The Subaru Seminar is
usually held in Room 104 of the Hilo Base Facility, adjacent
to the main lobby. Everyone is welcome to attend. If you are
interested in giving a seminar, please contact Subaru seminar organizers
(Tadayuki Kodama, Nagayoshi Ohashi, Tomonori Usuda)
by email : sseminar_at_subaru.naoj.org (please change"_at_" to @).
Jun 25, Monday, at 3:00 pm
" Cosmic star formation history and AGN evolution near and far: AKARI reveals both "
(University of Copenhagen)
Understanding infrared (IR) luminosity is fundamental to understanding the cosmic star formation history and AGN evolution,
since their most intense stages are often obscured by dust.
Japanese infrared satellite, AKARI, provided unique data sets to probe
this both at low and high redshift; the AKARI all sky survey in 6
bands (9-160um), and the AKARI NEP Deep survey in 9 bands (2-24um).
The AKARI performed all sky survey in 6 IR bands (9, 18, 65, 90,
140, and 160um) with 3-10 times better sensitivity than IRAS, covering
the crucial far-IR wavelengths across the peak of the dust emission.
Combined with a better spatial resolution, AKARI can much more
precisely measure the total infrared luminosity (L_TIR) of individual
galaxies, and thus, the total infrared luminosity density of the local
In the AKARI NEP deep field, we construct restframe 8um, 12um, and
total infrared (TIR) luminosity functions (LFs) at 0.15
# Infrared Luminosity Functions of AKARI-SDSS Galaxies
Goto, T. et al. 2011, MNRAS, 414, 1903
# Luminosity Functions of Local Infrared Galaxies Revisited:
Implications to the Cosmic
Star Formation History and AGN Evolution
Goto, T. et al. 2011, MNRAS, 410,5 73
# Evolution of Infrared Luminosity functions of Galaxies in the AKARI
Revealing the cosmic star formation history hidden by dust
Goto, T. et al. 2010, A&A, 514A, 6
# Environmental dependence of 8um luminosity functions of galaxies at z~0.8
Comparison between RXJ1716.4+6708 and the AKARI NEP deep field.
Goto, T. , et al., 2010, A&A, 514A,7
Seminars are also held at JAC,