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The HerMES Local Luminosity Function

Part of: IAU Issue 315 - From Interstellar Clouds...

Published online by Cambridge University Press:  12 September 2016

Lucia Marchetti ,
Mattia Vaccari  and
Alberto Franceschini
Lucia Marchetti
Affiliation:
Department of Physical Sciences, The Open University, UK Dipartimento di Fisica e Astronomia, Università di Padova, Italy
Mattia Vaccari
Affiliation:
Dipartimento di Fisica e Astronomia, Università di Padova, Italy Astrophysics Group, Physics Department, University of the Western Cape, South Africa INAF - Istituto di Radioastronomia, Italy email: lucia.marchetti@open.ac.uk
Alberto Franceschini
Affiliation:
Dipartimento di Fisica e Astronomia, Università di Padova, Italy
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Abstract

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We exploit the Herschel Extragalactic Multi-Tiered Survey (HerMES) dataset along with ancillary multi-wavelength photometry and spectroscopy from the Spitzer Data Fusion to provide the most accurate determination to date of the local (0.02<z<0.5) Far-Infrared Luminosity and Star Formation Rate Function. We present and compare our results with model predictions as well as other multi-wavelength estimates of the local star formation rate density.

Keywords

galaxies: luminosity functionmass functiongalaxies: evolutioninfrared: galaxiessubmillimeterastronomical data bases: miscellaneous
Type
Poster Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Symposium S315: From Interstellar Clouds to Star-Forming Galaxies: Universal Processes? , August 2015 , E52
Copyright
Copyright © International Astronomical Union 2016 

References

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