kosmos
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| + | ===== KOSMOS ===== | ||
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| The Kitt Peak Ohio State Multi-Object Spectrograph (KOSMOS) was loaned to ARC by NOAO for use on the 3.5m telescope. | The Kitt Peak Ohio State Multi-Object Spectrograph (KOSMOS) was loaned to ARC by NOAO for use on the 3.5m telescope. | ||
| - | A quick-look fact sheet from September, 2019, about KOSMOS II is available | + | A quick-look fact sheet about KOSMOS II from September 2019 is available |
| + | [[https:// | ||
| + | contains the latest edits. | ||
| + | |||
| + | KOSMOS can be used in longslit mode, but also with custom slitmasks, as described in more detail | ||
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| + | [[https:// | ||
| + | |||
| + | ==== Features / issues ==== | ||
| + | |||
| + | * There is significant pattern noise on the detector that varies from frame to frame, likely providing a larger noise floor than expected from the readout noise alone | ||
| + | |||
| + | * There is a Littrow ghost that can appear. Note that this can be seen in flat fields, leading to issues in flat-fielded images if it is not removed from the flat! | ||
| + | |||
| + | * KOSMOS has internal calibration lamps, but the external truss lamps can also be used. There is some flexure in the instrument at different rotator angles. It should be | ||
| + | possible to correct for these using more frequent internal lamp images, but it is also likely that sky lines can be used to achieve this if exposures are sufficiently | ||
| + | long enough to see sky lines, and if you are working in a region where there are sky lines! | ||
| + | |||
| + | ==== Data reduction ==== | ||
| + | |||
| + | * IRAF-based alternatives | ||
| + | * standard IRAF routines (onedspec and twodspec) can be used | ||
| - | The google doc containing | + | * Python alternatives |
| + | * [[https:// | ||
| + | * [[https:// | ||
| + | * Abdullah Korra at the College of Idaho wrote a [[https://github.com/mwbest/CofI_2025|meta package]] to handle slitmask data that uses pyvista under an additional layer of abstraction that allows users to select files to process graphically | ||
| + | * [[https://PypeIt.readthedocs.io|PypeIt]] : a general package for optimal extraction of spectrograph data, including echelle data. Work is in progress on a configuration for KOSMOS | ||
| - | {{medialist> | ||
| - | At the Users Committee meeting on 8/2/2022, someone asked whether any KOSMOS | + | ==== KOSMOS |
| - | ====== KOSMOS multi-object slit masks ====== | ||
| In Summer and Fall 2022, Joe Burchett, Jon Holtzman, and Bill Ketzeback commissioned the multi-object mode of KOSMOS. | In Summer and Fall 2022, Joe Burchett, Jon Holtzman, and Bill Ketzeback commissioned the multi-object mode of KOSMOS. | ||
| Note that the mask wheel for KOSMOS only holds 6 masks and one should be left open for imaging. It may be desirable to have another of the slots left for a long slit. So 4-5 slit masks per night of observations may be ambitious. Making masks for a large number of fields should be avoided for beginning users. | Note that the mask wheel for KOSMOS only holds 6 masks and one should be left open for imaging. It may be desirable to have another of the slots left for a long slit. So 4-5 slit masks per night of observations may be ambitious. Making masks for a large number of fields should be avoided for beginning users. | ||
| - | ===== Mask design | + | === Mask design === |
| Bill has set up a virtual machine at APO with the KOSMOS mask design software, KMS. To access the machine, you'll first need VPN access, a VPN client, and a VNC viewer. | Bill has set up a virtual machine at APO with the KOSMOS mask design software, KMS. To access the machine, you'll first need VPN access, a VPN client, and a VNC viewer. | ||
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| * Once you've output the design (it makes two files), notify Bill (bketzeba at apo.nmsu.edu), | * Once you've output the design (it makes two files), notify Bill (bketzeba at apo.nmsu.edu), | ||
| - | ===== Aligning the mask and observing ===== | + | === Aligning the mask and observing === |
| - | The following is a mask alignment and observing procedure kindly provided by Amanda Townsend. | + | |
| + | The following is a mask alignment and observing procedure kindly provided by Amanda Townsend. | ||
| - Observer should take slit mask alignment map images (initial can be done at start of night with cals) = dim truss qtz OR internal qtz (or arc) with ND5 filter. Match up alignment map to finder chart with slits, figure out which are which ahead of time to save time later! | - Observer should take slit mask alignment map images (initial can be done at start of night with cals) = dim truss qtz OR internal qtz (or arc) with ND5 filter. Match up alignment map to finder chart with slits, figure out which are which ahead of time to save time later! | ||
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| - Put in disperser now. Optional: short exposure to check? | - Put in disperser now. Optional: short exposure to check? | ||
| - Science exposures! | - Science exposures! | ||
| - | ===== Reducing the data ===== | + | |
| + | === Reducing the data === | ||
kosmos.1688489893.txt.gz · Last modified: by jnb
