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Paper: Spitzer 70-micron Confusion Level
Volume: 381, The Second Annual Spitzer Science Center Conference: Infrared Diagnostics of Galaxy Evolution
Page: 260
Authors: Frayer, D.T.; Huynh, M.T.
Abstract: Spitzer 70μm confusion measurements are presented based on ultra-deep MIPS-70μm observations of GOODS Hubble Deep Field North (HDFN). The instrument noise for the MIPS-70μm band integrates down with nearly t−0.5 for the low background HDF-N field. The estimated confusion level is σc = 0.30 ± 0.15mJy for a limiting flux density of 1.5mJy (q = 5).
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