscopic measurement of galaxy formation time-scales with the Redshift One LDSS3 Emission line Survey |
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| The star formation history of the Hubble sequence: spatially resolved colour distributions of intermediate-redshift galaxies in the Hubble Deep Field |
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| Star-Forming, Recently Star-Forming, and “Red and Dead” Galaxies at 1 < Z < 2 |
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| The stellar mass–size relation for cluster galaxies at z = 1 with high angular resolution from the Gemini/GeMS multiconjugate adaptive optics system |
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| A Study of Quasar Selection in the Supernova Fields of the Dark Energy Survey |
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| A study of selection methods for Hα-emitting galaxies atz∼ 1.3 for the Subaru/FMOS galaxy redshift survey for cosmology |
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| The Subaru FMOS galaxy redshift survey (FastSound). IV. New constraint on gravity theory from redshift space distortions atz∼ 1.4 |
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| Substructure analysis of selected low-richness 2dFGRS clusters of galaxies |
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| Supernova 2001O in anonymous galaxy |
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| A supernova at Z = 0.458 and implications for measuring the cosmological deceleration |
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| Supernova host galaxies in the dark energy survey: I. Deep coadds, photometry, and stellar masses |
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| Suppression of the near-infrared OH night-sky lines with fibre Bragg gratings - first results |
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| A test of SDSS aperture corrections using integral-field spectroscopy |
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| Testing Feedback-regulated Star Formation in Gas-rich, Turbulent Disk Galaxies |
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| Testing gravity using galaxy-galaxy lensing and clustering amplitudes in KiDS-1000, BOSS, and 2dFLenS |
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| Testing Potential New Sites for Optical Telescopes in Australia |
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| The Theta-z relation for HST bulges and disks out to Z approximately equal 0.8 |
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| The Tully-Fisher relation for 25 000 Sloan Digital Sky Survey galaxies as a function of environment |
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| The Type Ia Supernova Rate at z ~ 0.4 |
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| Universal fitting formulae for baryon oscillation surveys |
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| An unusual high-redshift object discovered with the Hubble Space Telescope: peculiar starburst galaxy or new gravitational lens? |
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| UV to IR luminosities and dust attenuation determined from ~4000 k-selected galaxies at 1 < z < 3 in the ZFOURGE survey |
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| When do early-type galaxies form? |
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| WiggleZ Dark Energy Survey: Cosmological neutrino mass constraint from blue high-redshift galaxies |
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| The WiggleZ Dark Energy Survey: high-resolution kinematics of luminous star-forming galaxies |
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| The WiggleZ Dark Energy Survey: measuring the cosmic expansion history using the Alcock-Paczynski test and distant supernovae |
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| The WiggleZ Dark Energy Survey: small-scale clustering of Lyman-break galaxies atz< 1 |
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| The WiggleZ Dark Energy Survey: testing the cosmological model with baryon acoustic oscillations at z= 0.6 |
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| The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9 |
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| The WiggleZ Dark Energy Survey: the selection function and z= 0.6 galaxy power spectrum |
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| The WiggleZ Dark Energy Survey: the transition to large-scale cosmic homogeneity |
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| WiggleZ 암흑 에너지 설문조사: 설문조사 디자인 및 첫 번째 데이터 릴리스 |
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| XMS and NG1dF: extreme multiplex spectrographs for wide-field multi-object spectroscopy |
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| Z-FIRE: ISM properties of the z = 2.095 COSMOS cluster |
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| ZFIRE: a KECK/MOSFIRE spectroscopic survey of galaxies in rich environments at z ~ 2 |
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| ZFIRE: galaxy cluster kinematics, H{alpha} star formation rates, and gas phase metallicities of XMM-LSS J02182-05102 at z_cl_ = 1.6232 |
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| ZFIRE: similar stellar growth in H{alpha}-emitting cluster and field galaxies at z ~ 2 |
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| ZFIRE: The Evolution of the Stellar Mass Tully–Fisher Relation to Redshift ∼2.2 |
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| ZFIRE: the kinematics of star-forming galaxies as a function of environment at z ~ 2 |
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| ZFIRE: using Hα equivalent widths to investigate the in situ initial mass function at z ∼ 2 |
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| ZFOURGE/CANDELS: on the evolution of M* galaxy progenitors from z = 3 to 0.5 |
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| ZFOURGE catalogue of AGN candidates: an enhancement of 160-μm-derived star formation rates in active galaxies toz = 3.2 |
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| ZFOURGE: extreme 5007 {AA} emission may be a common early-lifetime phase for star-forming galaxies at z > 2.5 |
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| ZFOURGE: Using composite spectral energy distributions to characterize galaxy populations at 1 < z < 4 |
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