Focus | Setup and Remarks | Date |
---|---|---|
1877 | CCD#8, new camera | 10/2003 | 1580 | CCD#8, new camera, flipped MOS mask, Up/Down masks in filter wheel, no grism | 12/6/2004 | 1600 | CCD#8, new camera, 1.0 arcsec slit, Up/Down masks in filter wheel, no grism | 12/6/2004 | 1653 | CCD#8, re-coated new camera, small pinhole, Left/Right masks in grism wheel, no filter Up/Down focus also OK for this value | 29/11/2005 | 1670 | CCD#8, CPH grid upside down, Up/Down hartmanns in grism wheel, no filter | 02/2007 | 1810 | CCD#8, CPH grid, Up/Down hartmanns in grism wheel, no filter | 02/2007 | 2020 | CCD#8, CPH grid , Up/Down hartmanns in grism wheel, B #74 in ALFOSC | 02/2007 | 1820 | CCD#8, CPH grid , Up/Down hartmanns in grism wheel, V #75 in ALFOSC | 02/2007 | 2060 | CCD#8, CPH grid , Up/Down hartmanns in grism wheel, R #76 in ALFOSC | 02/2007 | 1830 | CCD#8, CPH grid , Up/Down hartmanns in grism wheel, B #105 in FASU | 02/2007 | 1810 | CCD#8, CPH grid , Up/Down hartmanns in grism wheel, R #107 in FASU | 02/2007 | 1910 | CCD#8, new CCD3 controller, Up/Down hartmanns, gr7, slit_0.5 TAU | 06/2011 | 1940 | CCD#8, new CCD3 controller, Up/Down hartmanns, gr7, slit_0.5 TAU | 09/2011 | 1315 | CCD#14, Up/Down hartmanns, slit_0.5 JHT, TP | 2016 | 1610 | CCD#14, Up/Down hartmanns, slit_0.5, no grism, with Dome and internal ThAr JHT, TP | 12/2017 |
The above procedure will focus the aperture wheel items onto the detector. It has been investigated that flipping a MOS mask in the aperture wheel makes no significant change to the internal focus. For spectroscopy, a grism has to be added to the beam which will slightly change the internal focus. However, this grism-dependent focus change does not seem to compromise the spectral resolution. Nevertheless, for optimal spectral resolution a Hartmann test with a slit and the grism in the beam can be done, using the pixel shifts of the arc lines.
Any other optics in the beam of ALFOSC, such as filters or calcite blocks, will also change the internal focus of the instrument. For ALFOSC imaging modes we usually choose to compensate for this by changing the telescope focus. However, for slit spectroscopy with added optics (e.g. spectropolarimetry) one has to adjust the internal focus.