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Residual image

Figure 6 Superimposition of wiid-type CPS (red) (1 JOB) and the C248D CPS mutant (blue) (1T36) showing the structural changes when Cys248 is repiaced by an aspartate residue, image rendered in PYMOL. Figure 6 Superimposition of wiid-type CPS (red) (1 JOB) and the C248D CPS mutant (blue) (1T36) showing the structural changes when Cys248 is repiaced by an aspartate residue, image rendered in PYMOL.
Image sticking time Image sticking Residual image time sifter a black box is displayed. [Pg.49]

We have seen no latent or residual images with this device. We have imaged Vega (> 10 photons/sec in the K band) using the 1.3M telescope at ICitt Peak as well as bright sources in the lab and have seen no effects when the array is immediately put in the dark. This is the most significant improvement that has been made by SBRC in the production of InSb astronomy arrays. [Pg.402]

See other pages where Residual image is mentioned: [Pg.506]    [Pg.295]    [Pg.126]    [Pg.106]    [Pg.11]    [Pg.301]    [Pg.367]    [Pg.720]    [Pg.38]    [Pg.169]    [Pg.202]    [Pg.64]    [Pg.50]    [Pg.70]    [Pg.50]    [Pg.70]    [Pg.328]    [Pg.283]    [Pg.283]    [Pg.283]    [Pg.215]   
See also in sourсe #XX -- [ Pg.283 ]



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