Astronomical Images from Keck Observatory
Click on an image to see the full-size version
(all images are false-color and limited resolution)
5 Feb 1999
Keck AO First Light
This spectroscopic double has possibly been resolved optically
(confirmation needed)
Separation is 52 milli-arcsec as measured by KCam with adaptive optics corrections.
Parallax for Sao64240 is 7.8 mas.
Comparison of star imaged without, and with AO
(non-corrected image is on left)
(--More pics on Keck AO Page--)
PXL Guide Camera image, field about 50x50 arcsec, pixel scale 0.1"/pixel
1 millisec exposure with our new PXL guide camera and new F/40 chopping secondary (2x2 binning, 0.2"/pixel)
This is the expanding gas shell remnant of the famous supernova observed by Chinese astronomers in 1054 AD
30sec LRIS+Hippo polarimeter image, radius 1.8 arcmin, by Ken Chambers (UH Institute for Astronomy), 30 Aug 1997
Imaged with LRIS, low-resolution imaging spectrometer, R-band 150sec exposure, Dec 1994 by J.Cohen
Imaged with our CCD guide camera (false color), on 10 June 96. Seeing was poor that night (~1 arcsec)
Abell 79 Supernova remnant, imaged with the Keck 2 guide camera
Showing the LRIS spectroscopic slit (horizontal black line), and the gas shell as it expands about the source supernova (bright star below slit, near center left-right)
"Einstein Ring"- The image of a distant galaxy, gravitationally distorted into a "ring" by a massive object between the galaxy and the Earth
M77 (guider image)
Abell 370, containing a gravitational lens
(5-minute LRIS image in V)
MIRLIN mid-IR images
NIRC 2.3um image
Taken 30 June 1998 by BGoodrich
Seeing was marginal at 0.6" (K)
Pixel size is 0.15 arcsec