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Resource Record Summary

Image Service:
NEOWISE Post-Cryo L1b Images


http://wise2.ipac.caltech.edu/docs/release/allsky/expsup/wise_logo_sm.jpg[Logo URL]
Short name: WISE 2-Band L1b
IVOA Identifier: ivo://irsa.ipac/WISE/Images/Post-Cryo/L1bPublisher: NASA/IPAC Infrared Science Archiveivo://irsa.ipac/IRSA[Pub. ID]
More Info: http://wise2.ipac.caltech.edu/docs/release/allsky/expsup/sec8_1.html
VO Compliance: Level 2: This is a VO-compliant resource.
Status: active
Registered: 2015 Mar 26 02:04:00Z
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Description


The WISE 3-Band Cryo Data Release products are comprised of data taken during the mission's 3-Band Cryo survey phase. This phase covers the time following the exhaustion of solid hydrogen in the WISE payload outer cryogen tank, while the detectors and telescope were still cooled by the inner cryogen tank. During this time, WISE's W1, W2 and W3 bands were operational and continued to acquire useful data, but the W4 detector was saturated by thermal emission from the warming telescope. The sensitivity achieved in the W1 and W2 bands was similar to that during the full cryogenic mission phase. The W3 measurement sensitivity was degraded and decreased steadily during the 3-Band Cryo phase because of the increasing telescope temperature and decreasing exposure times. The NEOWISE Post-Cryo Data Release products were generated using data taken during the mission's Post-Cryo survey phase. This phase covers the time following the exhaustion of solid hydrogen in the WISE payload inner cryogen tank, when the detectors and optics gradually warmed until they reached a stable equilibrium temperature near 73.5 K (VIII.1.a.i). During this time, WISE's W1 and W2 detectors continued to acquire high quality imaging data with sensitivities close to that during the mission's cryogenic survey phases. The W3 and W4 detectors were fully saturated by the thermal emission from the warming telescope. WISE scanned approximately 70% of the sky during the Post-Cryo survey phase continuing with the same strategy that was used during the full cryogenic survey. WISE scanned along lines of constant ecliptic longitude from near one ecliptic pole to near the other pole with a scan rate close to the orbital rate of 3.8 arc-minutes/second in order to always point away from the Earth. Each semi-circular track from ecliptic pole to ecliptic pole is called a scan. During each scan WISE took a frameset every 11 seconds. Each Post-Cryo frameset contains two images, one for each of the W1 and W2 bands, both observing the same 47x47 arc-minute square patch of sky.

More About this Resource

About the Resource Providers

This section describes who is responsible for this resource

Publisher: NASA/IPAC Infrared Science Archiveivo://irsa.ipac/IRSA[Pub. ID]

Creator: WISE team Contributor: IPAC, UCLA, JPL/Caltech

Contact Information:
X IRSA Support Team
Email: irsasupport at ipac.caltech.edu
Address:

Status of This Resource

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

Version: n/a
Availability: This is an active resource.
  • This service apparently provides only public data
Relevant dates for this Resource:
  • Creation: 2013 May 20

This resource was registered on: 2015 Mar 26 02:04:00Z
This resource description was last updated on: 2017 Mar 16 01:00:00Z

What This Resource is About

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

Resource Class: CatalogService
This resource is a service that provides access to data (specifically, images). With this type of service, you can search for data by issuing a query, and information about available data is returned as a table.
Resource type keywords:
  • Survey
Subject keywords:
  • sky survey
Intended audience or use:
  • Research: This resource provides information appropriate for supporting scientific research.
More Info: http://wise2.ipac.caltech.edu/docs/release/allsky/expsup/sec8_1.html

Data Coverage Information

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

Wavebands covered:

  • Infrared

Available Service Interfaces

Simple Image AccessXX

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

VO Compliance: Level 2: This is a VO-compliant resource.
Available endpoints for the standard interface:
  • https://irsa.ipac.caltech.edu/ibe/sia/wise/postcryo/2band_p1bm_frm?X(version compatible)
Image service type: Atlas: pre-computed survey images will be returned.
Maximum query region accepted: longitude: 1.0 degrees; latitude: 1.0 degrees
Maximum region size returned: longitude: 0.776 degrees; latitude: 0.776 degrees
Maximum image size returned: 1016 X 1016 pixels
Maximum image size returned: 2 GB
Maximum number of matching records returned: 2147483647


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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