SkyView Usage Patterns
Figures from SkyView: A Decade with the Virtual Telescope,
a paper presented at the American Astronomical Society meeting in Seattle, WA in January 2004.
Usage plots

This plot shows steady growth over the past 7 years with a large rise this past year after the installation of new hardware and with the selection as a Scientific American SciTech web site.
(The drop in 1997 is due to a gap in data collection)

This usage plot shows diurnal variations and a drop on weekends.
Percentage of SkyView requests by wavelength

Obviously, optical surveys are the most popular.
Logarithmic densities of all requested image center locations (galactic coordinates)
(Click for larger image)

Locations of all requested image centers (galactic coordinates)
(Click for larger image)
Image center locations by wavelength
These plots show the number of locations requested and areas of interest for
each wavelength
(Click for larger image)
 Gamma-ray |
 X-ray |
 EUV |
 UV |
 Optical |
 Infrared |
 Radio |
Density of image center locations by wavelength
These plots show the density (logarithmic) of images at requested locations for each wavelength
(Click for larger image)
 Gamma-ray |
 X-ray |
 EUV |
 UV |
 Optical |
 Infrared |
 Radio |
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SkyView has been developed with generous support from the NASA AISR
and ADP programs (P.I. Thomas A. McGlynn)
under the auspices of the High Energy
Astrophysics Science Archive Research Center (HEASARC) at the NASA/
GSFC
Astrophysics Science Division.
We gratefully acknowledge the support of NASA and contributors
of SkyView surveys.