Confusion of extragalactic sources in the mid- and far-infrared:: Spitzer and beyond

被引：97

作者：

Dole, H

Rieke, GH

Lagache, G

Puget, JL

Alonso-Herrero, A

Bai, L

Blaylock, M

Egami, E

Engelbracht, CW

Gordon, KD

Hines, DC

Kelly, DM

Le Floc'h, E

Misselt, KA

Morrison, JE

Muzerolle, J

Papovich, C

Perez-Gonzalez, PG

Rieke, MJ

Rigby, JR

Neugebauer, G

Stansberry, JA

Su, KYL

Young, ET

Beichman, CA

Richards, PL

机构：

[1] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA

[2] Univ Paris 11, Inst Astrophys Spatiale, F-91405 Orsay, France

[3] Space Sci Inst, Boulder, CO 80301 USA

[4] CALTECH, Michelson Sci Ctr, Pasadena, CA 91125 USA

[5] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA

来源：

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES | 2004年 / 154卷 / 01期

关键词：

galaxies : evolution; galaxies : statistics; infrared : galaxies;

D O I：

10.1086/422690

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We use the source counts measured with the Multiband Imaging Photometer for Spitzer at 24, 70, and 160 mum to determine the 5 sigma confusion limits due to extragalactic sources: 56 muJy, 3.2 mJy, and 40 mJy at 24, 70, and 160 mum, respectively. We also make predictions for confusion limits for a number of proposed far-infrared missions of larger aperture (3.5 - 10 m diameter).

引用

页码：93 / 96

页数：4

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