TY - JOUR
T1 - Nature of infrared sources in 11 μm selected sample from early data of the AKARI north ecliptic pole deep survey
AU - Lee, Hyung Mok
AU - Im, Myungshin
AU - Wada, Takehiko
AU - Shim, Hyunjin
AU - Kim, Seong Jin
AU - Lee, Myung Gyoon
AU - Hwang, Narae
AU - Matsuhara, Hideo
AU - Nakagawa, Takao
AU - Oyabu, Shinki
AU - Pearson, Chris P.
AU - Takagi, Toshinobu
AU - Onaka, Takashi
AU - Fujishiro, Naofumi
AU - Hanami, Hitoshi
AU - Ishihara, Daisuke
AU - Ita, Yoshifusa
AU - Kataza, Hirokazu
AU - Kim, Woojung
AU - Matusmoto, Toshio
AU - Murakami, Hiroshi
AU - Ohyama, Youichi
AU - Sakon, Itsuki
AU - Tanabé, Toshihiko
AU - Uemizu, Kazunori
AU - Ueno, Munetaka
AU - Usui, Fumihiko
AU - Watarai, Hidenori
PY - 2007
Y1 - 2007
N2 - We present the properties of 11 μm selected sources detected in the early data of the North Ecliptic Pole Deep (NEP-Deep) Survey of AKARI. The data set covers 6 wavelength bands from 2.5 to 11 μm, with exposure times of 10-20 minutes. This field lies within the CFHT survey with four filter bands (g′, r′, i′, z′), enabling us to establish nearly continuous spectral energy distributions (SEDs) for wavelengths ranging from 0.4 to 11 μm. The main sample studied here consists of 72 sources whose 11 μm AB magnitudes are equal to or brighter than 18.5 (144 μJy), which is complete to more than 90%. The 11 μm band has an advantage of sampling star-forming galaxies with low-to-medium redshifts, since the prominent PAH feature shifts into this band. As expected, we find that the majority (71%) of 11 μm bright sources are star-forming galaxies at 0.2 ≲ z ≲ 0.7 with LIR ∼ 1010-1012 L⊙ based on detailed modelling of the SEDs. We also find four AGNs lying at various redshifts in the main sample. In addition, we discuss a few sources that have non-typical SEDs of the main sample, including a brown-dwarf candidate, a steep power-law source, a flat-spectrum object, and an early-type galaxy at moderate redshift.
AB - We present the properties of 11 μm selected sources detected in the early data of the North Ecliptic Pole Deep (NEP-Deep) Survey of AKARI. The data set covers 6 wavelength bands from 2.5 to 11 μm, with exposure times of 10-20 minutes. This field lies within the CFHT survey with four filter bands (g′, r′, i′, z′), enabling us to establish nearly continuous spectral energy distributions (SEDs) for wavelengths ranging from 0.4 to 11 μm. The main sample studied here consists of 72 sources whose 11 μm AB magnitudes are equal to or brighter than 18.5 (144 μJy), which is complete to more than 90%. The 11 μm band has an advantage of sampling star-forming galaxies with low-to-medium redshifts, since the prominent PAH feature shifts into this band. As expected, we find that the majority (71%) of 11 μm bright sources are star-forming galaxies at 0.2 ≲ z ≲ 0.7 with LIR ∼ 1010-1012 L⊙ based on detailed modelling of the SEDs. We also find four AGNs lying at various redshifts in the main sample. In addition, we discuss a few sources that have non-typical SEDs of the main sample, including a brown-dwarf candidate, a steep power-law source, a flat-spectrum object, and an early-type galaxy at moderate redshift.
KW - Galaxies: active
KW - Galaxies: evolution
KW - Galaxies: formation
KW - Infrared: galaxies
KW - Stars: low-mass, brown dwarfs
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U2 - 10.1093/pasj/59.sp2.s529
DO - 10.1093/pasj/59.sp2.s529
M3 - Review article
AN - SCOPUS:36849022186
VL - 59
SP - S529-S542
JO - Publications of the Astronomical Society of Japan
JF - Publications of the Astronomical Society of Japan
SN - 0004-6264
IS - SPEC. ISS. 2
ER -