The Orthogonal Transfer CCD
| dc.creator | Tonry, John L. | |
| dc.creator | Burke, Barry E. | |
| dc.creator | Schechter, Paul L. | |
| dc.date | 1997-05-21 | |
| dc.date.accessioned | 2026-07-07T02:23:25Z | |
| dc.date.available | 2026-07-07T02:23:25Z | |
| dc.description | We have designed and built a new type of CCD that we call an orthogonal transfer CCD (OTCCD), which permits parallel clocking horizontally as well as vertically. The device has been used successfully to remove image motion caused by atmospheric turbulence at rates up to 100 Hz, and promises to be a better, cheaper way to carry out image motion correction for imaging than by using fast tip/tilt mirrors. We report on the device characteristics, and find that the large number of transfers needed to track image motion does not significantly degrade the image either because of charge transfer inefficiency or because of charge traps. For example, after 100 sec of tracking at 100 Hz approximately 3% of the charge would diffuse into a skirt around the point spread function. Four nights of data at the Michigan-Dartmouth-MIT (MDM) 2.4-m telescope also indicate that the atmosphere is surprisingly benign, in terms of both the speed and coherence angle of image motion. Image motion compensation improved image sharpness by about 0.5 arcsec in quadrature with no degradation over a field of at least 3 arcminutes. | |
| dc.description | 21 pages, AASTeX Latex, including 15 Postscript figures, to be published in PASP | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9705165 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9705165 | |
| dc.identifier | Exper.Astron. 8 (1998) 77-87 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/11238 | |
| dc.subject | Astrophysics | |
| dc.title | The Orthogonal Transfer CCD | |
| dc.type | text |