Spitzer MIPS 24 and 70 micron Imaging of the South Ecliptic Pole (SEP)
The
Spitzer/
MIPS 24 and 70 μm imaging of an 11.5 square degree region near the South Ecliptic Pole (SEP) has been carried out in order to complement sub-millimeter wavelength observations (250-500 μm) of the same region of sky taken with the Balloon-borne Large Aperture Sub-millimeter Telescope (
BLAST), with the goal of better characterizing the nature of sub-millimeter selected galaxies and their role in galaxy evolution. This field has also been extensively mapped at other wavelengths, and will be imaged from 100-500 μm as part of the Herschel Multi-tiered Extragalactic Survey (
HerMES).
Use the form below to enter a coordinate or
object name to search for data, or click the image above to retrieve cutout images for your area of interest (along with links to the original mosaics). You can also bypass searching and browse the
images and
catalogs.
Also available are SEP image "cutouts" using IRSA's
Cutouts Service, which is a general tool to
create single or multiple small FITS (and JPEG) image cutouts of data sets archived at IRSA.
Access all the Spitzer Legacy datasets at IRSA.
Access BLAST data at IRSA.
