Lahav, Ofer, Kiakotou, Angeliki, Abdalla, Filipe B., Blake, Chris
We study the prospects for detecting neutrino masses from the galaxy angular power spectrum in photometric redshift shells of the Dark Energy Survey (DES) over a volume of 20 (Gpc/h)^3 combined with...
Forecasts for Dark Energy Measurements with Future HI Surveys (2009)
Abdalla, Filipe B., Blake, Chris, Rawlings, Steve
We use two independent methods to forecast the dark energy measurements achievable by combining future galaxy redshift surveys based on the radio HI emission line with Cosmic Microwave Background...
The WiggleZ Dark Energy Survey: small-scale clustering of Lyman-break galaxies at z < 1 (2009)
Blake, Chris, Jurek, Russell J., Brough, Sarah, Colless, Matthew, Couch, Warrick, Croom, Scott, ...
The WiggleZ Dark Energy Survey is a large-scale structure survey of intermediate-redshift ultraviolet-selected (UV-selected) emission-line galaxies scheduled to cover 1000 deg^2, spanning a broad...
The Billion Galaxy Cosmological HI Large Deep Survey (2009)
Myers, Steven T., Abdalla, Filipe B., Blake, Chris, Koopmans, Leon, Lazio, Joseph, Rawlings, Steve
We outline the case for a comprehensive wide and deep survey ultimately targeted at obtaining 21-cm HI line emission spectroscopic observations of more than a billion galaxies to redshift z=1.5 and...
The WiggleZ Dark Energy Survey: small-scale clustering of Lyman Break Galaxies at z < 1 (2009)
Blake, Chris, Jurek, Russell, Brough, Sarah, Colless, Matthew, Couch, Warrick, Croom, Scott, ...
The WiggleZ Dark Energy Survey is a large-scale structure survey of intermediate-redshift UV-selected emission-line galaxies scheduled to cover 1000 sq deg, spanning a broad redshift range 0.2 < z <...
The WiggleZ Dark Energy Survey: small-scale clustering of Lyman-break galaxies at z < 1 (2009)
Blake, Chris, Jurek, Russell, Brough, Sarah, Colless, Matthew, Couch, Warrick, Croom, Scott M., ...
The WiggleZ Dark Energy Survey is a large-scale structure survey of intermediate-redshift ultraviolet-selected (UV-selected) emission-line galaxies scheduled to cover 1000 deg2, spanning a broad...
The 'billion galaxy' cosmological HI Large Deep Survey (BiG-CHILDS) (2009)
Myers, Steven T., Abdalla, Filipe B., Blake, Chris, Koopmans, Leon, Lazio, Joseph, Rawlings, Steve
We outline the case for a comprehensive wide and deep survey ultimately targeted at obtaining 21-cm HI line emission spectroscopic observations of more than a billion galaxies to redshift z > 1.5...
Abstract not available.
The kinematics and spatial distribution of stellar populations in E plus A galaxies (2009)
Pracy, Michael B., Kuntschner, Harald, Couch, Warrick J., Blake, Chris, Bekki, Kenji, Briggs, F. H.
We have used the Gemini Multi-Object Spectragraph (GMOS) instrument on the 8.1-m Gemini-South Telescope to obtain spatially resolved two-colour imaging and integral field unit (IFU) spectroscopy of a...
The WiggleZ Dark Energy Survey: small-scale clustering of Lyman-break galaxies at z < 1 (2009)
Blake, Chris, Jurek, Russell, Brough, Sarah, Colless, Matthew, Couch, Warrick, Croom, Scott M., ...
The WiggleZ Dark Energy Survey is a large-scale structure survey of intermediate-redshift ultraviolet-selected (UV-selected) emission-line galaxies scheduled to cover 1000 deg2, spanning a broad...
The 'billion galaxy' cosmological HI Large Deep Survey (BiG-CHILDS) (2009)
Myers, Steven T., Abdalla, Filipe B., Blake, Chris, Koopmans, Leon, Lazio, Joseph, Rawlings, Steve
We outline the case for a comprehensive wide and deep survey ultimately targeted at obtaining 21-cm HI line emission spectroscopic observations of more than a billion galaxies to redshift z > 1.5...
Abstract not available.
The kinematics and spatial distribution of stellar populations in E plus A galaxies (2009)
Pracy, Michael B., Kuntschner, Harald, Couch, Warrick J., Blake, Chris, Bekki, Kenji, Briggs, F. H.
We have used the Gemini Multi-Object Spectragraph (GMOS) instrument on the 8.1-m Gemini-South Telescope to obtain spatially resolved two-colour imaging and integral field unit (IFU) spectroscopy of a...
The WiggleZ dark energy survey (2008)
Blake, Chris, Brough, Sarah, Couch, Warrick, Glazebrook, Karl, Poole, Greg, Davis, Tamara, ...
The accelerating expansion of the universe, attributed to "dark energy", has no accepted theoretical explanation. The origin of this phenomenon unambiguously implicates new physics via a novel form...
Science with ASKAP: the Australian square-kilometre-array pathfinder (2008)
Johnston, Simon, Bailes, Matthew, Bartel, Norbert, Baugh, Carlton, Bietenholz, Michael F., Blake, Chris, ...
The future of cm and m-wave astronomy lies with the Square Kilometre Array (SKA), a telescope under development by a consortium of 17 countries. The SKA will be 50 times more sensitive than any...
Science with ASKAP: the Australian square-kilometre-array pathfinder (2008)
Johnston, Simon, Bailes, Matthew, Bartel, Norbert, Baugh, Carlton, Bietenholz, Michael F., Blake, Chris, ...
The future of cm and m-wave astronomy lies with the Square Kilometre Array (SKA), a telescope under development by a consortium of 17 countries. The SKA will be 50 times more sensitive than any...
The WiggleZ dark energy survey (2008)
Blake, Chris, Brough, Sarah, Couch, Warrick J., Glazebrook, Karl, Poole, Greg, Davis, Tamara M., ...
The accelerating expansion of the universe, attributed to 'dark energy', has no accepted theoretical explanation. The origin of this phenomenon unambiguously implicates new physics via a novel form...
Blake, Chris, Collister, Adrian, Lahav, Ofer
We analyse the small-scale clustering in 'MegaZ-LRG', a large photometric redshift catalogue of luminous red galaxies extracted from the imaging data set of the Sloan Digital Sky Survey. MegaZ-LRG,...
The WiggleZ dark energy survey (2008)
Blake, Chris, Brough, Sarah, Couch, Warrick, Glazebrook, Karl, Poole, Greg, Davis, Tamara, ...
The accelerating expansion of the universe, attributed to "dark energy", has no accepted theoretical explanation. The origin of this phenomenon unambiguously implicates new physics via a novel form...
Science with ASKAP: the Australian square-kilometre-array pathfinder (2008)
Johnston, Simon, Bailes, Matthew, Bartel, Norbert, Baugh, Carlton, Bietenholz, Michael F., Blake, Chris, ...
The future of cm and m-wave astronomy lies with the Square Kilometre Array (SKA), a telescope under development by a consortium of 17 countries. The SKA will be 50 times more sensitive than any...
The WiggleZ dark energy survey (2008)
Blake, Chris, Brough, Sarah, Couch, Warrick J., Glazebrook, Karl, Poole, Gregory B., Davis, Tamara M., ...
The accelerating expansion of the universe, attributed to 'dark energy', has no accepted theoretical explanation. The origin of this phenomenon unambiguously implicates new physics via a novel form...
Blake, Chris, Collister, Adrian, Lahav, Ofer
We analyse the small-scale clustering in 'MegaZ-LRG', a large photometric redshift catalogue of luminous red galaxies extracted from the imaging data set of the Sloan Digital Sky Survey. MegaZ-LRG,...
The environments and clustering properties of 2dFGRS-selected starburst galaxies (2007)
Owers, Matt, Blake, Chris, Couch, Warrick, Pracy, Mike, Bekki, Kenji
We investigate the environments and clustering properties of starburst galaxies selected from the 2dF Galaxy Redshift Survey (2dFGRS) in order to determine which, if any, environmental factors play a...
Halo-model signatures from 380,000 SDSS Luminous Red Galaxies with photometric redshifts (2007)
Blake, Chris, Collister, Adrian, Lahav, Ofer
We analyze the small-scale clustering in "MegaZ-LRG", a large photometric-redshift catalogue of Luminous Red Galaxies extracted from the imaging dataset of the Sloan Digital Sky Survey. MegaZ-LRG,...
Optimising Baryon Acoustic Oscillation Surveys - I: Testing the concordance LCDM cosmology (2007)
Parkinson, David, Blake, Chris, Kunz, Martin, Bassett, Bruce A., Nichol, Robert C., Glazebrook, Karl
We optimize the design of future spectroscopic redshift surveys for constraining the dark energy via precision measurements of the baryon acoustic oscillations (BAO), with particular emphasis on the...
The WiggleZ project: AAOmega and Dark Energy (2007)
Glazebrook, Karl, Blake, Chris, Couch, Warrick, Forbes, Duncan, Drinkwater, Michael, Jurek, Russell, ...
We describe the `WiggleZ' spectroscopic survey of 280,000 star-forming galaxies selected from a combination of GALEX ultra-violet and SDSS + RCS2 optical imaging. The fundamental goal is a detection...
Optimizing baryon acoustic oscillation surveys I: testing the concordance (2007)
Parkinson, David, Blake, Chris, Kunz, Martin, Bassett, Bruce A., Nichol, Robert C., Glazebrook, Karl
We optimize the design of future spectroscopic redshift surveys for constraining the dark energy via precision measurements of the baryon acoustic oscillations (BAOs), with particular emphasis on the...
MegaZ-LRG: a photometric redshift catalogue of one million SDSS luminous red galaxies (2007)
Collister, Adrian, Lahav, Ofer, Blake, Chris, Cannon, Russell D., Croom, Scott M., Drinkwater, Michael J., ...
We describe the construction of MegaZ-LRG, a photometric redshift catalogue of over one million luminous red galaxies (LRGs) in the redshift range 0.4 < z < 0.7 with limiting magnitude i < 20. The...
Blake, Chris, Collister, Adrian, Bridle, Sarah, Lahav, Ofer
We analyse MegaZ-LRG, a photometric-redshift catalogue of luminous red galaxies (LRGs) based on the imaging data of the Sloan Digital Sky Survey (SDSS) 4th Data Release. MegaZ-LRG, presented in a...
Parkinson, David, Blake, Chris, Kunz, Martin, Bassett, Bruce A., Nichol, Robert C., Glazebrook, Karl
We optimize the design of future spectroscopic redshift surveys for constraining the dark energy via precision measurements of the baryon acoustic oscillations (BAOs), with particular emphasis on the...
Parkinson, David, Blake, Chris, Kunz, Martin, Bassett, Bruce A., Nichol, Robert C., Glazebrook, Karl
We optimize the design of future spectroscopic redshift surveys for constraining the dark energy via precision measurements of the baryon acoustic oscillations (BAOs), with particular emphasis on the...
Science with the Australian Square Kilometre Array Pathfinder (2007)
Johnston, Simon, Bailes, Matthew, Bartel, Norbert, Baugh, Carlton, Bietenholz, Michael F., Blake, Chris, ...
The future of centimetre and metre-wave astronomy lies with the Square Kilometre Array (SKA), a telescope under development by a consortium of 17 countries that will be 50 times more sensitive than...
Science with the Australian Square Kilometre Array Pathfinder (2007)
Johnston, Simon, Bailes, Matthew, Bartel, Norbert, Baugh, Carlton, Bietenholz, Michael F., Blake, Chris, ...
The future of centimetre and metre-wave astronomy lies with the Square Kilometre Array (SKA), a telescope under development by a consortium of 17 countries that will be 50 times more sensitive than...
Parkinson, David, Blake, Chris, Kunz, Martin, Bassett, Bruce A., Nichol, Robert C., Glazebrook, Karl
We optimize the design of future spectroscopic redshift surveys for constraining the dark energy via precision measurements of the baryon acoustic oscillations (BAOs), with particular emphasis on the...
Science with the Australian Square Kilometre Array Pathfinder (2007)
Johnston, Simon, Bailes, Matthew, Bartel, Norbert, Baugh, Carlton, Bietenholz, Michael F., Blake, Chris, ...
The future of centimetre and metre-wave astronomy lies with the Square Kilometre Array (SKA), a telescope under development by a consortium of 17 countries that will be 50 times more sensitive than...
The WiggleZ Project: AAOmega and dark energy (2007)
Glazebrook, Karl, Blake, Chris, Couch, Warrick J., Forbes, Duncan A., Drinkwater, Michael J., Jurek, Russell, ...
We describe the 'WiggleZ' spectroscopic survey of 400,000 star-forming galaxies selected from a combination of GALEX ultra-violet and SDSS + RCS2 optical imaging. The fundamental goal is a detection...
Owers, Matthew S., Blake, Chris, Couch, Warrick J., Pracy, Michael B., Bekki, Kenji
We investigate the environments and clustering properties of starburst galaxies selected from the 2dF Galaxy Redshift Survey (2dFGRS) in order to determine which, if any, environmental factors play a...
Parkinson, David, Blake, Chris, Kunz, Martin, Bassett, Bruce A., Nichol, Robert C., Glazebrook, Karl
We optimize the design of future spectroscopic redshift surveys for constraining the dark energy via precision measurements of the baryon acoustic oscillations (BAOs), with particular emphasis on the...
Science with the Australian Square Kilometre Array Pathfinder (2007)
Johnston, Simon, Bailes, Matthew, Bartel, Norbert, Baugh, Carlton, Bietenholz, Michael F., Blake, Chris, ...
The future of centimetre and metre-wave astronomy lies with the Square Kilometre Array (SKA), a telescope under development by a consortium of 17 countries that will be 50 times more sensitive than...
Photometric and spectroscopic dissection of E A galaxies with GMOS (2007)
Couch, Warrick, Pracy, Michael, Blake, Chris, Bekki, Kenji, Kuntschner, Harald, Burgmann, Marcel, ...
The characteristic E A galaxy spectrum - strong Balmer-line absorption superimposed upon an elliptical galaxy spectrum - is a signpost to galaxies in the process of transformation. Such a spectrum...
The WiggleZ Project: AAOmega and dark energy (2007)
Glazebrook, Karl, Blake, Chris, Couch, Warrick J., Forbes, Duncan A., Drinkwater, Michael J., Jurek, Russell, ...
We describe the 'WiggleZ' spectroscopic survey of 400,000 star-forming galaxies selected from a combination of GALEX ultra-violet and SDSS + RCS2 optical imaging. The fundamental goal is a detection...
Blake, Chris, Collister, Adrian, Bridle, Sarah, Lahav, Ofer
We analyse MegaZ-LRG, a photometric-redshift catalogue of luminous red galaxies (LRGs) based on the imaging data of the Sloan Digital Sky Survey (SDSS) 4th Data Release. MegaZ-LRG, presented in a...
MegaZ-LRG: a photometric redshift catalogue of one million SDSS luminous red galaxies (2007)
Collister, Adrian, Lahav, Ofer, Blake, Chris, Cannon, Russell D., Croom, Scott M., Drinkwater, Michael J., ...
We describe the construction of MegaZ-LRG, a photometric redshift catalogue of over one million luminous red galaxies (LRGs) in the redshift range 0.4 < z < 0.7 with limiting magnitude i < 20. The...
Owers, Matthew S., Blake, Chris, Couch, Warrick J., Pracy, Michael B., Bekki, Kenji
We investigate the environments and clustering properties of starburst galaxies selected from the 2dF Galaxy Redshift Survey (2dFGRS) in order to determine which, if any, environmental factors play a...
Parkinson, David, Blake, Chris, Kunz, Martin, Bassett, Bruce A., Nichol, Robert C., Glazebrook, Karl
We optimize the design of future spectroscopic redshift surveys for constraining the dark energy via precision measurements of the baryon acoustic oscillations (BAOs), with particular emphasis on the...
Science with the Australian Square Kilometre Array Pathfinder (2007)
Johnston, Simon, Bailes, Matthew, Bartel, Norbert, Baugh, Carlton, Bietenholz, Michael F., Blake, Chris, ...
The future of centimetre and metre-wave astronomy lies with the Square Kilometre Array (SKA), a telescope under development by a consortium of 17 countries that will be 50 times more sensitive than...
Photometric and spectroscopic dissection of E A galaxies with GMOS (2007)
Couch, Warrick, Pracy, Michael, Blake, Chris, Bekki, Kenji, Kuntschner, Harald, Burgmann, Marcel, ...
The characteristic E A galaxy spectrum - strong Balmer-line absorption superimposed upon an elliptical galaxy spectrum - is a signpost to galaxies in the process of transformation. Such a spectrum...
MegaZ-LRG: A photometric redshift catalogue of one million SDSS Luminous Red Galaxies (2006)
Collister, Adrian, Lahav, Ofer, Blake, Chris, Cannon, Russell, Croom, Scott, Drinkwater, Michael, ...
We describe the construction of MegaZ-LRG, a photometric redshift catalogue of over one million luminous red galaxies (LRGs) in the redshift range 0.4 < z < 0.7 with limiting magnitude i < 20. The...
Blake, Chris, Collister, Adrian, Bridle, Sarah, Lahav, Ofer
We analyze MegaZ-LRG, a photometric-redshift catalogue of Luminous Red Galaxies (LRGs) based on the imaging data of the Sloan Digital Sky Survey (SDSS) 4th Data Release. MegaZ-LRG, presented in a...
On the cross-correlation of sub-mm sources and optically-selected galaxies (2006)
Blake, Chris, Pope, Alexandra, Scott, Douglas, Mobasher, Bahram
Bright sub-mm galaxies are expected to arise in massive highly-biased haloes, and hence exhibit strong clustering. We argue that a valuable tool for measuring these clustering properties is the...
The WiggleZ Dark Energy Survey: 1000 redshifts and beyond (2006)
Drinkwater, Michael J., Pimbblet, Kevin, Jurek, Russell, Blake, Chris, Glazebrook, Karl, Woods, David, ...
Here we outline design aspects and first results of the WiggleZ Dark Energy Survey that has recently been awarded long-term status on the AAT from the 2006B semester. The primary aim of the WiggleZ...
Curran, Stephen J., Whiting, Matthew T., Murphy, Michael T., Webb, J. K., Longmore, Steven N., Pihlstrom, Ylva M., ...
We are currently undertaking a large survey for redshifted atomic and molecular absorption lines at radio frequencies. In this paper, we present the results from the first phase of this survey: the...
Universal fitting formulae for baryon oscillation surveys (2006)
Blake, Chris, Parkinson, David, Bassett, Bruce A., Glazebrook, Karl, Kunz, Martin, Nichol, Robert C.
The next generation of galaxy surveys will attempt to measure the baryon oscillations in the clustering power spectrum with high accuracy. These oscillations encode a preferred scale which may be...
On the cross-correlation of sub-mm sources and optically selected galaxies (2006)
Blake, Chris, Pope, Alexandra, Scott, Douglas, Mobasher, Bahram
Bright submillimetre (sub-mm) galaxies are expected to arise in massive highly biased haloes, and hence exhibit strong clustering. We argue that a valuable tool for measuring these clustering...
Corasaniti, Pier Stefano, LoVerde, Marilena, Crotts, Arlin, Blake, Chris
The Advanced Liquid-mirror Probe of Asteroids, Cosmology and Astrophysics (ALPACA) is a proposed 8-m liquid-mirror telescope surveying of the Southern hemisphere sky. It will be a remarkably simple...
The WiggleZ Dark Energy Survey: 1000 redshifts and beyond (2006)
Drinkwater, Michael J., Pimbblet, Kevin, Jurek, Russell, Blake, Chris, Glazebrook, Karl, Woods, David, ...
Here we outline design aspects and first results of the WiggleZ Dark Energy Survey that has recently been awarded long-term status on the AAT from the 2006B semester. The primary aim of the WiggleZ...
Curran, Stephen J., Whiting, Matthew T., Murphy, Michael T., Webb, J. K., Longmore, Steven N., Pihlstrom, Ylva M., ...
We are currently undertaking a large survey for redshifted atomic and molecular absorption lines at radio frequencies. In this paper, we present the results from the first phase of this survey: the...
Universal fitting formulae for baryon oscillation surveys (2006)
Blake, Chris, Parkinson, David, Bassett, Bruce A., Glazebrook, Karl, Kunz, Martin, Nichol, Robert C.
The next generation of galaxy surveys will attempt to measure the baryon oscillations in the clustering power spectrum with high accuracy. These oscillations encode a preferred scale which may be...
On the cross-correlation of sub-mm sources and optically selected galaxies (2006)
Blake, Chris, Pope, Alexandra, Scott, Douglas, Mobasher, Bahram
Bright submillimetre (sub-mm) galaxies are expected to arise in massive highly biased haloes, and hence exhibit strong clustering. We argue that a valuable tool for measuring these clustering...
Corasaniti, Pier Stefano, LoVerde, Marilena, Crotts, Arlin, Blake, Chris
The Advanced Liquid-mirror Probe of Asteroids, Cosmology and Astrophysics (ALPACA) is a proposed 8-m liquid-mirror telescope surveying of the Southern hemisphere sky. It will be a remarkably simple...
Corasaniti, Pier Stefano, LoVerde, Marilena, Crotts, Arlin, Blake, Chris
The Advanced Liquid-Mirror Probe of Asteroids, Cosmology and Astrophysics (ALPACA) is a proposed 8-meter liquid mirror telescope surveying 1000 square degree of the southern-hemisphere sky. It will...
Universal fitting formulae for baryon oscillation surveys (2005)
Blake, Chris, Parkinson, David, Bassett, Bruce, Glazebrook, Karl, Kunz, Martin, Nichol, Robert C.
The next generation of galaxy surveys will attempt to measure the baryon oscillations in the clustering power spectrum with high accuracy. These oscillations encode a preferred scale which may be...
Crotts, Arlin, Garnavich, Peter, Priedhorsky, William, Habib, Salman, Heitmann, Katrin, Wang, Yun, ...
JEDI will probe dark energy in three independent ways by measuring the expansion history of the universe: (1) using type Ia supernovae as cosmological standard candles over a range of distances, (2)...
Glazebrook, Karl, Blake, Chris
We use Monte Carlo techniques to simulate the ability of future large high-redshift galaxy surveys to measure the temporal evolution of the dark energy equation-of-state w(z), using the baryonic...
Allen, Paul D., Moustakas, Leonidas A., Dalton, Gavin, MacDonald, Emily, Blake, Chris, Clewley, Lee, ...
We present measurements of the clustering properties of bright ($L>L_{*}$) z$\sim$4 Lyman Break Galaxies (LBGs) selected from the Oxford-Dartmouth Thirty Degree Survey (ODT). We describe techniques...
Allen, Paul D., Moustakas, Leonidas A., Dalton, Gavin, MacDonald, Emily, Blake, Chris, Clewley, Lee, ...
We present measurements of the clustering properties of bright (L > L*) z~ 4 Lyman break galaxies (LBGs) selected from the Oxford- Dartmouth Thirty Degree Survey (ODT). We describe techniques used to...
Galaxy groups: proceedings from a Swinburne University Workshop (2005)
Kilborn, Virginia A., Bekki, Kenji, Brough, Sarah, Doyle, Marianne T., Evstigneeva, Ekaterina A., Forbes, Duncan A., ...
We present the proceedings from a two-day workshop held at Swinburne University on 2005 May 24–25. The workshop participants highlighted current Australian research on both theoretical and...
Burton, Michael G., Lawrence, J. S., Ashley, M. C. B., Bailey, J. A., Blake, Chris, Bedding, T. R., ...
The cold, dry, and stable air above the summits of the Antarctic plateau provides the best ground-based observing conditions from optical to sub-millimetre wavelengths to be found on the Earth....
Glazebrook, Karl, Blake, Chris
We use Monte Carlo techniques to simulate the ability of future large high-redshift galaxy surveys to measure the temporal evolution of the dark energy equation of state ω(z) , using the...
Glazebrook, Karl, Blake, Chris
We use Monte Carlo techniques to simulate the ability of future large high-redshift galaxy surveys to measure the temporal evolution of the dark energy equation of state ω(z) , using the...
Cosmology with photometric redshift surveys (2005)
We explore the utility of future photometric redshift imaging surveys for delineating the large-scale structure of the Universe, and assess the resulting constraints on the cosmological model. We...
Spatially resolved spectroscopy of the E+A galaxies in the z = 0.32 cluster AC 114 (2005)
Pracy, Michael B., Couch, Warrick J., Blake, Chris, Bekki, Kenji, Harrison, Craig, Colless, Matthew, ...
We present spatially resolved intermediate-resolution spectroscopy of a sample of 12 E+A galaxies in the z= 0.32 rich galaxy cluster AC 114, obtained with the FLAMES multi-integral field unit system...
Allen, Paul D., Moustakas, Leonidas A., Dalton, Gavin, MacDonald, Emily, Blake, Chris, Clewley, Lee, ...
We present measurements of the clustering properties of bright (L > L*) z∼ 4 Lyman break galaxies (LBGs) selected from the Oxford–Dartmouth Thirty Degree Survey (ODT). We describe...
Burton, Michael G., Lawrence, J. S., Ashley, M. C. B., Bailey, J. A., Blake, Chris, Bedding, T. R., ...
The cold, dry, and stable air above the summits of the Antarctic plateau provides the best ground-based observing conditions from optical to sub-millimetre wavelengths to be found on the Earth....
Galaxy groups: proceedings from a Swinburne University workshop (2005)
Kilborn, Virginia A., Bekki, Kenji, Brough, Sarah, Doyle, Marianne T., Evstigneeva, Ekaterina A., Forbes, Duncan A., ...
We present the proceedings from a two-day workshop held at Swinburne University on 2005 May 24–25. The workshop participants highlighted current Australian research on both theoretical and...
Glazebrook, Karl, Blake, Chris
We use Monte Carlo techniques to simulate the ability of future large high-redshift galaxy surveys to measure the temporal evolution of the dark energy equation of state ω(z) , using the...
Cosmology with photometric redshift surveys (2005)
We explore the utility of future photometric redshift imaging surveys for delineating the large-scale structure of the Universe, and assess the resulting constraints on the cosmological model. We...
Spatially resolved spectroscopy of the E+A galaxies in the z = 0.32 cluster AC 114 (2005)
Pracy, Michael B., Couch, Warrick J., Blake, Chris, Bekki, Kenji, Harrison, Craig, Colless, Matthew, ...
We present spatially resolved intermediate-resolution spectroscopy of a sample of 12 E+A galaxies in the z= 0.32 rich galaxy cluster AC 114, obtained with the FLAMES multi-integral field unit system...
Allen, Paul D., Moustakas, Leonidas A., Dalton, Gavin, MacDonald, Emily, Blake, Chris, Clewley, Lee, ...
We present measurements of the clustering properties of bright (L > L*) z∼ 4 Lyman break galaxies (LBGs) selected from the Oxford–Dartmouth Thirty Degree Survey (ODT). We describe...
Cosmology with photometric redshift surveys (2004)
We explore the utility of future photometric redshift imaging surveys for delineating the large-scale structure of the Universe, and assess the resulting constraints on the cosmological model. We...
Cosmology with the Square Kilometre Array (2004)
Blake, Chris, Abdalla, Filipe, Bridle, Sarah, Rawlings, Steve
We argue that the Square Kilometre Array has the potential to make both redshift (HI) surveys and radio continuum surveys that will revolutionize cosmological studies, provided that it has sufficient...
The 2dF Galaxy Redshift Survey: the local E+A galaxy population (2004)
Blake, Chris, Pracy, Michael, Couch, Warrick, Bekki, Kenji, Lewis, Ian, Glazebrook, Karl, ...
We select a sample of low-redshift (z ~ 0.1) E+A galaxies from the 2dF Galaxy Redshift Survey (2dFGRS). The spectra of these objects are defined by strong hydrogen Balmer absorption lines (H-delta,...
MacDonald, Emily C., Allen, Paul, Dalton, Gavin, Moustakas, Leonidas A., Heymans, Catherine, Edmondson, Edward, ...
The Oxford Dartmouth Thirty Degree Survey (ODTS) is a deep, wide, multi-band imaging survey designed to cover a total of 30 square degrees in BVRi'Z, with a subset of U and K band data, in four...
The angular power spectrum of NVSS radio galaxies (2004)
Blake, Chris, Ferreira, Pedro G., Borrill, Julian
We measure the angular power spectrum of radio galaxies in the NRAO VLA Sky Survey (NVSS) using two independent methods: direct spherical harmonic analysis and maximum likelihood estimation. The...
The 2dF Galaxy Redshift Survey: the local E+A galaxy population (2004)
Blake, Chris, Pracy, Michael B., Couch, Warrick J., Bekki, Kenji, Lewis, Ian, Glazebrook, Karl, ...
We select a sample of low-redshift (z ∼ 0.1) E+A galaxies from the 2dF Galaxy Redshift Survey (2dFGRS). The spectra of these objects are defined by strong hydrogen Balmer absorption lines...
The angular power spectrum of NVSS radio galaxies (2004)
Blake, Chris, Ferreira, Pedro G., Borrill, Julian
We measure the angular power spectrum Cℓ of radio galaxies in the NRAO VLA Sky Survey (NVSS) using two independent methods: direct spherical harmonic analysis and maximum likelihood estimation...
MacDonald, Emily C., Allen, Paul, Dalton, Gavin, Moustakas, Leonidas A., Heymans, Catherine, Edmondson, Edward, ...
The Oxford-Dartmouth Thirty Degree Survey (ODTS) is a deep, wide, multiband imaging survey designed to cover a total of 30 deg2 in BVRi'Z, with a subset of U- and K-band data, in four separate fields...
Angular clustering in the Sydney University Molonglo Sky Survey (2004)
Blake, Chris, Mauch, Tom, Sadler, Elaine M.
We measure the angular correlation function of radio galaxies selected by the 843-MHz Sydney University Molonglo Sky Survey (SUMSS). We find that the characteristic imprint of large-scale structure...
The 2dF Galaxy Redshift Survey: the local E+A galaxy population (2004)
Blake, Chris, Pracy, Michael B., Couch, Warrick J., Bekki, Kenji, Lewis, Ian, Glazebrook, Karl, ...
We select a sample of low-redshift (z ∼ 0.1) E+A galaxies from the 2dF Galaxy Redshift Survey (2dFGRS). The spectra of these objects are defined by strong hydrogen Balmer absorption lines...
The angular power spectrum of NVSS radio galaxies (2004)
Blake, Chris, Ferreira, Pedro G., Borrill, Julian
We measure the angular power spectrum Cℓ of radio galaxies in the NRAO VLA Sky Survey (NVSS) using two independent methods: direct spherical harmonic analysis and maximum likelihood estimation...
MacDonald, Emily C., Allen, Paul, Dalton, Gavin, Moustakas, Leonidas A., Heymans, Catherine, Edmondson, Edward, ...
The Oxford-Dartmouth Thirty Degree Survey (ODTS) is a deep, wide, multiband imaging survey designed to cover a total of 30 deg2 in BVRi'Z, with a subset of U- and K-band data, in four separate fields...
Angular clustering in the Sydney University Molonglo Sky Survey (2004)
Blake, Chris, Mauch, Tom, Sadler, Elaine M.
We measure the angular correlation function of radio galaxies selected by the 843-MHz Sydney University Molonglo Sky Survey (SUMSS). We find that the characteristic imprint of large-scale structure...
Angular clustering in the SUMSS radio survey (2003)
Blake, Chris, Mauch, Tom, Sadler, Elaine M.
We measure the angular correlation function of radio galaxies selected by the 843 MHz Sydney University Molonglo Sky Survey (SUMSS). We find that the characteristic imprint of large-scale structure...
Blake, Chris, Glazebrook, Karl
We show that the baryonic oscillations expected in the galaxy power spectrum may be used as a "standard cosmological ruler'' to facilitate accurate measurement of the cosmological equation of state....
Blake, Chris, Glazebrook, Karl
We show that the baryonic oscillations expected in the galaxy power spectrum may be used as a "standard cosmological ruler" to facilitate accurate measurement of the cosmological equation of state....
Blake, Chris, Glazebrook, Karl
We show that the baryonic oscillations expected in the galaxy power spectrum may be used as a "standard cosmological ruler" to facilitate accurate measurement of the cosmological equation of state....
Quantifying angular clustering in wide-area radio surveys (2002)
We quantify the angular clustering of radio galaxies in the NVSS and FIRST radio surveys using the two-point correlation function and the moments of counts-in-cells - both important points of...
Detection of the velocity dipole in the radio galaxies of the NRAO VLA Sky Survey (2002)
We are in motion against the cosmic backdrop. This motion is evidenced by the systematic temperature shift - or dipole anisotropy - observed in the Cosmic Microwave Background radiation (CMB)....
Quantifying angular clustering in wide-area radio surveys (2002)
We quantify the angular clustering of radio galaxies in the NVSS and FIRST surveys using the two-point correlation function and the moments of counts-in-cells – both important points of...
Abstract not available.
Quantifying angular clustering in wide-area radio surveys (2002)
We quantify the angular clustering of radio galaxies in the NVSS and FIRST surveys using the two-point correlation function and the moments of counts-in-cells – both important points of...
Abstract not available.
A velocity dipole in the distribution of radio galaxies (2002)
The motion of our Galaxy through the Universe is reflected in a systematic shift in the temperature of the cosmic microwave background - because of the Doppler effect, the temperature of the...
We quantify the angular distribution of radio sources in the NVSS by measuring the two-point angular correlation function. By careful consideration of the resolution of radio galaxies into multiple...
Measurement of the star formation rate from Halpha in field galaxies at z=1 (1999)
Glazebrook, Karl, Blake, Chris, Economou, Frossie, Lilly, Simon, Colless, Matthew
We report the results of J-band infrared spectroscopy of a sample of 13 z=1 field galaxies drawn from the Canada-France Redshift Survey, targeting galaxies with redshifts that place the rest-frame...
Measurement of the star formation rate from Halpha in field galaxies at z=1 (1999)
Glazebrook, Karl, Blake, Chris, Economou, Frossie, Lilly, Simon, Colless, Matthew
We report the results of J-band infrared spectroscopy of a sample of 13 z=1 field galaxies drawn from the Canada-France Redshift Survey, targeting galaxies with redshifts that place the rest-frame...
Measurement of the star formation rate from Halpha in field galaxies at z=1 (1999)
Glazebrook, Karl, Blake, Chris, Economou, Frossie, Lilly, Simon, Colless, Matthew
We report the results of J-band infrared spectroscopy of a sample of 13 z=1 field galaxies drawn from the Canada-France Redshift Survey, targeting galaxies with redshifts that place the rest-frame...
Measurement of the star formation rate from Halpha in field galaxies at z=1 (1999)
Glazebrook, Karl, Blake, Chris, Economou, Frossie, Lilly, Simon, Colless, Matthew
We report the results of J-band infrared spectroscopy of a sample of 13 z=1 field galaxies drawn from the Canada-France Redshift Survey, targeting galaxies with redshifts that place the rest-frame...
Measurement of the star formation rate from Halpha in field galaxies at z=1 (1999)
Glazebrook, Karl, Blake, Chris, Economou, Frossie, Lilly, Simon, Colless, Matthew
We report the results of J-band infrared spectroscopy of a sample of 13 z=1 field galaxies drawn from the Canada-France Redshift Survey, targeting galaxies with redshifts that place the rest-frame...
Measurement of the star formation rate from H alpha in field galaxies at z=1 (1999)
Glazebrook, Karl, Blake, Chris, Economou, Frossie, Lilly, Simon J., Colless, Matthew
We report the results of J-band infrared spectroscopy of a sample of 13 z = 1 field galaxies drawn from the Canada-France Redshift Survey, targeting galaxies with redshifts that place the rest-frame...
Measurement of the star formation rate from H alpha in field galaxies at z=1 (1999)
Glazebrook, Karl, Blake, Chris, Economou, Frossie, Lilly, Simon J., Colless, Matthew
We report the results of J-band infrared spectroscopy of a sample of 13 z = 1 field galaxies drawn from the Canada-France Redshift Survey, targeting galaxies with redshifts that place the rest-frame...
Measurement of the star formation rate from Halpha in field galaxies at z=1 (1999)
Glazebrook, Karl, Blake, Chris, Economou, Frossie, Lilly, Simon, Colless, Matthew
We report the results of J-band infrared spectroscopy of a sample of 13 z=1 field galaxies drawn from the Canada-France Redshift Survey, targeting galaxies with redshifts that place the rest-frame...
Measurement of Star-Formation Rate from H-alpha in field galaxies at z=1 (1998)
Glazebrook, Karl, Blake, Chris, Economou, Frossie, Lilly, Simon, Colless, Matthew
We report the results of J-band infrared spectroscopy of a sample of 13 z=1 field galaxies drawn from the Canada-France Redshift Survey, targeting galaxies whose redshifts place the rest frame...