Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/40516
Title: Herschel unveils a puzzling uniformity of distant dusty galaxies
Authors: Elbaz, D
Hwang, HS
Magnelli, B
Daddi, E
Aussel, H
Altieri, B
Amblard, A
Andreani, P
Arumugam, V
Auld, R
Babbedge, T
Berta, S
Blain, Andrew W.
Bock, J
Bongiovanni, A
Boselli, A
Buat, V
Burgarella, D
Castro-Rodriguez, N
Cava, A
Cepa, J
Chanial, P
Chary, R-R
Cimatti, A
Clements, DL
Conley, A
Conversi, L
Cooray, A
Dickinson, M
Dominguez, H
Dowell, CD
Dunlop, JS
Dwek, E
Eales, S
Farrah, D
Förster Schreiber, N
Fox, M
Franceschini, A
Gear, W
Genzel, R
Glenn, J
Griffin, M
Gruppioni, C
Halpern, M
Hatziminaoglou, E
Ibar, E
Isaak, K
Ivison, RJ
Lagache, G
Le Borgne, D
Le Floc h, E
Levenson, L
Lu, N
Lutz, D
Madden, S
Maffei, B
Magdis, G
Mainetti, G
Maiolino, R
Marchetti, L
Mortier, AMJ
Nguyen, HT
Nordon, R
O Halloran, B
Okumura, K
Oliver, SJ
Omont, A
Page, MJ
Panuzzo, P
Papageorgiou, A
Pearson, CP
Perez Fournon, I
Pérez García, AM
Poglitsch, A
Pohlen, M
Popesso, P
Pozzi, F
Rawlings, JI
Rigopoulou, D
Riguccini, L
Rizzo, D
Rodighiero, G
Roseboom, IG
Rowan-Robinson, M
Saintonge, A
Sanchez Portal, M
Santini, P
Sauvage, M
Schulz, B
Scott, D
Seymour, N
Shao, L
Shupe, DL
Smith, AJ
Stevens, JA
Sturm, E
Symeonidis, M
Tacconi, L
Trichas, M
Tugwell, KE
Vaccari, M
Valtchanov, I
Vieira, J
Vigroux, L
Wang, L
Ward, R
Wright, G
Xu, CK
Zemcov, M
First Published: 16-Jul-2010
Publisher: EDP Sciences for European Southern Observatory (ESO)
Citation: Astronomy and Astrophysics, 2010, 518, L29
Abstract: The Herschel Space Observatory enables us to accurately measure the bolometric output of starburst galaxies and active galactic nuclei (AGN) by directly sampling the peak of their far-infrared (IR) emission. Here we examine whether the spectral energy distribution (SED) and dust temperature of galaxies have strongly evolved over the last 80% of the age of the Universe. We discuss possible consequences for the determination of star-formation rates (SFR) and any evidence for a major change in their star-formation properties. We use Herschel deep extragalactic surveys from 100 to 500 μm to compute total IR luminosities in galaxies down to the faintest levels, using PACS and SPIRE in the GOODS-North field (PEP and HerMES key programs). An extension to fainter luminosities is done by stacking images on 24 μm prior positions. We show that measurements in the SPIRE bands can be used below the statistical confusion limit if information at higher spatial resolution is used, e.g. at 24 μm, to identify “isolated” galaxies whose flux is not boosted by bright neighbors. Below z ~ 1.5, mid-IR extrapolations are correct for star-forming galaxies with a dispersion of only 40% (0.15 dex), therefore similar to z ~ 0 galaxies, over three decades in luminosity below the regime of ultra-luminous IR galaxies (ULIRGs, LIR ≥ 1012 ). This narrow distribution is puzzling when considering the range of physical processes that could have affected the SED of these galaxies. Extrapolations from only one of the 160 μm, 250 μm or 350 μm bands alone tend to overestimate the total IR luminosity. This may be explained by the lack of far-IR constraints around and above ~150 μm (rest-frame) before Herschel on those templates. We also note that the dust temperature of luminous IR galaxies (LIRGs, LIR ≥ 1011 ) around z ~ 1 is mildly colder by 10–15% than their local analogs and up to 20% for ULIRGs at z ~ 1.6 (using a single modified blackbody-fit to the peak far-IR emission with an emissivity index of β = 1.5). Above z = 1.5, distant galaxies are found to exhibit a substantially larger mid- over far-IR ratio, which could either result from stronger broad emission lines or warm dust continuum heated by a hidden AGN. Two thirds of the AGNs identified in the field with a measured redshift exhibit the same behavior as purely star-forming galaxies. Hence a large fraction of AGNs harbor coeval star formation at very high SFR and in conditions similar to purely star-forming galaxies.
DOI Link: 10.1051/0004-6361/201014687
ISSN: 0004-6361
eISSN: 1432-0746
Links: https://www.aanda.org/articles/aa/abs/2010/10/aa14687-10/aa14687-10.html
http://hdl.handle.net/2381/40516
Version: Post-print
Status: Peer-reviewed
Type: Journal Article
Rights: Copyright © 2010, ESO. Deposited with reference to the publisher’s open access archiving policy.
Description: archiveprefix: arXiv primaryclass: astro-ph.CO keywords: galaxies: evolution, galaxies: active, galaxies: starburst, infrared: galaxies eid: L29 adsurl: http://adsabs.harvard.edu/abs/2010A%26A...518L..29E adsnote: Provided by the SAO/NASA Astrophysics Data System
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

Files in This Item:
File Description SizeFormat 
1005.2859v1.pdfPost-review (final submitted author manuscript)545.38 kBAdobe PDFView/Open


Items in LRA are protected by copyright, with all rights reserved, unless otherwise indicated.