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Resource Record Summary

Image Service:
Spitzer MIPS 24 and 70 micron Imaging of the South Ecliptic Pole

Short name: SEP
IVOA Identifier: ivo://irsa.ipac/Spitzer/Images/SEPPublisher: NASA/IPAC Infrared Science Archive[+][Pub. ID]
More Info: https://irsa.ipac.caltech.edu/data/SPITZER/SEP
VO Compliance: Level 2: This is a VO-compliant resource.
Status: active
Registered: 2014 Oct 28 17:31:00Z
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Description


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).

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[+] About the Resource Providers

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[+] Status of This Resource

This section provides some status information: the resource version, availability, and relevant dates.

[+] What This Resource is About

This section describes what the resource is, what it contains, and how it might be relevant.

[+] Data Coverage Information

This section describes the data's coverage over the sky, frequency, and time.

Available Service Interfaces

[+] Simple Image Access (version 2.0)XX

This is a standard IVOA service used to search for images from this resource that overlap with a specified region of the sky.

[+] Custom Service

This is service that does not comply with any IVOA standard but instead provides access to special capabilities specific to this resource.



Developed with the support of the National Science Foundation
under Cooperative Agreement AST0122449 with the Johns Hopkins University
The NAVO project is a member of the International Virtual Observatory Alliance

This NAVO Application is hosted by the Space Telescope Science Institute

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