The Herschel* PEP/HerMES luminosity function - I. Probing the evolution of PACS selected Galaxies to z similar or equal to 4
- Gruppioni, C.
- Pozzi, F.
- Rodighiero, G.
- Delvecchio, I.
- Berta, S.
- Pozzetti, L.
- Zamorani, G.
- Andreani, P.
- Cimatti, Alessandro
- Ilbert, O.
- Le Floc'H, E.
- Lutz, D.
- Magnelli, B.
- Marchetti, L.
- Monaco, P.
- Nordon, R.
- Oliver, S.
- Popesso, P.
- Riguccini, L.
- Roseboom, I.
- Rosario, D. J.
- Sargent, M.
- Vaccari, M.
- Altieri, B.
- Aussel, H.
- Bongiovanni, A.
- Cepa, J.
- Daddi, E.
- Dominguez-Sanchez, H.
- Elbaz, D.
- Schreiber, N. Foerster
- Genzel, R.
- Iribarrem, A.
- Magliocchetti, M.
- Maiolino, R.
- Poglitsch, A.
- Perez Garcia, A.
- Sanchez-Portal, M.
- Sturm, E.
- Tacconi, L.
- Valtchanov, I.
- Amblard, A.
- Arumugam, V.
- Bethermin, M.
- Bock, J.
- Boselli, A.
- Buat, V.
- Burgarella, D.
- Castro-Rodriguez, N.
- Cava, A.
- Chanial, P.
- Clements, D. L.
- Conley, A.
- Cooray, A.
- Dowell, C. D.
- Dwek, E.
- Eales, S.
- Franceschini, A.
- Glenn, J.
- Griffin, M.
- Hatziminaoglou, E.
- Ibar, E.
- Isaak, K.
- Ivison, R. J.
- Lagache, Guilaine
- Levenson, L.
- Lu, N.
- Madden, S.
- Maffei, B.
- Mainetti, G.
- Nguyen, H. T.
- O'Halloran, B.
- Page, M. J.
- Panuzzo, P.
- Papageorgiou, A.
- Pearson, C. P.
- Perez-Fournon, I.
- Pohlen, M.
- Rigopoulou, D.
- Rowan-Robinson, M.
- Schulz, B.
- Scott, D.
- Seymour, N.
- Shupe, D. L.
- Smith, A. J.
- Stevens, J. A.
- Symeonidis, M.
- Trichas, M.
- Tugwell, K. E.
- Vigroux, L.
- Wang, L.
- Wright, Gavin
- Xu, C. K.
- Zemcov, M.
- Bardelli, S.
- Carollo, M.
- Contini, T.
- Le Fevre, O.
- Lilly, S.
- Mainieri, V.
- Renzini, A.
- Scodeggio, M.
- Zucca, E.
DOIAbstract
International audienceWe exploit the deep and extended far-IR data sets (at 70, 100 and 160 mu m) of the Herschel Guaranteed Time Observation (GTO) PACS Evolutionary Probe (PEP) Survey, in combination with the Herschel Multi-tiered Extragalactic Survey data at 250, 350 and 500 mu m, to derive the evolution of the rest-frame 35-, 60-, 90-and total infrared (IR) luminosity functions (LFs) up to z similar to 4. We detect very strong luminosity evolution for the total IR LF (L-IR alpha (1 + z)(3.55 +/- 0.10) up to z similar to 2, and. (1 + z) 1.62 similar to 0.51 at 2 \textless z less than or similar to 4) combined with a density evolution ( (1 + z)-0.57 +/- 0.22 up to z similar to 1 and. (1 + z)-3.92 +/- 0.34 at 1 \textless z less than or simi...
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