J
Joss Bland-Hawthorn
Researcher at University of Sydney
Publications - 1157
Citations - 84957
Joss Bland-Hawthorn is an academic researcher from University of Sydney. The author has contributed to research in topics: Galaxy & Stars. The author has an hindex of 136, co-authored 1114 publications receiving 77593 citations. Previous affiliations of Joss Bland-Hawthorn include Macquarie University & Australian National University.
Papers
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Proceedings ArticleDOI
GNOSIS: an OH suppression unit for near-infrared spectrographs
Simon Ellis,Joss Bland-Hawthorn,Jon Lawrence,Julia J. Bryant,Roger Haynes,Anthony Horton,Steve Lee,Sergio G. Leon-Saval,Hans Gerd Löhmannsröben,J. Mladenoff,John O'Byrne,William Rambold,Markus Roth,Christopher Q. Trinh +13 more
TL;DR: GNOSIS as mentioned in this paper is an OH suppression unit to be used in conjunction with existing spectrographs, achieved using fibre Bragg gratings (FBGs), and will deliver the darkest near-infrared background of any ground-based instrument.
Journal ArticleDOI
Galaxy and Mass Assembly (GAMA) : small-scale anisotropic galaxy clustering and the pairwise velocity dispersion of galaxies.
Jon Loveday,L. Christodoulou,Peder Norberg,John A. Peacock,Ivan K. Baldry,Joss Bland-Hawthorn,Michael J. I. Brown,Matthew Colless,Simon P. Driver,Simon P. Driver,Benne W. Holwerda,Andrew M. Hopkins,Prajwal R. Kafle,Jochen Liske,Angel R. Lopez-Sanchez,Angel R. Lopez-Sanchez,Edward N. Taylor +16 more
TL;DR: In this paper, the authors measured the PVD of galaxies in the Galaxy and Mass Assembly (GAMA) survey as a function of projected separation and galaxy luminosity and showed that the measured PVD at projected separations increases near-monotonically with increasing luminosity.
Journal ArticleDOI
OAM interferometry: the detection of the rotational Doppler shift.
TL;DR: It is demonstrated that an OAM interferometer capable of extracting the rotational Doppler shift from OAM correlations can be constructed from a standard OAM modesorter combined with a phase filter.
Journal ArticleDOI
Correlations between age, kinematics, and chemistry as seen by the RAVE survey
Jennifer Wojno,Jennifer Wojno,Georges Kordopatis,Matthias Steinmetz,Paul J. McMillan,James Binney,Benoit Famaey,Giacomo Monari,Ivan Minchev,Rosemary F. G. Wyse,Teresa Antoja,Arnaud Siebert,I. Carrillo,Joss Bland-Hawthorn,Eva K. Grebel,Tomaž Zwitter,Olivier Bienaymé,Brad K. Gibson,Andrea Kunder,Ulisse Munari,Julio F. Navarro,Quentin A. Parker,Warren A. Reid,Warren A. Reid,George M. Seabroke +24 more
TL;DR: In this paper, the authors explore the connections between stellar age, chemistry, and kinematics across a Galactocentric distance of 7.5 < R(kpc) < 9.0, using a sample of ∼12,000 intermediate-mass (FGK) turn-off stars observed with the RAdial Velocity Experiment (RAVE) survey.
Journal ArticleDOI
Galaxy and Mass Assembly: the evolution of the cosmic spectral energy distribution from z = 1 to z = 0
Stephen K. Andrews,Simon P. Driver,Simon P. Driver,Luke J. M. Davies,Prajwal R. Kafle,Aaron S. G. Robotham,Kevin Vinsen,A. H. Wright,A. H. Wright,Joss Bland-Hawthorn,Nathan Bourne,Malcolm N. Bremer,E. da Cunha,Michael J. Drinkwater,Benne W. Holwerda,Andrew M. Hopkins,Lee S. Kelvin,Jon Loveday,Steven Phillipps,S. Wilkins +19 more
TL;DR: In this article, the evolution of the cosmic spectral energy distribution (CSED) from z = 1 to 0 has been studied using panchromatic photometry from the Galaxy And Mass Assembly (GAMA) and COSMOS data sets in 10 redshift intervals with completeness corrections applied Below z = 045, we have credible SED fits from 100 nm to 1 mm.