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The brown dwarf CFBDS
J005910.83-011401.3Three-color image of the star field in which the brown dwarf has been discovered. The brown dwarf is the very red object seen at the top left of the image. This image illustrates how very different is the color of this object compared to the other cold stars around.
![]() Click on the image on the left for a larger version.
©
Canada-France-Brown-Dwarf-Survey 2008
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The spectrum of CFBDS
J005910.83-011401.3
This spectrum of the brown dwarf from the Gemini-NorthTelescope shows the brightness (flux) as a function of wavelength in the near-infrared. The peak at around 1.58 nm is characteristic of the p[resence of amonia.
© Canada-France-Brown-Dwarf-Survey 2008 |
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CFHT - The telescope with MegaPrime/MegaCam
The Canada-France-Hawaii telescope structure is based on an equatorial
mount design, with one of the axis of rotation set parallel to the axis
of the Earth¹s rotation. The mirror cell (the white circular
structure
at the bottom of the telescope, seen just above the person giving the
scale
on this photograph) holds and protects the most precious element: the
3.6-meter
diameter mirror. © Canada-France-Hawaii
Telescope Corporation 2006
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The MegaCam
CCD mosaic At the focal plane of MeagCam seen in this photograph, there are 40 CCDs. Each of them, known as the 'e2v 'CCD42-90'', account for more than 9.5 megapixels. 36 of them are used to image the sky, bringing the total number of pixels for the MegaCam mosaic to a staggering 340 million! Want to know more about MegaPrime/MegaCam? You can go here (first light of the camera) or here for more technical information. Various resolution downloads: © Canada-France-Hawaii
Telescope Corporation 2006
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All images on this page are to be used
exclusively for
the purpose of media announcements
related to the "
Astronomers find most
distant black hole (June 2007)" press
release.
For any other use, please seek authorization from CFHT's PR
officer .