Herschel-ATLAS/GAMA : dusty early-type galaxies and passive spirals

Rowlands, K.; Dunne, L.; Maddox, S.; Bourne, N.; Gomez, H.L.; Kaviraj, S.; Bamford, S.P.; Brough, S.; Charlot, S.; da Cunha, E.; Driver, S.P.; Eales, S.A.; Hopkins, A.M.; Kelvin, L.; Nichol, R.C.; Sansom, A.E.; Sharp, R.; Smith, D.J.B.; Temi, P.; van der Werf, P.; Baes, M.; Cava, A.; Cooray, A.; Croom, S.M.; Dariush, A.; De Zotti, G.; Dye, S.; Fritz, J.; Hopwood, R.; Ibar, E.; Ivison, R.J.; Liske, J.; Loveday, J.; Madore, B.; Norberg, P.; Popescu, C.C.; Rigby, E.E.; Robotham, A.; Rodighiero, G.; Seibert, M.; Tuffs, R.J.

doi:10.1111/j.1365-2966.2011.19905.x

Galaxy And Mass Assembly (GAMA): the 0.013 < z < 0.1 cosmic spectral energy distribution from 0.1 μm to 1 mm (2012)
Journal Article
Driver, S., Robotham, A., Kelvin, L., Alpaslan, M., Baldry, I., Bamford, S., …Wilkins, S. (2012). Galaxy And Mass Assembly (GAMA): the 0.013 < z < 0.1 cosmic spectral energy distribution from 0.1 μm to 1 mm. Monthly Notices of the Royal Astronomical Society, 427(4), 3244-3264. https://doi.org/10.1111/j.1365-2966.2012.22036.x

We use the Galaxy And Mass Assembly survey (GAMA) I data set combined with GALEX, Sloan Digital Sky Survey (SDSS) and UKIRT Infrared Deep Sky Survey (UKIDSS) imaging to construct the low-redshift (z < 0.1) galaxy luminosity functions in FUV, NUV, ugr... Read More about Galaxy And Mass Assembly (GAMA): the 0.013 < z < 0.1 cosmic spectral energy distribution from 0.1 μm to 1 mm.

Galaxy And Mass Assembly (GAMA): the mass-metallicity relationship (2012)
Journal Article
Foster, C., Hopkins, A., Gunawardhana, M., Lara-López, M., Sharp, R., Steele, O., …Wijesinghe, D. (2012). Galaxy And Mass Assembly (GAMA): the mass-metallicity relationship. Astronomy & Astrophysics, 547, https://doi.org/10.1051/0004-6361/201220050

Herschel-ATLAS/GAMA : spatial clustering of low-redshift submm galaxies (2012)
Journal Article
van Kampen, E., Smith, D., Maddox, S., Hopkins, A., Valtchanov, I., Peacock, J., …Tuffs, R. (2012). Herschel-ATLAS/GAMA : spatial clustering of low-redshift submm galaxies. Monthly Notices of the Royal Astronomical Society, 426(4), 3455-3463. https://doi.org/10.1111/j.1365-2966.2012.21949.x

We have measured the clustering properties of low-redshift (z < 0.3) submm galaxies detected at 250 μm in the Herschel-ATLAS science demonstration phase field. We selected a sample for which we have high-quality spectroscopic redshifts, obtained from... Read More about Herschel-ATLAS/GAMA : spatial clustering of low-redshift submm galaxies.

Galaxy And Mass Assembly (GAMA) : estimating galaxy group masses via caustic analysis (2012)
Journal Article
Alpaslan, M., Robotham, A., Driver, S., Norberg, P., Peacock, J., Baldry, I., …Pimbblet, K. (2012). Galaxy And Mass Assembly (GAMA) : estimating galaxy group masses via caustic analysis. Monthly Notices of the Royal Astronomical Society, 426(4), 2832-2846. https://doi.org/10.1111/j.1365-2966.2012.21020.x

We have generated complementary halo mass estimates for all the groups in the Galaxy And Mass Assembly Galaxy Group Catalogue (GAMA G3Cv1) using a modified caustic mass estimation algorithm, originally developed by Diaferio & Geller. We calibrate the... Read More about Galaxy And Mass Assembly (GAMA) : estimating galaxy group masses via caustic analysis.

Galaxy and mass assembly (GAMA): colour- and luminosity-dependent clustering from calibrated photometric redshifts (2012)
Journal Article
Christodoulou, L., Eminian, C., Loveday, J., Norberg, P., Baldry, I., Hurley, P., …Wijesinghe, D. (2012). Galaxy and mass assembly (GAMA): colour- and luminosity-dependent clustering from calibrated photometric redshifts. Monthly Notices of the Royal Astronomical Society, 425(2), 1527-1548. https://doi.org/10.1111/j.1365-2966.2012.21434.x

We measure the two-point angular correlation function of a sample of 4289 223 galaxies with r < 19.4 mag from the Sloan Digital Sky Survey (SDSS) as a function of photometric redshift, absolute magnitude and colour down to Mr − 5 log h = −14 mag. Pho... Read More about Galaxy and mass assembly (GAMA): colour- and luminosity-dependent clustering from calibrated photometric redshifts.

Galaxy And Mass Assembly (GAMA) : in search of Milky Way Magellanic Cloud analogues (2012)
Journal Article
Robotham, A., Baldry, I., Bland-Hawthorn, J., Driver, S., Loveday, J., Norberg, P., …Staveley-Smith, L. (2012). Galaxy And Mass Assembly (GAMA) : in search of Milky Way Magellanic Cloud analogues. Monthly Notices of the Royal Astronomical Society, 424(2), 1448-1453. https://doi.org/10.1111/j.1365-2966.2012.21332.x

Analysing all Galaxy And Mass Assembly (GAMA) galaxies within a factor of 2 (±0.3 dex) of the stellar mass of the Milky Way (MW), there is a 11.9 per cent chance that one of these galaxies will have a close companion (within a projected separation of... Read More about Galaxy And Mass Assembly (GAMA) : in search of Milky Way Magellanic Cloud analogues.

Galaxy And Mass Assembly (GAMA) : galaxy environments and star formation rate variations (2012)
Journal Article
Wijesinghe, D., Hopkins, A., Brough, S., Taylor, E., Norberg, P., Bauer, A., …Tuffs, R. (2012). Galaxy And Mass Assembly (GAMA) : galaxy environments and star formation rate variations. Monthly Notices of the Royal Astronomical Society, 423(4), 3679-3691. https://doi.org/10.1111/j.1365-2966.2012.21164.x

We present a detailed investigation into the effects of galaxy environment on their star formation rates (SFRs) using galaxies observed in the Galaxy And Mass Assembly (GAMA) survey. We use three independent volume-limited samples of galaxies within... Read More about Galaxy And Mass Assembly (GAMA) : galaxy environments and star formation rate variations.

Herschel-ATLAS/GAMA : a census of dust in optically selected galaxies from stacking at submillimetre wavelengths (2012)
Journal Article
Bourne, N., Maddox, S., Dunne, L., Auld, R., Baes, M., Baldry, I., …Temi, P. (2012). Herschel-ATLAS/GAMA : a census of dust in optically selected galaxies from stacking at submillimetre wavelengths. Monthly Notices of the Royal Astronomical Society, 421(4), 3027-3059. https://doi.org/10.1111/j.1365-2966.2012.20528.x

We use the Herschel‐ATLAS survey to conduct the first large‐scale statistical study of the submillimetre properties of optically selected galaxies. Using ∼80 000 r‐band selected galaxies from 126 deg2 of the GAMA survey, we stack into submillimetre... Read More about Herschel-ATLAS/GAMA : a census of dust in optically selected galaxies from stacking at submillimetre wavelengths.

Galaxy And Mass Assembly (GAMA) : structural investigation of galaxies via model analysis (2012)
Journal Article
Kelvin, L., Driver, S., Robotham, A., Hill, D., Alpaslan, M., Baldry, I., …Tuffs, R. (2012). Galaxy And Mass Assembly (GAMA) : structural investigation of galaxies via model analysis. Monthly Notices of the Royal Astronomical Society, 421(2), 1007-1039. https://doi.org/10.1111/j.1365-2966.2012.20355.x

We present single-Sérsic two-dimensional (2D) model fits to 167 600 galaxies modelled independently in the ugrizYJHK bandpasses using reprocessed Sloan Digital Sky Survey Data Release Seven (SDSS DR7) and UKIRT Infrared Deep Sky Survey Large Area Sur... Read More about Galaxy And Mass Assembly (GAMA) : structural investigation of galaxies via model analysis.

Galaxy And Mass Assembly (GAMA): the galaxy stellar mass function at z < 0.06 (2012)
Journal Article
Baldry, I., Driver, S., Loveday, J., Taylor, E., Kelvin, L., Liske, J., …Tuffs, R. (2012). Galaxy And Mass Assembly (GAMA): the galaxy stellar mass function at z < 0.06. Monthly Notices of the Royal Astronomical Society, 421(1), 621-634. https://doi.org/10.1111/j.1365-2966.2012.20340.x

We determine the low-redshift field galaxy stellar mass function (GSMF) using an area of 143 deg2 from the first three years of the Galaxy And Mass Assembly (GAMA) survey. The magnitude limits of this redshift survey are r < 19.4 mag over two-thirds... Read More about Galaxy And Mass Assembly (GAMA): the galaxy stellar mass function at z < 0.06.

Galaxy and Mass Assembly (GAMA): ugriz galaxy luminosity functions (2012)
Journal Article
Loveday, J., Norberg, P., Baldry, I., Driver, S., Hopkins, A., Peacock, J., …Wijesinghe, D. (2012). Galaxy and Mass Assembly (GAMA): ugriz galaxy luminosity functions. Monthly Notices of the Royal Astronomical Society, 420(2), 1239-1262. https://doi.org/10.1111/j.1365-2966.2011.20111.x

Galaxy and Mass Assembly (GAMA) is a project to study galaxy formation and evolution, combining imaging data from ultraviolet to radio with spectroscopic data from the AAOmega spectrograph on the Anglo-Australian Telescope. Using data from Phase 1 of... Read More about Galaxy and Mass Assembly (GAMA): ugriz galaxy luminosity functions.

Herschel-ATLAS/GAMA : dusty early-type galaxies and passive spirals (2012)
Journal Article
Rowlands, K., Dunne, L., Maddox, S., Bourne, N., Gomez, H., Kaviraj, S., …Tuffs, R. (2012). Herschel-ATLAS/GAMA : dusty early-type galaxies and passive spirals. Monthly Notices of the Royal Astronomical Society, 419(3), 2545-2578. https://doi.org/10.1111/j.1365-2966.2011.19905.x

We present the dust properties and star formation histories of local submillimetre-selected galaxies, classified by optical morphology. Most of the galaxies are late types and very few are early types. The early-type galaxies (ETGs) that are detected... Read More about Herschel-ATLAS/GAMA : dusty early-type galaxies and passive spirals.

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