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dc.contributor.authorDriver, Simon P.
dc.contributor.authorWright, Angus H.
dc.contributor.authorAndrews, Stephen K.
dc.contributor.authorDavies, Luke J.
dc.contributor.authorKafle, Prajwal R.
dc.contributor.authorLange, Rebecca
dc.contributor.authorMoffett, Amanda J.
dc.contributor.authorMannering, Elizabeth
dc.contributor.authorRobotham, Aaron S. G.
dc.contributor.authorVinsen, Kevin
dc.contributor.authorAlpaslan, Mehmet
dc.contributor.authorAndrae, Ellen
dc.contributor.authorBaldry, Ivan K.
dc.contributor.authorBauer, Amanda E.
dc.contributor.authorBamford, Steven P.
dc.contributor.authorBland-Hawthorn, Joss
dc.contributor.authorBourne, Nathan
dc.contributor.authorBrough, Sarah
dc.contributor.authorBrown, Michael J. I.
dc.contributor.authorCluver, Michelle E.
dc.contributor.authorCroom, Scott
dc.contributor.authorColless, Matthew
dc.contributor.authorConselice, Christopher J.
dc.contributor.authorda Cunha, Elisabete
dc.contributor.authorDe Propris, Roberto
dc.contributor.authorDrinkwater, Michael
dc.contributor.authorDunne, Loretta
dc.contributor.authorEales, Steve
dc.contributor.authorEdge, Alastair
dc.contributor.authorFrenk, Carlos
dc.contributor.authorGraham, Alister W.
dc.contributor.authorGrootes, Meiert
dc.contributor.authorHolwerda, Benne W.
dc.contributor.authorHopkins, Andrew M.
dc.contributor.authorIbar, Edo
dc.contributor.authorvan Kampen, Eelco
dc.contributor.authorKelvin, Lee S.
dc.contributor.authorJarrett, Tom
dc.contributor.authorJones, D. Heath
dc.contributor.authorLara-Lopez, Maritza A.
dc.contributor.authorLiske, Jochen
dc.contributor.authorLopez-Sanchez, Angel R.
dc.contributor.authorLoveday, Jon
dc.contributor.authorMaddox, Steve J.
dc.contributor.authorMadore, Barry
dc.contributor.authorMahajan, Smriti
dc.contributor.authorMeyer, Martin
dc.contributor.authorNorberg, Peder
dc.contributor.authorPenny, Samantha J.
dc.contributor.authorPhillipps, Steven
dc.contributor.authorPopescu, Cristina
dc.contributor.authorTuffs, Richard J.
dc.contributor.authorPeacock, John A.
dc.contributor.authorPimbblet, Kevin A.
dc.contributor.authorPrescott, Matthew
dc.contributor.authorRowlands, Kate
dc.contributor.authorSansom, Anne E.
dc.contributor.authorSeibert, Mark
dc.contributor.authorSmith, Matthew W. L.
dc.contributor.authorSutherland, Will J.
dc.contributor.authorTaylor, Edward N.
dc.contributor.authorValiante, Elisabetta
dc.contributor.authorVazquez-Mata, J. Antonio
dc.contributor.authorWang, Lingyu
dc.contributor.authorWilkins, Stephen M.
dc.contributor.authorWilliams, Richard
dc.identifier.citationDriver , S P , Wright , A H , Andrews , S K , Davies , L J , Kafle , P R , Lange , R , Moffett , A J , Mannering , E , Robotham , A S G , Vinsen , K , Alpaslan , M , Andrae , E , Baldry , I K , Bauer , A E , Bamford , S P , Bland-Hawthorn , J , Bourne , N , Brough , S , Brown , M J I , Cluver , M E , Croom , S , Colless , M , Conselice , C J , da Cunha , E , De Propris , R , Drinkwater , M , Dunne , L , Eales , S , Edge , A , Frenk , C , Graham , A W , Grootes , M , Holwerda , B W , Hopkins , A M , Ibar , E , van Kampen , E , Kelvin , L S , Jarrett , T , Jones , D H , Lara-Lopez , M A , Liske , J , Lopez-Sanchez , A R , Loveday , J , Maddox , S J , Madore , B , Mahajan , S , Meyer , M , Norberg , P , Penny , S J , Phillipps , S , Popescu , C , Tuffs , R J , Peacock , J A , Pimbblet , K A , Prescott , M , Rowlands , K , Sansom , A E , Seibert , M , Smith , M W L , Sutherland , W J , Taylor , E N , Valiante , E , Vazquez-Mata , J A , Wang , L , Wilkins , S M & 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 , vol. 455 , no. 4 , pp. 3911-3942 .
dc.identifier.otherPURE: 242361732
dc.identifier.otherPURE UUID: fc944dff-8770-4689-b16e-5e7b0e6c72ca
dc.identifier.otherBibCode: 2016MNRAS.455.3911D
dc.identifier.otherScopus: 84955490828
dc.identifier.otherWOS: 000368009300042
dc.descriptionLD and SJM acknowledge support from the European Advanced Investigator grant cosmicism. SB acknowledges support from an ARC Future Fellowship (FT140101166).NB acknowledges support from EC FP7 SPACE project ASTRODEEP (Ref. No: 312725). EI acknowledges funding from CONICYT/FONDECYT post-doctoral project no: 3130504. MALL acknowledges support from UNAM through PAPIIT project IA101315. PN acknowledges the support of the Royal Society through the award of a University Research Fellowship, the European Research Council, through receipt of a Starting Grant (DEGAS-259586) and support of the Science and Technology Facilities Council (ST/L00075X/1). Funding for the SDSS and SDSS-II has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, the US Department of Energy, the National Aeronautics and Space Administration, the Japanese Monbukagakusho, the Max Planck Society, and the Higher Education Funding Council for England.en
dc.description.abstractWe present the Galaxy And Mass Assembly (GAMA) Panchromatic Data Release (PDR) constituting over 230 deg2 of imaging with photometryin 21 bands extending from the far-UV to the far-IR. These data complement our spectroscopic campaign of over 300k galaxies, and are compiled from observations with a variety of facilities including: GALaxy Evolution eXplorer, Sloan Digital Sky Survey, Visible and Infrared Telescope for Astronomy (VISTA), Wide-field Infrared Survey Explorer, and Herschel, with the GAMA regions currently being surveyed by VLT Survey Telescope (VST) and scheduled for observations by Australian Square Kilometer Array Pathfinder (ASKAP). These data are processed to a common astrometric solution, from which photometry is derived for ∼221 373 galaxies with r <19.8 mag. Online tools are provided to access and download data cutouts, or the full mosaics of the GAMA regions in each band. We focus, in particular, on the reduction and analysis of the VISTA VIsta Kilo-degree INfrared Galaxy data, and compare to earlier data sets (i.e. 2MASS and UKIDSS) before combining the data and examining its integrity. Having derived the 21-band photometric catalogue, we proceed to fit the data using the energy balance code MAGPHYS. These measurements are then used to obtain the first fully empirical measurement of the 0.1-500 μm energy output of the Universe. Exploring the cosmic spectral energy distribution across three time-intervals (0.3-1.1, 1.1-1.8, and 1.8-2.4 Gyr), we find that the Universe is currently generating (1.5 ± 0.3) ×1035 h70 W Mpc-3, down from (2.5± 0.2) × 1035 h70 W Mpc-32.3 Gyr ago. More importantly, we identify significant and smooth evolution in the integrated photon escape fraction at all wavelengths, with the UV escape fraction increasing from 27(18) per cent at z = 0.18in NUV(FUV) to 34(23) per cent at z = 0.06. The GAMA PDR can be found at:
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.rights© 2015 The Authors, Published by Oxford University Press on behalf of the Royal Astronomical Society. This work is made available online in accordance with the publisher’s policies. This is the final published version of the work, which was originally published at
dc.subjectAstronomical data bases: miscellaneousen
dc.subjectGalaxies: evolutionen
dc.subjectGalaxies: generalen
dc.subjectGalaxies: photometryen
dc.subjectSosmology: observationsen
dc.subjectQC Physicsen
dc.subjectQB Astronomyen
dc.titleGalaxy And Mass Assembly (GAMA) : Panchromatic Data Release (far-UV-far-IR) and the low-z energy budgeten
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews.School of Physics and Astronomyen
dc.contributor.institutionUniversity of St Andrews.School of Biologyen
dc.description.statusPeer revieweden

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