• DOI:10.1093/mnras/stw712
• Corpus ID: 53142310

A complete census of Herschel-detected infrared sources within the HST Frontier Fields

@article{Rawle2015ACC,
  title={A complete census of Herschel-detected infrared sources within the HST Frontier Fields},
  author={Timothy D. Rawle and Bruno Altieri and Eiichi Egami and Pablo G. P'erez-Gonz'alez and Fr'ed'eric Boone and Benjamin Cl{\'e}ment and Robert J. Ivison and Johan Richard and Wiphu Rujopakarn and Ivan Valtchanov and Gregory L. Walth and Benjamin J. Weiner and Andrew W. Blain and Miroslava Dessauges-Zavadsky and Jean-Paul Kneib and Dieter Lutz and Giulia Rodighiero and Daniel Schaerer and I. Smail Esaesac and ESASTScI and University of Arizona and Universidad Complutense de Madrid and Universit'e de Toulouse and Observatoire de Lyon and Eső and Royal Observatory of Edinburgh and Chulalongkorn University and University of Tokyo and University of Leicester and Obs. Geneve and Observatoire de Sauverny and Mpe and Universit̀a di Padova and Durham University},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2015},
  volume={459},
  pages={1626-1645}
}

• T. Rawle, B. Altieri, +31 authors D. University
• Published 3 August 2015
• Physics
• Monthly Notices of the Royal Astronomical Society

We present a complete census of all Herschel-detected sources within the six massive lensing clusters of the HST Frontier Fields (HFF). We provide a robust legacy catalogue of 263 sources with Herschel fluxes, primarily based on imaging from the Herschel Lensing Survey and PEP/HerMES Key Programmes. We optimally combine Herschel, Spitzer and WISE infrared (IR) photometry with data from HST, VLA and ground-based observatories, identifying counterparts to gain source redshifts. For each Herschel-detected source we also present magnification factor (mu), intrinsic IR luminosity and characteristic dust temperature, providing a comprehensive view of dust-obscured star formation within the HFF. We demonstrate the utility of our catalogues through an exploratory overview of the magnified population, including more than 20 background sub-LIRGs unreachable by Herschel without the assistance gravitational lensing.