Search Publications

GOODS-Herschel: an infrared main sequence for star-forming galaxies
DOI: 10.1051/0004-6361/201117239 Bibcode: 2011A&A...533A.119E

Magnelli, B.; Lutz, D.; Altieri, B. +52 more

We present the deepest 100 to 500 µm far-infrared observations obtained with the Herschel Space Observatory as part of the GOODS-Herschel key program, and examine the infrared (IR) 3-500 µm spectral energy distributions (SEDs) of galaxies at 0 < z < 2.5, supplemented by a local reference sample from IRAS, ISO, Spitzer, and AKARI …

2011 Astronomy and Astrophysics
AKARI Herschel ISO eHST 1004
Extragalactic background light inferred from AEGIS galaxy-SED-type fractions
DOI: 10.1111/j.1365-2966.2010.17631.x Bibcode: 2011MNRAS.410.2556D

Barmby, P.; Cooper, M. C.; Huang, J. -S. +15 more

The extragalactic background light (EBL) is of fundamental importance both for understanding the entire process of galaxy evolution and for γ-ray astronomy, but the overall spectrum of the EBL between 0.1 and 1000 µm has never been determined directly from galaxy spectral energy distribution (SED) observations over a wide redshift range. The…

2011 Monthly Notices of the Royal Astronomical Society
AKARI 704
Defining the intrinsic AGN infrared spectral energy distribution and measuring its contribution to the infrared output of composite galaxies
DOI: 10.1111/j.1365-2966.2011.18448.x Bibcode: 2011MNRAS.414.1082M

Alexander, D. M.; Hickox, R. C.; Mullaney, J. R. +1 more

We use infrared spectroscopy and photometry to empirically define the intrinsic mid- to far-infrared spectral energy distribution (i.e. 6-100 µm SED) of thermal emission produced by typical (i.e. 2-10 keV luminosity, L2-10 keV∼ 1042-1044 erg s-1) active galactic nuclei (hereafter AGNs). The average…

2011 Monthly Notices of the Royal Astronomical Society
AKARI 365
The Tucana/Horologium, Columba, AB Doradus, and Argus Associations: New Members and Dusty Debris Disks
DOI: 10.1088/0004-637X/732/2/61 Bibcode: 2011ApJ...732...61Z

Zuckerman, B.; Song, Inseok; Bessell, M. S. +1 more

We propose 35 star systems within ~70 pc of Earth as newly identified members of nearby young stellar kinematic groups; these identifications include the first A- and late-B-type members of the AB Doradus moving group and field Argus Association. All but one of the 35 systems contain a bright solar- or earlier-type star that should make an excelle…

2011 The Astrophysical Journal
AKARI 227
Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey
DOI: 10.1093/pasj/63.5.1117 Bibcode: 2011PASJ...63.1117U

Oyabu, Shinki; Hasegawa, Sunao; Onaka, Takashi +10 more

We present the results of an unbiased asteroid survey in the mid-infrared wavelength region with the Infrared Camera (IRC) on board the Japanese infrared satellite AKARI. About 20% of the point source events recorded in the AKARI All-Sky Survey observations are not used for the IRC Point Source Catalog (IRC-PSC) in its production process because o…

2011 Publications of the Astronomical Society of Japan
AKARI 194
Modeling the evolution of infrared galaxies: a parametric backward evolution model
DOI: 10.1051/0004-6361/201015841 Bibcode: 2011A&A...529A...4B

Dole, H.; Lagache, G.; Béthermin, M. +2 more


Aims: We attempt to model the infrared galaxy evolution in as simple a way as possible and reproduce statistical properties such as the number counts between 15 µm and 1.1 mm, the luminosity functions, and the redshift distributions. We then use the fitted model to interpret observations from Spitzer, AKARI, BLAST, LABOCA, AzTEC, SPT, a…

2011 Astronomy and Astrophysics
AKARI Herschel 138
Mapping the radial structure of AGN tori
DOI: 10.1051/0004-6361/201117367 Bibcode: 2011A&A...536A..78K

Hönig, S. F.; Kishimoto, M.; Tristram, K. R. W. +3 more

We present mid-IR interferometric observations of six type 1 AGNs at multiple baseline lengths ranging from 27 m to 130 m, reaching high angular resolutions up to λ/B ~ 0.02 arcsec. For two of the targets, we have simultaneous near-IR interferometric measurements as well, taken within a week. We find that all the objects are partially resolved at …

2011 Astronomy and Astrophysics
AKARI 135
MESS (Mass-loss of Evolved StarS), a Herschel key program
DOI: 10.1051/0004-6361/201015829 Bibcode: 2011A&A...526A.162G

Ivison, R. J.; Blommaert, J. A. D. L.; Olofsson, G. +39 more

MESS (Mass-loss of Evolved StarS) is a guaranteed time key program that uses the PACS and SPIRE instruments on board the Herschel space observatory to observe a representative sample of evolved stars, that include asymptotic giant branch (AGB) and post-AGB stars, planetary nebulae and red supergiants, as well as luminous blue variables, Wolf-Rayet…

2011 Astronomy and Astrophysics
AKARI Herschel ISO 122
Evidence for an FU Orionis-like Outburst from a Classical T Tauri Star
DOI: 10.1088/0004-637X/730/2/80 Bibcode: 2011ApJ...730...80M

Filippenko, Alexei V.; Cenko, S. Bradley; Law, Nicholas M. +28 more

We present pre- and post-outburst observations of the new FU Orionis-like young stellar object PTF 10qpf (also known as LkHα 188-G4 and HBC 722). Prior to this outburst, LkHα 188-G4 was classified as a classical T Tauri star (CTTS) on the basis of its optical emission-line spectrum superposed on a K8-type photosphere and its photometric variabilit…

2011 The Astrophysical Journal
AKARI 96
Planck early results. XXII. The submillimetre properties of a sample of Galactic cold clumps
DOI: 10.1051/0004-6361/201116481 Bibcode: 2011A&A...536A..22P

Kneissl, R.; Miville-Deschênes, M. -A.; Boulanger, F. +201 more

We perform a detailed investigation of sources from the Cold Cores Catalogue of Planck Objects (C3PO). Our goal is to probe the reliability of the detections, validate the separation between warm and cold dust emission components, provide the first glimpse at the nature, internal morphology and physical characterictics of the Planck-detected sourc…

2011 Astronomy and Astrophysics
AKARI Herschel Planck 95