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Cited article:

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The Astrophysical Journal 862 (1) 77 (2018)
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IDENTIFICATION OF A COMPLETE 160 μm FLUX-LIMITED SAMPLE OF INFRARED GALAXIES IN THEISOLOCKMAN HOLE 1 deg2DEEP FIELDS: SOURCE PROPERTIES AND EVIDENCE FOR STRONG EVOLUTION IN THE FIR LUMINOSITY FUNCTION FOR ULIRGs

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DETECTION OF THE COSMIC FAR-INFRARED BACKGROUND IN AKARI DEEP FIELD SOUTH

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The Astrophysical Journal 737 (1) 2 (2011)
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Stellar population and dust extinction in an ultraluminous infrared galaxy at z= 1.135

K. Kawara, S. Oyabu, Y. Matsuoka, et al.
Monthly Notices of the Royal Astronomical Society 402 (1) 335 (2010)
https://doi.org/10.1111/j.1365-2966.2009.15873.x

Determination of the cosmic far-infrared background level with the ISOPHOT instrument

M. Juvela, K. Mattila, D. Lemke, et al.
Astronomy & Astrophysics 500 (2) 763 (2009)
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AKARI Far-Infrared Source Counts in the Lockman Hole

Shuji Matsuura, Mai Shirahata, Mitsunobu Kawada, Yasuo Doi, Takao Nakagawa, Hiroshi Shibai, Chris P. Pearson, Toshinobu Takagi, Woong-Seob Jeong, Shinki Oyabu and Hideo Matsuhara
Publications of the Astronomical Society of Japan 59 (sp2) S503 (2007)
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Far‐infrared Source Counts at 70 and 160 Microns in Spitzer Deep Surveys

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The Astrophysical Journal Supplement Series 154 (1) 87 (2004)
https://doi.org/10.1086/422472