A Complete 16 micron-Selected Galaxy Sample at $z\sim1$: Mid-infrared Spectral Energy Distributions.

J. S. Huang,Y.S. Dai,S. P. Willner,S. M. Faber,Cheng Cheng,H. Xu,Shumei Wu,Xu Shao,C Hao,X. Xia,Dimitra Rigopoulou,M. Pereira-Santaella,Georgios E. Magdis,Isabella Cortzen,Haojing Yan,G. G. Fazio,P. Assmann,N. Araneda,L. Fan,M. Musin,Zhong Wang,K.C. Xu,C. He,E. Esamdin

A Complete 16 micron-Selected Galaxy Sample at $z\sim1$: Mid-infrared Spectral Energy Distributions.

2021

We describe a complete, flux-density-limited sample of galaxies at redshift $0.8 $10$^{11}$\,\Msun\ are unlikely to host an AGN. About 1% of the sample galaxies show an SED with dust emission typical of neither star formation nor an AGN.

Keywords:

dust emission
Spectral density
Astrophysics
Physics
Galaxy
Micrometre
Star formation
mid infrared
Redshift

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