4.7 Article

Galaxy And Mass Assembly (GAMA): Panchromatic Data Release (far-UV-far-IR) and the low-z energy budget

Journal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 455, Issue 4, Pages 3911-3942

Publisher

OXFORD UNIV PRESS
DOI: 10.1093/mnras/stv2505

Keywords

astronomical data bases: miscellaneous; galaxies: evolution; galaxies: general; galaxies: photometry; cosmology: observations

Funding

  1. European Advanced Investigator grant cosmicism
  2. ARC Future Fellowship [FT140101166]
  3. EC FP7 SPACE project ASTRODEEP [312725]
  4. CONICYT/FONDECYT [3130504]
  5. UNAM through PAPIIT project [IA101315]
  6. Royal Society through the award of a University Research Fellowship
  7. European Research Council [DEGAS-259586]
  8. Science and Technology Facilities Council [ST/L00075X/1]
  9. Alfred P. Sloan Foundation
  10. National Science Foundation
  11. US Department of Energy
  12. National Aeronautics and Space Administration
  13. Japanese Monbukagakusho
  14. Max Planck Society
  15. Higher Education Funding Council for England
  16. American Museum of Natural History
  17. Astrophysical Institute Potsdam
  18. University of Basel
  19. University of Cambridge
  20. Case Western Reserve University
  21. University of Chicago
  22. Drexel University
  23. Fermilab
  24. Institute for Advanced Study
  25. Japan Participation Group
  26. Johns Hopkins University
  27. Joint Institute for Nuclear Astrophysics
  28. Kavli Institute for Particle Astrophysics and Cosmology
  29. Korean Scientist Group
  30. Chinese Academy of Sciences (LAMOST)
  31. Los Alamos National Laboratory
  32. Max-Planck-Institute for Astronomy (MPIA)
  33. Max-Planck-Institute for Astrophysics (MPA)
  34. New Mexico State University
  35. Ohio State University
  36. University of Pittsburgh
  37. University of Portsmouth
  38. Princeton University
  39. United States Naval Observatory
  40. University of Washington
  41. ESO Telescopes at the La Silla Paranal Observatory [179.A-2004]
  42. STFC (UK)
  43. ARC (Australia)
  44. AAO
  45. Australian Government
  46. Government of Western Australia
  47. Science and Technology Facilities Council [ST/L000652/1, ST/J001414/1, ST/J002291/1, ST/H008578/1, ST/H001530/1, ST/H007156/1, ST/M000966/1, ST/M000907/1, ST/I003088/1, ST/H00131X/1, ST/J001546/1, ST/K003577/1, ST/L00075X/1] Funding Source: researchfish
  48. STFC [ST/H008578/1, ST/J001414/1, ST/K003577/1, ST/L000652/1, ST/J002291/1, ST/L000695/1, ST/L00075X/1, ST/K000926/1, ST/I003088/1, ST/H007156/1, ST/J001546/1, ST/M000907/1, ST/H001530/1, ST/H00131X/1] Funding Source: UKRI

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We present the Galaxy And Mass Assembly (GAMA) Panchromatic Data Release (PDR) constituting over 230 deg(2) 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 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 similar to 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 mu m 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) x 10(35) h(70) W Mpc(-3), down from (2.5 +/- 0.2) x 10(35) h(70) W Mpc(-3) 2.3 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 = 0.18 in NUV(FUV) to 34(23) per cent at z = 0.06. The GAMA PDR can be found at: http://gama-psi.icrar.org/.

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