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Comparing the relation between star formation and galaxy mass in different environments
Benedetta Vulcani, Bianca M. Poggianti, Rose A. Finn +3
Analyzing 24 mu m MIPS/Spitzer data and the [O II]3727 line of a sample of galaxies at 0.4 < z < 0.8 from the ESO Distant Cluster Survey (EDisCS), we investigate the ongoing star f…
GAMA: towards a physical understanding of galaxy formation
Simon P. Driver, Peder Norberg, Ivan K. Baldry +46
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 Spri…
Galaxy and Mass Assembly (GAMA): Optimal Tiling of Dense Surveys with a Multi-Object Spectrograph
Aaron Robotham, S. P. Driver, P. Norberg +23
A heuristic greedy algorithm is developed for efficiently tiling spatially dense redshift surveys. In its first application to the Galaxy and Mass Assembly (GAMA) redshift survey w…
Galaxy And Mass Assembly (GAMA): The input catalogue and star-galaxy separation
I. K. Baldry, A. S. G. Robotham, D. T. Hill +24
We describe the spectroscopic target selection for the Galaxy And Mass Assembly (GAMA) survey. The input catalogue is drawn from the Sloan Digital Sky Survey (SDSS) and UKIRT Infra…
Galaxy Zoo: Passive Red Spirals
Karen L. Masters, Moein Mosleh, A. Kathy Romer +14
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…
Galaxy Zoo: Reproducing Galaxy Morphologies Via Machine Learning
Manda Banerji, Ofer Lahav, Chris J. Lintott +10
We present morphological classifications obtained using machine learning for objects in SDSS DR6 that have been classified by Galaxy Zoo into three classes, namely early types, spi…