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Galaxy And Mass Assembly (GAMA): the Stellar Mass Budget by Galaxy Type
Amanda J. Moffett, Stephen A. Ingarfield, Simon P. Driver +16
We report an expanded sample of visual morphological classifications from the Galaxy and Mass Assembly (GAMA) survey phase two, which now includes 7,556 objects (previously 3,727 i…
H-ATLAS/GAMA: The nature and characteristics of optically red galaxies detected at submillimetre wavelengths
A. Dariush, S. Dib, S. Hony +39
We combine Herschel/SPIRE sub-millimeter (submm) observations with existing multi-wavelength data to investigate the characteristics of low redshift, optically red galaxies detecte…
Galaxy And Mass Assembly (GAMA): growing up in a bad neighbourhood - how do low-mass galaxies become passive?
L. J. M. Davies, A. S. G. Robotham, S. P. Driver +13
Both theoretical predictions and observations of the very nearby Universe suggest that low-mass galaxies (log[M/M]<9.5) are likely to remain star-forming unl…
Galaxy and Mass Assembly (GAMA): Projected Galaxy Clustering
D. J. Farrow, Shaun Cole, Peder Norberg +11
We measure the projected 2-point correlation function of galaxies in the 180 deg equatorial regions of the GAMA II survey, for four different redshift slices between z = 0.0 an…
Galaxy And Mass Assembly (GAMA): The Bright Void Galaxy Population in the Optical and Mid-IR
S. J. Penny, M. J. I. Brown, K. A. Pimbblet +22
We examine the properties of galaxies in the Galaxies and Mass Assembly (GAMA) survey located in voids with radii Mpc. Utilising the GAMA equatorial survey, 592 void g…
Hyper-Fit: Fitting Linear Models to Multidimensional Data with Multivariate Gaussian Uncertainties
A. S. G. Robotham, D. Obreschkow
Astronomical data is often uncertain with errors that are heteroscedastic (different for each data point) and covariant between different dimensions. Assuming that a set of D-dimen…