All MAST catalog holdings are available via a ConeSearch endpoint.
The Very Large Array (VLA) FIRST -- Faint Images of the Radio Sky at Twenty-cm -- is a project designed to produce the radio equivalent of the Palomar Observatory Sky Survey over 10,000 square degrees of the North and South Galactic Caps. Using the NRAO Very Large Array (VLA) and an automated mapping pipeline, we produce images with 1.8" pixels, a typical rms of 0.15 mJy, and a resolution of 5". At the 1 mJy source detection threshold, there are ~90 sources per square degree, ~35% of which have resolved structure on scales from 2-30". 30% of the sources have counterparts in the Sloan Digital Sky Survey.
The VLA FIRST catalog at MAST was published December 17, 2014. More information is available at http://sundog.stsci.edu
All available missions are listed at http://archive.stsci.edu/vo/mast_services.html.
All MAST catalog holdings are available via Cone Search endpoints.
This service provides access to the MAST copy of the VST Atlas:
This survey is targeting 4500 square degrees of the Southern sky in five filters (U, V, R, I and Z) to depths comparable to those of the SDSS. This survey is also complemented by near-infrared data from the VISTA Hemisphere Survey. The primary aim is to examine ‘baryon wiggles’ (small-amplitude oscillations observed in the power spectrum of galaxies) by looking at luminous red galaxies in order to determine the dark energy equation of state. Along with this, the VST ATLAS will provide an imaging base for spectroscopic surveys by the VLT.
All available missions are listed at http://archive.stsci.edu/vo/mast_services.html.
All MAST catalog holdings are available via Cone Search endpoints.
This service provides access to the MAST copy of the VST Kilo-degree Infrared Galaxy (VIKING) Survey
All available missions are listed at http://archive.stsci.edu/vo/mast_services.html.
All MAST catalog holdings are available via Cone Search endpoints.
This service provides access to the MAST copy of the VST Kilo-degree survey
All available missions are listed at http://archive.stsci.edu/vo/mast_services.html.
NASA's Wide-field Infrared Survey Explorer (WISE; Wright et al. 2010) mapped the sky at 3.4, 4.6, 12, and 22 μm (W1, W2, W3, W4) in 2010 with an angular resolution of 6.1", 6.4", 6.5", and 12.0" in the four bands. WISE achieved 5σ point source sensitivities better than 0.08, 0.11, 1 and 6 mJy in unconfused regions on the ecliptic in the four bands. Sensitivity improves toward the ecliptic poles due to denser coverage and lower zodiacal background.
The WISE All-Sky Release Source Catalog is mirrored at MAST and is thus available as a cone search.
All available catalogs are listed at http://archive.stsci.edu/vo/mast_services.html.
