This page describes issues that are currently affecting the DEIMOS science detector. The page will be updated regularly with the latest status.
Each CCD on the detector mosaic can be read using two amplifiers. In spectroscopy mode, we use the B amplifiers (AMPMODE = SINGLE:B), because A amplifiers are overall noisier. In direct imaging mode, we normally use both amplifiers (AMPMODE = DUAL:A+B) to read the detector, because the readout time is twice as fast than with one amplifier for mask alignments. It is not possible to read the detector using both amplifiers in spectroscopy mode.)
As of September 15, 2020, the DEIMOS detector mosaic presents the following issues (see CCD issues for details):
As of February 14, 2020, the DEIMOS detector mosaic presents the following issues (see CCD issues for details):
This section describes the relative orientation between the dsimulator user interface, mask design blueprints and detector plane. This is intended to serve as a reference to determine which areas on the dsimulator interface should be avoided to prevent the spectra of the highest priority targets from being affected by any given issue on the detector mosaic. Plesae, click on the images below for an expanded view.
The next figure shows the location and orientation of the instrument focal plane with respect to the detector as it is normally seen on a modern DS9 display tool. The image was opened using DS9 with the option to match the coordinate system to the WCS. This is not a sky WCS but a detector WCS that contains the relative location between amplifiers on a DEIMOS mosaic image. This is also how the image looks like when opened with the DEIMOS real-time DS9 GUI. The image was taken with one of the internal calibration lamps and no mask inserted in the optical path. Note that CCD5 looks like a bias due to the issue described reported on February 14, 2020.
The next image was also illuminated with one of the internal calibration lamps, but a mask was inserted in the optical path (please, expand the image for a better visualization of the slits and alignment boxes).
Next figure shows an internal spectral flat taken with the same slitmask that was used to take the mask image shown in the previous figure.
The following figure shows the blueprint corresponding to the mask shown in the previous section. Note that the blueprint is rotated by 180 degrees with respect to the mask image displayed with DS9. CCD1 is on the right-hand side in the blueprint, instead of the left-hand side.
The following image shows the dsimulator user interface for a different mask than the one shown in the image above. It is important to note that the disimulator orientation matches the blueprint orientation. The slitmask diagram shown in the dsimulatior is rotated by 180 deg with respect to the image displayed with DS9.
The following figure shows a flat and a bias frame taken with the B amplifiers on October 17, 2020. The CCD5B bias is noisier the rest of the CCDs. The flat frame displayed on the left-hand side of the figure is nominal for all CCDs, including CCD5B. Note also the horizontal bands on the CCD8B bias.
The following figure shows a flat and a bias frame taken with the A amplifiers on October 17, 2020. The CCD5A bias is nominal, but CCD5A does not respond to illumination. Note also the horizontal bands on the CCD3A bias. The CCD6A bias has all pixel values at 1024 counts. The CCD8A flat counts are about half the flat counts on the neighbor CCDs.
The following figure shows a flat and a bias frame taken on February 14, 2020. The bias frame on the right-hand side of the figure looks normal. The flat frame displayed on the left-hand side of the figure does not contain any signal on CCD5. Therefore, spectra from slits placed on the the CCD below CCD5, i.e. CCD1, will be missing the red side of the spectrum.