Instrument Description"; $browserTitle = "La Silla Instrumentation: HARPS"; # # ##### insert the navigation item where your page is to be shown # ##### NEEDED if not a direct node $current_page = "Instrument Description"; # # ##### Author and AuthorEmail to create a "Send comments to... " instead of the # ##### the standard Contact Form link. $author = "HARPS Instrument Team"; $authorEmail = "harps@eso.org"; # # ******************************************************************************************************************** # do not delete or change these lines include 'frame_top.php'; ?>
There are two readout modes currently offered. Their characteristics, as measured at the telescope, are displayed in the table below. They can differ slightly from what has been measured in the test bench in Garching. The mode of 50kpix/s has been abandoned because, as measured at the telescope, it shows a large readout noise.
Readout mode | Readout frequency | Readout time | Average gain | Average RON (e-) |
Normal | 416kpix/s | 22.5s | 0.75ADU/e- | 4.9e- |
Slow | 104kpix/s | 87.5s | 2.00ADU/e- | 2.9e- |
Below are the links to the monitoring pages of the two CCDs. The CCD "health test" is performed once per week using LEDs located just above the CCDs. A more stable source like the beta light cannot be used as it would require to break the vacuum of the vacuum vessel, a lenghty operation that would compromise the stability of the instrument.