• DOI:10.1111/j.1365-2966.2010.17643.x
• Corpus ID: 12697421

The Deep SPIRE HerMES Survey: spectral energy distributions and their astrophysical indications at high redshift

@inproceedings{Brisbin2010TheDS,
  title={The Deep SPIRE HerMES Survey: spectral energy distributions and their astrophysical indications at high redshift},
  author={D. Brisbin and Martin O. Harwit and Bruno Altieri and Alexandre Amblard and Vinodiran Arumugam and H. Aussel and T. S. R. Babbedge and A. W. Blain and James J. Bock and Alessandro Boselli and V{\'e}ronique Buat and Nieves Castro-Rodr'iguez and Antonio Cava and P. Chanial and David L. Clements and Alex Conley and L Conversi and Asantha Cooray and Charles Darren Dowell and Eli Dwek and Stephen A. Eales and David Elbaz and M. J. Fox and Alberto Franceschini and Walter Gear and Jason Glenn and Matthew Joseph Griffin and Mark Halpern and Evanthia Hatziminaoglou and Edo Ibar and Kate Gudrun Isaak and R. J. Ivison and Guilaine Lagache and Louis Robert Levenson and Carol J. Lonsdale and Nanyao Lu and Steve Madden and Bruno Maffei and Gabriele Mainetti and Lucia Marchetti and Glenn Evan Morrison and H. T. Nguyen and Brian O'Halloran and Seb Oliver and Alain Omont and Frazer N. Owen and Maurilio Pannella and Pasquale Panuzzo and Andreas Papageorgiou and C. P. Pearson and Ismael P'erez-Fournon and Michael F. Pohlen and David Del Rizzo and Isaac Roseboom and Michael Rowan-Robinson and M. S'anchez Portal and Bernhard Schulz and Nick Seymour and David L. Shupe and A. J. Smith and Jason A. Stevens and Veronica Strazzullo and Myrto Symeonidis and Markos Trichas and K. E. Tugwell and Mattia Vaccari and Ivan Valtchanov and Laurent G. Vigroux and L. Wang and Robyn L. Ward and Geoffrey A. E. Wright and C. Kevin Xu and Michael Zemcov},
  year={2010}
}

• D. Brisbin, M. Harwit, +70 authors M. Zemcov
• Published 7 September 2010
• Physics

The Spectral and Photometric Imaging Receiver on-board Herschel has been carrying out deep extragalactic surveys, one of the aims of which is to establish spectral energy distributions of individual galaxies spanning the infrared/submillimetre (IR/SMM) wavelength region. We report observations of the IR/SMM emission from the Lockman North field and Great Observatories Origins Deep Survey Field-North. Because galaxy images in the wavelength range covered by Herschel generally represent a blend with contributions from neighbouring galaxies, we present sets of galaxies in each field, especially free of blending at 250, 350 and 500 mu m. We identify the cumulative emission of these galaxies and the fraction of the FIR cosmic background radiation they contribute. Our surveys reveal a number of highly luminous galaxies at redshift z less than or similar to 3 and a novel relationship between IR and visible emission that shows a dependence on luminosity and redshift.