- The University of SydneyAU578 papers
- Australian National UniversityAU542 papers
- Commonwealth Scientific and Industrial Research OrganisationAU328 papers
- Centre National de la Recherche ScientifiqueFR319 papers
- Macquarie UniversityAU309 papers
- Data61AU267 papers
- University of CambridgeGB253 papers
- Australian Astronomical ObservatoryAU246 papers
- Centre for Quantum Computation and Communication TechnologyAU243 papers
- Australian Defence Force AcademyAU233 papers
- ARC Centre of Excellence for All-sky AstrophysicsAU232 papers
- Swinburne University of TechnologyAU209 papers
14 papers · 2 filters
Cosmic Microwave Background Observations: Implications for Hubble's Constant and the Spectral Parameters $\n$ and in Cold Dark Matter Critical Density Universes
Charles H. Lineweaver, Domingos Barbosa
Recent cosmic microwave background (CMB) measurements over a large range of angular scales have become sensitive enough to provide interesting constraints on cosmological parameter…
Are the Perseus-Pisces chain and the Pavo-Indus wall connected?
Helene Di Nella, W. Couch, G. Paturel +1
A significant empty region was found between the southern Pavo- Indus (PI) wall and the northern Perseus-Pisces (PP) chain. This survey tests the reality of this void which may sim…
A Catalog of Morphological Types in 10 Distant Rich Clusters of Galaxies
Ian Smail, Alan Dressler, Warrick J. Couch +4
We present catalogs of objects detected in deep images of 11 fields in 10 distant clusters obtained using WFPC-2 on board the Hubble Space Telescope. The clusters span the redshift…
A Comparison of Direct and Indirect Mass Estimates for Distant Clusters of Galaxies
Ian Smail, Richard S. Ellis, Alan Dressler +4
We present weak lensing results for 12 distant clusters determined from images obtained with the refurbished HST. We detect the signature of gravitational lensing in 11 of the 12 c…
The Faint End of the Galaxy Luminosity Function In Moderate Redshift Clusters
Gillian Wilson, Ian Smail, Richard S. Ellis +1
We present deep two-colour photometry of two rich clusters at z=0.18, A665 and A1689. We use these data to construct number counts as a function of magnitude in the two fields. By…
Measurements of the Cosmological Parameters Omega and Lambda from the First 7 Supernovae at z >= 0.35
S. Perlmutter, S. Gabi, G. Goldhaber +21
We have developed a technique to systematically discover and study high-redshift supernovae that can be used to measure the cosmological parameters. We report here results based on…