Spitzer 70-micron Confusion Level

Details Spitzer 70-micron Confusion Level Spitzer 70-micron Confusion Level

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..381..260f&link_type=abstract

The Second Annual Spitzer Science Center Conference: Infrared Diagnostics of Galaxy Evolution. ASP Conference Series, Vol. 381,

Astronomy and Astrophysics

Astronomy

Scientific paper

Spitzer 70μm confusion measurements are presented based on ultra-deep MIPS-70μm observations of GOODS Hubble Deep Field North (HDF-N). 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 sigma_c = 0.30pm0.15 mJy for a limiting flux density of 1.5 mJy (q=5).

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