4.7 Article

G10/COSMOS: 38 band (far-UV to far-IR) panchromatic photometry using LAMBDAR

Journal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 464, Issue 2, Pages 1569-1590

Publisher

OXFORD UNIV PRESS
DOI: 10.1093/mnras/stw2395

Keywords

catalogues; galaxies: general; galaxies: photometry

Funding

  1. Australian Government's Department of Industry Australian Postgraduate Awards (APA)
  2. Australian Research Council [140100395]
  3. ESO Telescopes at the La Silla or Paranal Observatories [175.A-0839]
  4. International Centre for Radio Astronomy Research (ICRAR) at the University of Western Australia
  5. ESO Telescopes at the La Silla Paranal Observatory under ESO programme [179.A-2005]
  6. NASA [1407]

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We present a consistent total flux catalogue for a similar to 1 deg(2) subset of the Cosmic Evolution Survey (COSMOS) region (RA is an element of [149.degrees 55, 150.degrees 65], Dec. is an element of [1.degrees 80, 2.degrees 73]) with near-complete coverage in 38 bands from the far-ultraviolet to the far-infrared. We produce aperture matched photometry for 128 304 objects with i < 24.5 in a manner that is equivalent to the Wright et al. catalogue from the low-redshift (z < 0.4) Galaxy and Mass Assembly (GAMA) survey. This catalogue is based on publicly available imaging from GALEX, Canada-France-Hawaii Telescope, Subaru, Visible and Infrared Survey Telescope for Astronomy, Spitzer and Herschel, contains a robust total flux measurement or upper limit for every object in every waveband and complements our re-reduction of publicly available spectra in the same region. We perform a number of consistency checks, demonstrating that our catalogue is comparable to existing data sets, including the recent COSMOS2015 catalogue. We also release an updated Davies et al. spectroscopic catalogue that folds in new spectroscopic and photometric redshift data sets. The catalogues are available for download at http://cutout.icrar.org/G10/dataRelease.php. Our analysis is optimised for both panchromatic analysis over the full wavelength range and for direct comparison to GAMA, thus permitting measurements of galaxy evolution for 0 < z < 1 while minimizing the systematic error resulting from disparate data reduction methods.

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