2 SEP-M70PSC ivo://irsa.ipac/Spitzer/Catalog/SEP/SEP-M70PSC NASA/IPAC Infrared Science Archive Scott et al. 2011-05-19 IRSA Support Team

irsasupport@ipac.caltech.edu extragalactic survey 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). Source detection and photometry were performed using the APEX software within the MOPEX package. Source candidates with S/N > 6 and reduced chi-squared values less than or equal to three (93% of the sources) are considered reliable detections. The remaining source candidates were then inspected (see Scott et al. 2010 for details) and false positives were removed from the catalog. https://irsa.ipac.caltech.edu/data/SPITZER/SEP/gator_docs/SEPM70_colDescriptions.html Catalog Research derived-from Spitzer MIPS 24 and 70 micron Imaging of the South Ecliptic Pole served-by IRSA TAP service 2 https://irsa.ipac.caltech.edu/SCS?table=sepm70& 180 2147483647 false 67.286527 -55.437514 0.0028 2 To access this resource via TAP, issue ADQL queries on the table named sepm70. https://irsa.ipac.caltech.edu/TAP 2 https://irsa.ipac.caltech.edu/cgi-bin/Gator/nph-dd?catalog=sepm70 Infrared spitzer Spitzer South Ecliptic Pole (SEP) sepm70Spitzer South Ecliptic Pole MIPS 70 micron Point Source Catalog