Power Spectrum Analysis of Far-IR Background Fluctuations in Spitzer Maps at 160 Microns

Loading...
Thumbnail Image

Date

Journal Title

Journal ISSN

Volume Title

Publisher

Abstract

Description

We describe data reduction and analysis of fluctuations in the Cosmic Far-IR Background (CFIB) in large maps observed with the Multiband Imaging Photometer for Spitzer (MIPS) instrument 160 micron detectors. We analyzed the extragalactic First Look Survey (FLS) and the Spitzer Wide-area Infrared Extragalactic Survey (SWIRE) Lockman Hole observations, the latter being the largest low-cirrus mapping observation available. In the Lockman Hole map, we measured the power spectrum of the CFIB by fitting a power law to the IR cirrus component, the dominant foreground contaminant, and subtracting this cirrus signal. The CFIB power spectrum at mid-high k (k ~ 0.2 - 0.5 arc min^-1) is consistent with previous measurements of a relatively flat component. At lower k, however, the power spectrum is clearly not flat, decreasing from our lowest frequencies (k ~ 0.03 arc min^-1) and flattening at mid-frequencies (k ~ 0.1 - 0.2 arc min^-1). This behavior is consistent with the gross characteristics of predictions of a source clustering signature in CFIB power spectra, and this is the first report of such a detection.
Please download the superior-quality, single file PDF, see additional figures of higher quality, and look for updates at http://www-astro.lbl.gov/~bruce/spitzerpaper1/ .(This version has submission text, but not submission graphics.)

Keywords

Citation

Collections