Outputs (3)

Galaxy And Mass Assembly (GAMA): Panchromatic Data Release (far-UV-far-IR) and the low-z energy budget (2015)
Journal Article
Driver, S. P., Wright, A. H., Andrews, S. K., Davies, L. J., Kafle, P. R., Lange, R., …Williams, R. (2016). Galaxy And Mass Assembly (GAMA): Panchromatic Data Release (far-UV-far-IR) and the low-z energy budget. Monthly Notices of the Royal Astronomical Society, 455(4), 3911-3942. https://doi.org/10.1093/mnras/stv2505

We present the Galaxy And Mass Assembly (GAMA) Panchromatic Data Release (PDR) constituting over 230 deg2 of imaging with photometry in 21 bands extending from the far-UV to the far-IR. These data complement our spectroscopic campaign of over 300k ga... Read More about Galaxy And Mass Assembly (GAMA): Panchromatic Data Release (far-UV-far-IR) and the low-z energy budget.

Galaxy And Mass Assembly (GAMA): the effect of close interactions on star formation in galaxies (2015)
Journal Article
Davies, L., Robotham, A., Driver, S., Alpaslan, M., Baldry, I., Bland-Hawthorn, J., …Smith, M. (2015). Galaxy And Mass Assembly (GAMA): the effect of close interactions on star formation in galaxies. Monthly Notices of the Royal Astronomical Society, 452(1), 616-636. https://doi.org/10.1093/mnras/stv1241

The modification of star formation (SF) in galaxy interactions is a complex process, with SF observed to be both enhanced in major mergers and suppressed in minor pair interactions. Such changes likely to arise on short time-scales and be directly re... Read More about Galaxy And Mass Assembly (GAMA): the effect of close interactions on star formation in galaxies.

Co-evolution of black hole growth and star formation from a cross-correlation analysis between quasars and the cosmic infrared background (2015)
Journal Article
Wang, L., Viero, M., Ross, N., Asboth, V., Béthermin, M., Bock, J., …Zemcov, M. (2015). Co-evolution of black hole growth and star formation from a cross-correlation analysis between quasars and the cosmic infrared background. Monthly Notices of the Royal Astronomical Society, 449(4), 4476-4493. https://doi.org/10.1093/mnras/stv559

We present the first cross-correlation measurement between Sloan Digital Sky Survey type 1 quasars and the cosmic infrared background (CIB) measured by Herschel. The quasars cover the redshift range 0.15 < z < 3.5 where most of the CIB originates. We... Read More about Co-evolution of black hole growth and star formation from a cross-correlation analysis between quasars and the cosmic infrared background.