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A snapshot beyond the Local Universe with Herschel/SPIRE

Published online by Cambridge University Press:  17 August 2016

Sandor Pinter ,
Gabor Marton ,
L. Viktor Toth ,
Chris Pearson ,
Zsolt Bagoly ,
Lajos G. Balazs ,
Istvan Horvath  and
Istvan I. Racz
Sandor Pinter
Affiliation:
Eotvos Lorand University, Hungary, email: [email protected]
Gabor Marton
Affiliation:
Konkoly Observatory of the Hungarian Academy of Sciences
L. Viktor Toth
Affiliation:
Eotvos Lorand University, Hungary, email: [email protected]
Chris Pearson
Affiliation:
Science and Technology Facilities Council Rutherford Appleton Laboratory
Zsolt Bagoly
Affiliation:
Eotvos Lorand University, Hungary, email: [email protected]
Lajos G. Balazs
Affiliation:
Eotvos Lorand University, Hungary, email: [email protected] Konkoly Observatory of the Hungarian Academy of Sciences
Istvan Horvath
Affiliation:
National University of Public Service, Hungary
Istvan I. Racz
Affiliation:
Eotvos Lorand University, Hungary, email: [email protected]
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Abstract

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The European Large-Area ISO Survey (ELAIS) N1 field is one of the extragalactic windows where the lack of the Galactic ISM allows us to analyze the unbiased FIR properties of extragalactic objects. The field was investigated recently based on Herschel observations by the HerMES key project. We present a survey of the field covering a larger area than HerMES (12.54 deg2 vs 3.47 deg2). We provide accurate 250, 350, and 500 micrometer flux densities for about 8000 point sources using the latest Herschel analysis and calibration procedures. Based on SDSS spectroscopic and SWIRE photometric data our sample has approximately 4000 and 4500 galaxies with 0.2 < z < 0.5 and z > 0.5 redshifts, respectively. The new flux densities are crucial limiting the star-forming activity of galaxies outside the Local Universe, as it is demonstrated in the star-forming galaxy 2MASS J16072472+5412119.

Keywords

galaxies: starburstinfrared: galaxiesgalaxies: individual (ELAIS N1-015)
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Symposium S319: Galaxies at High Redshift and Their Evolution Over Cosmic Time , August 2015 , pp. 103 - 104
Copyright
Copyright © International Astronomical Union 2016 

References

Oliver, S. et al. 2012 MNRAS, 424, 1614 Google Scholar
Ott, S. 2010 ASP Conference, 434, 139 Google Scholar
Pearson, C. et al. 2014 Exp. Astr., 37, 175 CrossRefGoogle Scholar
Rowan-Robinson, M. et al. 2013 MNRAS, 428, 1958 Google Scholar
Sajina, A. et al. 2006 MNRAS, 369, 939 Google Scholar