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 February 14, 2020, the DEIMOS detector mosaic presents the following issues (see CCD issues for details):

From dsimulator to detector plane

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.

1. Mask location on the detector plane

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.

DEIMOS image focal plane without mask in spectral mode

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).

DEIMOS image of mask in spectral mode

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.

DEIMOS flat field in spectral mode

2. Blueprint and dsimulator user interface

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.

Blueprint from slitmask database

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.

dsimulator user interface

CCD issues

2020-02-14: CCD5 bad response to illumination

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.

Close-to-nominal bias and bad flat on CCD5
As a consequence, placing high priority targets on CCD1 is not recommended if the spectral features of interest are located on the red side of the spectrum. Please, see section on the relative orientation between the dsimulator diagram and the detector plane to visualize the location of CCD1 on dsimulator. Alignment boxes placed on CCD1 will not be affected by the CCD5 issue.