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The Herschel PEP/HerMES Luminosity Function. I: Probing the Evolution of PACS selected Galaxies to z~4

Authors :
V. Arumugam
Ismael Perez-Fournon
M. Bethermin
Andreas Papageorgiou
Alberto Franceschini
Mattia Vaccari
A. M. Pérez García
Lucia Pozzetti
G. Wright
B. O'Halloran
P. Chanial
Giulia Rodighiero
Pierluigi Monaco
P. Popesso
E. Zucca
Michael Pohlen
Benjamin Magnelli
K. G. Isaak
Lucia Marchetti
Eckhard Sturm
Bruno Maffei
Michael Rowan-Robinson
Matthew Joseph Griffin
Michael Zemcov
Marco Scodeggio
C. K. Xu
Lian-Tao Wang
Antonio Cava
O. Le Fevre
K. E. Tugwell
M. Magliocchetti
Dimitra Rigopoulou
Albrecht Poglitsch
S. C. Madden
Bruno Altieri
Raanan Nordon
M. Carollo
Rob Ivison
Alexandre Amblard
N. Castro-Rodríguez
R. Genzel
James J. Bock
Vincenzo Mainieri
Linda J. Tacconi
Alvio Renzini
Anthony J. Smith
Francesca Pozzi
David J. Rosario
Chris Pearson
Mark Sargent
A. Boselli
Denis Burgarella
G. Mainetti
Edo Ibar
C. D. Dowell
Ivan Delvecchio
H. Aussel
A. Conley
Benjamin L. Schulz
Simon J. Lilly
Jamie Stevens
H. T. Nguyen
V. Buat
Guilaine Lagache
D. Elbaz
Nick Seymour
Asantha Cooray
Alessandro Cimatti
Douglas Scott
M. J. Page
Louis Levenson
M. Sánchez-Portal
Evanthia Hatziminaoglou
David L. Clements
Nanyao Y. Lu
M. Symeonidis
S. Berta
L. Riguccini
L. Vigroux
Ivan Valtchanov
Emanuele Daddi
Roberto Maiolino
Eli Dwek
J. Cepa
Stephen Anthony Eales
H. Dominguez-Sanchez
G. Zamorani
Dieter Lutz
P. Panuzzo
S. Bardelli
D. L. Shupe
Carlotta Gruppioni
E. Le Floc'h
Isaac Roseboom
Seb Oliver
Ángel Bongiovanni
P. Andreani
Alvaro Iribarrem
Thierry Contini
N. M. Foerster Schreiber
Jason Glenn
Markos Trichas
O. Ilbert
C., Gruppioni
F., Pozzi
G., Rodighiero
I., Delvecchio
S., Berta
L., Pozzetti
G., Zamorani
P., Andreani
A., Cimatti
O., Ilbert
E., Le Floc'h
D., Lutz
B., Magnelli
L., Marchetti
Monaco, Pierluigi
R., Nordon
S., Oliver
P., Popesso
L., Riguccini
I., Roseboom
D. J., Rosario
M., Sargent
M., Vaccari
B., Altieri
H., Aussel
A., Bongiovanni
J., Cepa
E., Daddi
H., Dominguez Sanchez
D., Elbaz
N., Forster Schreiber
R., Genzel
A., Iribarrem
M., Magliocchetti
R., Maiolino
A., Poglitsch
A., Perez Garcia
M., Sanchez Portal
E., Sturm
L., Tacconi
I., Valtchanov
A., Amblard
V., Arumugam
M., Bethermin
J., Bock
A., Boselli
V., Buat
D., Burgarella
N., Castro Rodriguez
A., Cava
P., Chanial
D. L., Clement
A., Conley
A., Cooray
C. D., Dowell
E., Dwek
S., Eale
A., Franceschini
J., Glenn
M., Griffin
E., Hatziminaoglou
E., Ibar
K., Isaak
R. J., Ivison
G., Lagache
L., Levenson
N., Lu
S., Madden
B., Maffei
G., Mainetti
H. T., Nguyen
B., O'Halloran
M. J., Page
P., Panuzzo
A., Papageorgiou
C. P., Pearson
I., Perez Fournon
M., Pohlen
D., Rigopoulou
M., Rowan Robinson
B., Schulz
D., Scott
N., Seymour
D. L., Shupe
A. J., Smith
J. A., Steven
M., Symeonidi
M., Tricha
K. E., Tugwell
L., Vigroux
L., Wang
G., Wright
C. K., Xu
M., Zemcov
S., Bardelli
M., Carollo
T., Contini
O., Le Fevre
S., Lilly
V., Mainieri
A., Renzini
M., Scodeggio
E., Zucca
C. Gruppioni
F. Pozzi
G. Rodighiero
I. Delvecchio
S. Berta
L. Pozzetti
G. Zamorani
P. Andreani
A. Cimatti
O. Ilbert
E. Le Floc'h
D. Lutz
B. Magnelli
L. Marchetti
P. Monaco
R. Nordon
S. Oliver
P. Popesso
L. Riguccini
I. Roseboom
D. J. Rosario
M. Sargent
M. Vaccari
B. Altieri
H. Aussel
A. Bongiovanni
J. Cepa
E. Daddi
H. Dominguez-Sanchez
D. Elbaz
N. Forster Schreiber
R. Genzel
A. Iribarrem
M. Magliocchetti
R. Maiolino
A. Poglitsch
A. Perez Garcia
M. Sanchez-Portal
E. Sturm
L. Tacconi
I. Valtchanov
A. Amblard
V. Arumugam
M. Bethermin
J. Bock
A. Boselli
V. Buat
D. Burgarella
N. Castro-Rodriguez
A. Cava
P. Chanial
D. L. Clement
A. Conley
A. Cooray
C. D. Dowell
E. Dwek
S. Eale
A. Franceschini
J. Glenn
M. Griffin
E. Hatziminaoglou
E. Ibar
K. Isaak
R. J. Ivison
G. Lagache
L. Levenson
N. Lu
S. Madden
B. Maffei
G. Mainetti
H. T. Nguyen
B. O'Halloran
M. J. Page
P. Panuzzo
A. Papageorgiou
C. P. Pearson
I. Perez-Fournon
M. Pohlen
D. Rigopoulou
M. Rowan-Robinson
B. Schulz
D. Scott
N. Seymour
D. L. Shupe
A. J. Smith
J. A. Steven
M. Symeonidi
M. Tricha
K. E. Tugwell
L. Vigroux
L. Wang
G. Wright
C. K. Xu
M. Zemcov
S. Bardelli
M. Carollo
T. Contini
O. Le Fevre
S. Lilly
V. Mainieri
A. Renzini
M. Scodeggio
E. Zucca
Source :
E-Prints Complutense. Archivo Institucional de la UCM, instname, E-Prints Complutense: Archivo Institucional de la UCM, Universidad Complutense de Madrid
Publication Year :
2013
Publisher :
arXiv, 2013.

Abstract

We exploit the deep and extended far infrared data sets (at 70, 100 and 160 um) of the Herschel GTO PACS Evolutionary Probe (PEP) Survey, in combination with the HERschel Multi tiered Extragalactic Survey (HerMES) data at 250, 350 and 500 um, to derive the evolution of the restframe 35 um, 60 um, 90 um, and total infrared (IR) luminosity functions (LFs) up to z~4. We detect very strong luminosity evolution for the total IR LF combined with a density evolution. In agreement with previous findings, the IR luminosity density increases steeply to z~1, then flattens between z~1 and z~3 to decrease at z greater than 3. Galaxies with different SEDs, masses and sSFRs evolve in very different ways and this large and deep statistical sample is the first one allowing us to separately study the different evolutionary behaviours of the individual IR populations contributing to the IR luminosity density. Galaxies occupying the well established SFR/stellar mass main sequence (MS) are found to dominate both the total IR LF and luminosity density at all redshifts, with the contribution from off MS sources (0.6 dex above MS) being nearly constant (~20% of the total IR luminosity density) and showing no significant signs of increase with increasing z over the whole 0.8<br />Comment: 32 pages, 20 figures, 9 tables. Published in MNRAS. Replaced Fig. 8 (small scaling bug in the previous version)

Details

ISSN :
00358711
Database :
OpenAIRE
Journal :
E-Prints Complutense. Archivo Institucional de la UCM, instname, E-Prints Complutense: Archivo Institucional de la UCM, Universidad Complutense de Madrid
Accession number :
edsair.doi.dedup.....c5d7cc70c7ac7880301e3887ab85057c
Full Text :
https://doi.org/10.48550/arxiv.1302.5209