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[[File:milkyway.png|400px|thumb|right|The Galactic Center, from Paranal (Credit:ESO)]]
[[File:milkyway.png|400px|thumb|right|The Galactic Center, from Paranal (Credit:ESO)]]
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What is the structure of the inner Galactic bulge? How did the Milky Way form? Thanks to [[VISTA Telescope | VISTA]], a 4.1 meter telescope, and its superb near-infrared camera VIRCAM, new observations can be done to help the astronomers to further answer these questions.
+
What is the structure of the inner Galactic bulge? How did the Milky Way form? Thanks to [[VISTA Telescope | VISTA]], a 4.1 meter telescope, and its superb near-infrared camera VIRCAM, new observations can be done to help astronomers to further answer these questions.
-
Even when the Milky Way can be observed by the naked eye from dark places at night, because of our position on the Galaxy we can actually only see our  nearest neighborhood: dust, gas, and the other stars block the light from other places of our galaxy and we can't observe far into the bulge. At least in the "visual" part of the spectrum of the light.
+
Even when the Milky Way can be observed by the naked eye from dark places at night, because of our position in the Galaxy, we can actually only see our  closest neighborhood. Dust, gas, and stars block the light from other places of our galaxy and thus we are not able to observe far into the bulge, at least in the "visual" part of the electromagnetic spectrum.
-
VISTA, the Visible and Infrared Survey Telescope for Astronomy, it is optimized to detect the near-infrared wavelengths of the light of the stars, which can travel further through the dust. This fact, along with its privileged site on the Southern Hemisphere, will allow us to map the Bulge with improved detail and perspective.
+
VISTA, the Visible and Infrared Survey Telescope for Astronomy, is optimized to detect the near-infrared emission of stars, which can travel further through the dust. This fact, along with its privileged site on the Southern Hemisphere, will allow us to map the Bulge with improved detail and perspective.
-
Previously, all-sky 2 dimensional maps in near-infrared wavelengths have been done with one epoch data. Otherwise, multi-epochs observations have been carried out for specific small field of view targets on the bulge an disk. The [[VVV_Survey:About | VISTA Variables in The Via Lactea (VVV) public survey]] will perform multi-epoch and wide FOV observations of the Galaxy's bulge and part of the disk, providing the astronomical public community with a high resolution 3-D (or 4-D if you include the time dimension) map of the bulge
+
Previously, all-sky 2 dimensional maps in near-infrared wavelengths have been done with single epoch data. Otherwise, multi-epoch observations have been carried out for specific small field of view targets on the bulge and disk. The [[VVV_Survey:About | VISTA Variables in The Via Lactea (VVV) public survey]] will perform wide FOV multi-epoch observations of the Galaxy's bulge and part of the disk, providing the astronomical public community with a high resolution 3-D (or 4-D if you include the time dimension) map of the bulge.
   
   
== Latest News ==
== Latest News ==

Revision as of 22:19, 11 August 2010

Welcome to VVV Survey,
An International/ESO/Vista Public Survey.
The Galactic Center, from Paranal (Credit:ESO)

What is the structure of the inner Galactic bulge? How did the Milky Way form? Thanks to VISTA, a 4.1 meter telescope, and its superb near-infrared camera VIRCAM, new observations can be done to help astronomers to further answer these questions.

Even when the Milky Way can be observed by the naked eye from dark places at night, because of our position in the Galaxy, we can actually only see our closest neighborhood. Dust, gas, and stars block the light from other places of our galaxy and thus we are not able to observe far into the bulge, at least in the "visual" part of the electromagnetic spectrum.

VISTA, the Visible and Infrared Survey Telescope for Astronomy, is optimized to detect the near-infrared emission of stars, which can travel further through the dust. This fact, along with its privileged site on the Southern Hemisphere, will allow us to map the Bulge with improved detail and perspective.

Previously, all-sky 2 dimensional maps in near-infrared wavelengths have been done with single epoch data. Otherwise, multi-epoch observations have been carried out for specific small field of view targets on the bulge and disk. The VISTA Variables in The Via Lactea (VVV) public survey will perform wide FOV multi-epoch observations of the Galaxy's bulge and part of the disk, providing the astronomical public community with a high resolution 3-D (or 4-D if you include the time dimension) map of the bulge.

Contents

Latest News

Color Tile from the Mid-Plane Area 008
Color Tile from the Bulge Area 349

Pages for Members

Wiki for Team Members

Acknowledgments

Notes and References

  1. [1], SExtractor, SCAMP, SWARP
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