18.1k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- J. Bland-Hawthorn3 profiles269 · h 100
- Q. Parker2 profiles146 · h 52
- A. Hopkins2 profiles140 · h 66
- S. Brough129 · h 65
- S. Croom127 · h 55
- M. Colless2 profiles92 · h 70
- K. Glazebrook85 · h 106
- M. Owers85 · h 54
- S. Driver85 · h 94
- J. Lawrence2 profiles77 · h 40
- C. Tinney76 · h 60
- Á. López-Sánchez2 profiles70 · h 68
- Macquarie UniversityAU873 papers
- The University of SydneyAU617 papers
- Australian National UniversityAU525 papers
- Centre National de la Recherche ScientifiqueFR516 papers
- University of CambridgeGB449 papers
- University College LondonGB423 papers
- Swinburne University of TechnologyAU371 papers
- University of SussexGB345 papers
- University of PortsmouthGB331 papers
- University of ChicagoUS328 papers
- University of MichiganUS327 papers
- Centro de Investigaciones Energéticas, Medioambientales y TecnológicasES324 papers
59 papers · 2 filters
The 6dF Galaxy Survey: Dependence of halo occupation on stellar mass
Florian Beutler, Chris Blake, Matthew Colless +6
In this paper we study the stellar-mass dependence of galaxy clustering in the 6dF Galaxy Survey. The near-infrared selection of 6dFGS allows more reliable stellar mass estimates c…
MegaMorph - multi-wavelength measurement of galaxy structure: complete Sérsic profile information from modern surveys
Boris Häußler, Steven P. Bamford, Marina Vika +13
In this paper, we demonstrate a new method for fitting galaxy profiles which makes use of the full multi-wavelength data provided by modern large optical-near-infrared imaging surv…
The 2MASS Tully-Fisher Survey : Mapping the Mass in the Universe
T. Hong, L. Staveley-Smith, K. Masters +5
The 2MASS Tully-Fisher Survey (2MTF) aims to measure Tully-Fisher (TF) distances for all bright inclined spirals in the 2MASS Redshift Survey (2MRS) using high quality HI widths an…
Herschel-ATLAS/GAMA: a difference between star-formation rates in strong-line and weak-line radio galaxies
M. J. Hardcastle, J. H. Y. Ching, J. S. Virdee +25
We have constructed a sample of radio-loud objects with optical spectroscopy from the Galaxy and Mass Assembly (GAMA) project over the Herschel-ATLAS Phase 1 fields. Classifying th…
Measuring H0 from the 6dF Galaxy Survey and future low-redshift surveys
Matthew Colless, Florian Beutler, Chris Blake
Baryon acoustic oscillations (BAO) at low redshift provide a precise and largely model-independent way to measure the Hubble constant, H0. The 6dF Galaxy Survey measurement of the…
The WiggleZ Dark Energy Survey: Probing the Epoch of Radiation Domination using Large Scale Structure
Gregory B. Poole, Chris Blake, David Parkinson +24
We place the most robust constraint to date on the scale of the turnover in the cosmological matter power spectrum using data from the WiggleZ Dark Energy Survey. We find this feat…
Photometric Constraints on the Redshift of z~10 candidate UDFj-39546284 from deeper WFC3/IR+ACS+IRAC observations over the HUDF
R. J. Bouwens, P. A. Oesch, G. D. Illingworth +10
Ultra-deep WFC3/IR observations on the HUDF from the HUDF09 program revealed just one plausible z~10 candidate UDFj-39546284. UDFj-39546284 had all the properties expected of a gal…
Radio Continuum Surveys with Square Kilometre Array Pathfinders
Ray P. Norris, J. Afonso, D. Bacon +48
In the lead-up to the Square Kilometre Array (SKA) project, several next-generation radio telescopes and upgrades are already being built around the world. These include APERTIF (T…
Extending the Nearby Galaxy Heritage with WISE: First Results from the WISE Enhanced Resolution Galaxy Atlas
T. H. Jarrett, F. Masci, C. W. Tsai +15
The Wide-field Infrared Survey Explorer (WISE) mapped the entire sky at mid-infrared wavelengths 3.4, 4.6, 12 and 22 microns. The mission was primarily designed to extract point so…
Status of the OTELO Project
J. Cepa, A. Bongiovanni, A. M. Perez Garcia +10
The OTELO project is the extragalactic survey currently under way using the tunable filters of the OSIRIS instrument at the GTC. OTELO is already providing the deepest emission lin…
Spectral properties of the narrow-line region in Seyfert galaxies selected from the SDSS-DR7
L. Vaona, S. Ciroi, F. Di Mille +3
Although the properties of the narrow-line region (NLR) of active galactic nuclei(AGN) have been deeply studied by many authors in the past three decades, many questions are still…
Galaxy And Mass Assembly (GAMA): The M-Z relation for galaxy groups
M. A. Lara-Lopez, A. M. Hopkins, A. Robotham +7
The stellar mass and metallicity are among the fundamental parameters of galaxies. An understanding of the interplay between those properties as well as their environmental depende…
The WiggleZ Dark Energy Survey: Final data release and cosmological results
David Parkinson, Signe Riemer-Sørensen, Chris Blake +25
This paper presents cosmological results from the final data release of the WiggleZ Dark Energy Survey. We perform full analyses of different cosmological models using the WiggleZ…
CALIFA, the Calar Alto Legacy Integral Field Area survey. II. First public data release
CALIFA collaboration, B. Husemann, K. Jahnke +74
We present the first public data release of the CALIFA survey. It consists of science-grade optical datacubes for the first 100 of eventually 600 nearby (0.005<z<0.03) galaxies, ob…
A Bayesian Approach to Locating the Red Giant Branch Tip Magnitude (Part II); Distances to the Satellites of M31
Anthony R. Conn, Rodrigo A. Ibata, Geraint F. Lewis +10
In `A Bayesian Approach to Locating the Red Giant Branch Tip Magnitude (PART I),' a new technique was introduced for obtaining distances using the TRGB standard candle. Here we des…
Herschel-ATLAS/GAMA: spatial clustering of low-redshift sub-mm galaxies
E. van Kampen, D. J. B. Smith, S. Maddox +44
We have measured the clustering properties of low-redshift (z < 0.3) sub-mm galaxies detected at 250 micron in the Herschel-ATLAS Science Demonstration Phase (SDP) field. We select…
The Dark Energy Spectrometer (DESpec): A Multi-Fiber Spectroscopic Upgrade of the Dark Energy Camera and Survey for the Blanco Telescope
F. Abdalla, J. Annis, D. Bacon +29
We describe an initiative to build and use the Dark Energy Spectrometer (DESpec), a wide-field spectroscopic survey instrument for the Blanco 4 meter telescope at Cerro Tololo Inte…
Galaxy And Mass Assembly (GAMA): The mass-metallicity relationship
C. Foster, A. M. Hopkins, M. Gunawardhana +37
Context: The mass-metallicity relationship (MMR) of star-forming galaxies is well-established, however there is still some disagreement with respect to its exact shape and its poss…
An Early & Comprehensive Millimeter and Centimeter Wave and X-ray Study of Supernova 2011dh: A Non-Equipartition Blastwave Expanding into A Massive Stellar Wind
Assaf Horesh, Christopher Stockdale, Derek B. Fox +24
Only a handful of supernovae (SNe) have been studied in multi-wavelength from radio to X-rays, starting a few days after explosion. The early detection and classification of the ne…
Galaxy And Mass Assembly (GAMA): The 0.013 < z < 0.1 cosmic spectral energy distribution from 0.1 micron to 1mm
S. P. Driver, A. S. G. Robotham, L. Kelvin +40
We use the GAMA I dataset combined with GALEX, SDSS and UKIDSS imaging to construct the low-redshift (z<0.1) galaxy luminosity functions in FUV, NUV, ugriz, and YJHK bands from wit…
The ATLAS 5.5 GHz survey of the Extended Chandra Deep Field South: Catalogue, Source Counts and Spectral Indices
M. T. Huynh, A. M. Hopkins, E. Lenc +4
Star forming galaxies are thought to dominate the sub-mJy radio population, but recent work has shown that low luminosity AGN can still make a significant contribution to the faint…
Evidence for Significant Growth in the Stellar Mass of Brightest Cluster Galaxies over the Past 10 Billion Years
C. Lidman, J. Suherli, A. Muzzin +17
Using new and published data, we construct a sample of 160 brightest cluster galaxies (BCGs) spanning the redshift interval 0.03 < z < 1.63. We use this sample, which covers 70% of…
Galaxy And Mass Assembly (GAMA): In Search of Milky-Way Magellanic Cloud Analogues
A. S. G. Robotham, I. K. Baldry, J. Bland-Hawthorn +13
Analysing all Galaxy and Mass Assembly (GAMA) galaxies within a factor two (+/- 0.3 dex) of the stellar mass of the Milky Way (MW), there is a 11.9% chance that one of these galaxi…
The Australia Telescope Large Area Survey: Spectroscopic Catalogue and Radio Luminosity Functions
Minnie Y. Mao, Rob Sharp, Ray P. Norris +9
The Australia Telescope Large Area Survey (ATLAS) has surveyed seven square degrees of sky around the Chandra Deep Field South (CDFS) and the European Large Area ISO Survey - South…