activity
19972026
most citedThe 2dF Galaxy Redshift Survey: Spectra and redshifts

2.4k citations · 44.2k across the 466 of their papers we have counts for

collaborators
Showing 2013Show all

26 papers · 1 filter

astro-ph.IM2013★ 132 cited

Focal ratio degradation in lightly-fused hexabundles

Julia Bryant, Joss Bland-Hawthorn, Lisa Fogarty +2

We are now moving into an era where multi-object wide-field surveys, which traditionally use single fibres to observe many targets simultaneously, can exploit compact integral fiel…

astro-ph.CO2013★ 122 cited

Galaxy And Mass Assembly (GAMA): The large scale structure of galaxies and comparison to mock universes

Mehmet Alpaslan, Aaron S. G. Robotham, Simon Driver +18

From a volume limited sample of 45,542 galaxies and 6,000 groups with we use an adapted minimal spanning tree algorithm to identify and classify large scale structur…

astro-ph.IM2013★ 35 cited

Beating the classical limit: A diffraction-limited spectrograph for an arbitrary input beam

Christopher H. Betters, Sergio G. Leon-Saval, J. Gordon Robertson +1

We demonstrate a new approach to classical fiber-fed spectroscopy. Our method is to use a photonic lantern that converts an arbitrary (e.g. incoherent) input beam into N diffractio…

astro-ph.CO2013★ 243 cited

Galaxy And Mass Assembly (GAMA): improved cosmic growth measurements using multiple tracers of large-scale structure

Chris Blake, Ivan K. Baldry, Joss Bland-Hawthorn +11

We present the first application of a "multiple-tracer" redshift-space distortion (RSD) analysis to an observational galaxy sample, using data from the Galaxy and Mass Assembly sur…

astro-ph.GA2013★ 90 cited

Fossil imprint of a powerful flare at the Galactic Centre along the Magellanic Stream

Joss Bland-Hawthorn, Phil Maloney, Ralph Sutherland +1

The Fermi satellite discovery of the gamma-ray emitting bubbles extending 50 deg (10 kpc) from the Galactic Centre has revitalized earlier claims that our Galaxy has undergone an e…

astro-ph.SR2013★ 38 cited

A RAVE Investigation on Galactic open Clusters I. Radial velocities and metallicities

C. Conrad, R. -D. Scholz, N. V. Kharchenko +25

Context. Galactic open clusters (OCs) mainly belong to the young stellar population in the Milky Way disk, but are there groups and complexes of OCs that possibly define an additio…

astro-ph.GA2013★ 387 cited

The RAdial Velocity Experiment (RAVE): Fourth data release

G. Kordopatis, G. Gilmore, M. Steinmetz +48

We present the stellar atmospheric parameters (effective temperature, surface gravity, overall metallicity), radial velocities, individual abundances and distances determined for 4…

astro-ph.SR2013★ 33 cited

Chromospherically Active Stars in the RAVE Survey. I. The Catalogue

M. Žerjal, T. Zwitter, G. Matijevič +15

RAVE, the unbiased magnitude limited survey of the southern sky stars, contained 456,676 medium-resolution spectra at the time of our analysis. Spectra cover the CaII IRT range whi…

astro-ph.GA2013★ 90 cited

Galactic kinematics and dynamics from RAVE stars

James Binney, Ben Burnett, Georges Kordopatis +15

We analyse the kinematics of ~400000 RAVE stars. We split the sample into hot and cold dwarfs, red-clump and non-clump giants. The kinematics of the clump giants are consistent wit…

astro-ph.GA2013★ 135 cited

Constraints on the Galactic Bar from the Hercules stream as traced with RAVE across the Galaxy

T. Antoja, A. Helmi, W. Dehnen +20

Non-axisymmetries in the Galactic potential (spiral arms and bar) induce kinematic groups such as the Hercules stream. Assuming that Hercules is caused by the effects of the Outer…

astro-ph.GA2013★ 107 cited

New distances to RAVE stars

James Binney, Ben Burnett, Georges Kordopatis +16

Probability density functions are determined from new stellar parameters for the distance moduli of stars for which the RAdial Velocity Experiment (RAVE) has obtained spectra with…

astro-ph.GA2013★ 10 cited

The Epoch of Assembly of Two Galaxy Groups: A comparative study

Matthew Nichols, Joss Bland-Hawthorn

Nearby galaxy groups of comparable mass to the Local Group show global variations that reflect differences in their evolutionary history. Satellite galaxies in groups have higher l…

astro-ph.GA2013★ 38 cited

The asymmetric drift, the local standard of rest, and implications from RAVE data

O. Golubov, A. Just, O. Bienaymé +13

The determination of the LSR is still a matter of debate. The classical value of the tangential peculiar motion of the Sun with respect to the LSR was challenged in recent years, c…

astro-ph.GA2013★ 12 cited

An empirical formula for the distribution function of a thin exponential disc

Sanjib Sharma, Joss Bland-Hawthorn

An empirical formula for a Shu distribution function that reproduces a thin disc with exponential surface density to good accuracy is presented. The formula has two free parameters…

astro-ph.CO2013★ 46 cited

Galaxy and Mass Assembly (GAMA): galaxy radial alignments in GAMA groups

Michael D. Schneider, Shaun Cole, Carlos S. Frenk +10

We constrain the distributions of projected radial alignment angles of satellite galaxy shapes within the Galaxy And Mass Assembly survey group catalogue. We identify the galaxy gr…

astro-ph.CO2013★ 104 cited

Galaxy And Mass Assembly (GAMA): Linking Star Formation Histories and Stellar Mass Growth

Amanda E. Bauer, A. M. Hopkins, M. Gunawardhana +23

We present evidence for stochastic star formation histories in low-mass (M* < 10^10 Msun) galaxies from observations within the Galaxy And Mass Assembly (GAMA) survey. For ~73,000…

astro-ph.CO2013★ 10 cited

Choirs, HI Galaxy Groups: Catalogue and Detection of Star-forming Dwarf Group Members

Sarah M. Sweet, Gerhardt Meurer, Michael J. Drinkwater +24

Hα observations centred on galaxies selected from the HI Parkes All Sky Survey (HIPASS, Barnes et al. 2001) typically show one and sometimes two star-forming galaxies within the ap…

astro-ph.GA2013★ 83 cited

The COS/UVES Absorption Survey of the Magellanic Stream: I. One-Tenth Solar Abundances along the Body of the Stream

Andrew J. Fox, Philipp Richter, Bart P. Wakker +5

The Magellanic Stream (MS) is a massive and extended tail of multi-phase gas stripped out of the Magellanic Clouds and interacting with the Galactic halo. In this first paper of an…

astro-ph.GA2013★ 86 cited

The COS/UVES Absorption Survey of the Magellanic Stream: II. Evidence for a complex enrichment history of the Stream from the Fairall 9 sightline

Philipp Richter, Andrew J. Fox, Bart P. Wakker +5

We present a multi-wavelength study of the Magellanic Stream (MS), a massive gaseous structure in the Local Group that is believed to represent material stripped from the Magellani…

astro-ph.GA2013★ 58 cited

The relation between chemical abundances and kinematics of the Galactic disc with RAVE

C. Boeche, C. Chiappini, I. Minchev +20

Aims: We study the relations between stellar kinematics and chemical abundances of a large sample of RAVE giants in search for selection criteria needed for disentangling different…

astro-ph.GA2013★ 275 cited

The wobbly Galaxy: kinematics north and south with RAVE red clump giants

M. E. K. Williams, M. Steinmetz, J. Binney +23

The RAVE survey, combined with proper motions and distance estimates, can be used to study in detail stellar kinematics in the extended solar neighbourhood (solar suburb). Using th…

astro-ph.CO2013★ 55 cited

Galaxy And Mass Assembly (GAMA): The Life and Times of L* Galaxies

A. S. G. Robotham, J. Liske, S. P. Driver +18

In this work we investigate in detail the effects local environment (groups and pairs) has on galaxies with stellar mass similar to the Milky-Way (L* galaxies). A volume limited sa…

astro-ph.CO2013★ 198 cited

Galaxy And Mass Assembly (GAMA): Spectroscopic analysis

A. M. Hopkins, S. P. Driver, S. Brough +79

The Galaxy And Mass Assembly (GAMA) survey is a multiwavelength photometric and spectroscopic survey, using the AAOmega spectrograph on the Anglo-Australian Telescope to obtain spe…

astro-ph.IM2013★ 15 cited

PRAXIS: a low background NIR spectrograph for fibre Bragg grating OH suppression

Anthony Horton, Simon Ellis, Jon Lawrence +1

Fibre Bragg grating (FBG) OH suppression is capable of greatly reducing the bright sky background seen by near infrared spectrographs. By filtering out the airglow emission lines a…