GAMA: towards a physical understanding of galaxy formation (2009)
Driver, Simon P., Norberg, Peder, Baldry, Ivan K., Bamford, Steven P., Hopkins, Andrew M., Liske, Jochen, ...
The Galaxy And Mass Assembly (GAMA) project is the latest in a tradition of large galaxy redshift surveys, and is now underway on the 3.9m Anglo-Australian Telescope at Siding Spring Observatory....
Galaxy Zoo: Passive Red Spirals (2009)
Masters, Karen L., Mosleh, Moein, Romer, A. Kathy, Nichol, Robert C., Bamford, Steven P., Schawinski, Kevin, ...
We study the spectroscopic properties and environments of red spiral galaxies found by the Galaxy Zoo project. By carefully selecting face-on, disk dominated spirals we construct a sample of truly...
Galaxy Zoo Green Peas: Discovery of A Class of Compact Extremely Star-Forming Galaxies (2009)
Cardamone, Carolin N., Schawinski, Kevin, Sarzi, Marc, Bamford, Steven P., Bennert, Nicola, Urry, C. M., ...
We investigate a class of rapidly growing emission line galaxies, known as "Green Peas", first noted by volunteers in the Galaxy Zoo project because of their peculiar bright green colour and small...
Galaxy Zoo: A sample of blue early-type galaxies at low redshift (2009)
Schawinski, Kevin, Lintott, Chris, Thomas, Daniel, Sarzi, Marc, Andreescu, Dan, Bamford, Steven P., ...
We report the discovery of a population of nearby, blue early-type galaxies with high star formation rates (0.5 < SFR < 50 Msun/yr). They are identified by their visual morphology as provided by...
Galaxy Zoo: a sample of blue early-type galaxies at low redshift (2009)
Schawinski, Kevin, Lintott, Chris, Thomas, Daniel, Sarzi, Marc, Andreescu, Dan, Bamford, Steven P., ...
GAMA: towards a physical understanding of galaxy formation (2009)
Driver, Simon P., Norberg, Peder, Baldry, Ivan K., Bamford, Steven P., Hopkins, Andrew M., Liske, Jochen, ...
Reviews progress on the latest large galaxy redshift survey now underway on the 3.9 m Anglo-Australian Telescope.
Galaxy Zoo: Disentangling the Environmental Dependence of Morphology and Colour (2008)
Skibba, Ramin A., Bamford, Steven P., Nichol, Robert C., Lintott, Chris J., Andreescu, Dan, Edmondson, Edward M., ...
We analyze the environmental dependence of galaxy morphology and colour with two-point clustering statistics, using data from the Galaxy Zoo, the largest sample of visually classified morphologies...
Revealing components of the galaxy population through nonparametric techniques (2008)
Bamford, Steven P., Rojas, Alex L., Nichol, Robert C., Miller, Christopher J., Wasserman, Larry, Genovese, Christopher R., ...
The distributions of galaxy properties vary with environment, and are often multimodal, suggesting that the galaxy population may be a combination of multiple components. The behaviour of these...
Galaxy Zoo: the dependence of morphology and colour on environment (2008)
Bamford, Steven P., Nichol, Robert C., Baldry, Ivan K., Land, Kate, Lintott, Chris J., Schawinski, Kevin, ...
We analyse the relationships between galaxy morphology, colour, environment and stellar mass using data for over 100,000 objects from Galaxy Zoo, the largest sample of visually classified...
Milvang-Jensen, Bo, Noll, Stefan, Halliday, Claire, Poggianti, Bianca M., Jablonka, Pascale, Aragon-Salamanca, Alfonso, ...
AIMS. We present spectroscopic observations of galaxies in 15 survey fields as part of the ESO Distant Cluster Survey (EDisCS). We determine the redshifts and velocity dispersions of the galaxy...
The Tully-Fisher relation of galaxies at z~0.85 in the DEEP2 survey (2007)
Chiu, Kuenley, Bamford, Steven P., Bunker, Andrew
Local and intermediate redshift (z~0.5) galaxy samples obey well correlated relations between the stellar population luminosity and maximal galaxy rotation that define the Tully-Fisher (TF) relation....
The evolution on disk galaxies in clusters and the field (2007)
Bamford, Steven P., Aragón-Salamanca, Alfonso, Milvang-Jensen, Bo
The 2MASS Tully-Fisher Relation and Local Peculiar Velocities (2002)
This study assesses the utility of applying the Tully-Fisher (TF) relation using photometric data from the 2MASS project. This is achieved by performing a preliminary analysis using 2MASS extended...