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calibration_files [2012/11/10 04:30]
mjc |
calibration_files [2015/04/28 05:34] (current)
mjc |
| ====== Calibration Files ====== | ====== Calibration Files ====== |
| This page is a repository of baseline calibration files to be used in circumstances where observers were unable to obtain those data during their run. | This page will ultimately be a repository of baseline calibration files to be used in circumstances where observers were unable to obtain those data during their run. The file formats changed in v0.5.0 so previous calibration files were removed. An update email will be sent when these files are available again. (MC: 2015-Apr-28) |
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| The calibration files needed to fully process the data are: | The calibration files needed to fully process the data are: |
| * Telluric correction (red side) | * Telluric correction (red side) |
| |
| To fix this, you need merely go to the repository below and choose the appropriate files for your given setup. Be sure to point your reduction script to these new files. | |
| |
| === Baseline Calibration Files === | |
| Slowly filling the tables of calibration files below... | |
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| A full listing of all baseline calibration files can be found [[http://www.mso.anu.edu.au/~mjc/wifes_redux/calibration_files/|here]]. | |
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| | 1x2 Binning ^ B3000 ^ R3000 ^ U7000 ^ B7000 ^ R7000 ^ I7000 ^ | |
| ^ Flat Response<sup>1</sup> | -- | -- | -- | -- | -- | -- | | |
| ^ Twilight (sky) Flat | -- | -- | -- | -- | -- | -- | | |
| ^ Wavelength Solution | -- | -- | -- | -- | -- | -- | | |
| ^ Wire Solution | -- | -- | -- | -- | -- | -- | | |
| ^ Flux Calibration<sup>2</sup> | [[http://www.mso.anu.edu.au/~mjc/wifes_redux/calibration_files/wifes_B3000_calib.pkl|B3000]] | [[http://www.mso.anu.edu.au/~mjc/wifes_redux/calibration_files/wifes_R3000_calib.pkl|R3000]] | [[http://www.mso.anu.edu.au/~mjc/wifes_redux/calibration_files/wifes_U7000_calib.pkl|U7000]] | [[http://www.mso.anu.edu.au/~mjc/wifes_redux/calibration_files/wifes_B7000_calib.pkl|B7000]] | [[http://www.mso.anu.edu.au/~mjc/wifes_redux/calibration_files/wifes_R7000_calib.pkl|R7000]] | [[http://www.mso.anu.edu.au/~mjc/wifes_redux/calibration_files/wifes_I7000_calib.pkl|I7000]] | | |
| ^ Telluric Correction<sup>2</sup> | N/A | [[http://www.mso.anu.edu.au/~mjc/wifes_redux/calibration_files/wifes_R3000_tellcorr.pkl|R3000]] | N/A | N/A | [[http://www.mso.anu.edu.au/~mjc/wifes_redux/calibration_files/wifes_R7000_tellcorr.pkl|R7000]] | [[http://www.mso.anu.edu.au/~mjc/wifes_redux/calibration_files/wifes_I7000_tellcorr.pkl|I7000]] | | |
| |
| | 1x1 Binning ^ B3000 ^ R3000 ^ U7000 ^ B7000 ^ R7000 ^ I7000 ^ | |
| ^ Flat Response<sup>1</sup> | -- | -- | -- | -- | -- | -- | | |
| ^ Twilight (sky) Flat | -- | -- | -- | -- | -- | -- | | |
| ^ Wavelength Solution | -- | -- | -- | -- | -- | -- | | |
| ^ Wire Solution | -- | -- | -- | -- | -- | -- | | |
| ^ Flux Calibration<sup>2</sup> | [[http://www.mso.anu.edu.au/~mjc/wifes_redux/calibration_files/wifes_B3000_calib.pkl|B3000]] | [[http://www.mso.anu.edu.au/~mjc/wifes_redux/calibration_files/wifes_R3000_calib.pkl|R3000]] | [[http://www.mso.anu.edu.au/~mjc/wifes_redux/calibration_files/wifes_U7000_calib.pkl|U7000]] | [[http://www.mso.anu.edu.au/~mjc/wifes_redux/calibration_files/wifes_B7000_calib.pkl|B7000]] | [[http://www.mso.anu.edu.au/~mjc/wifes_redux/calibration_files/wifes_R7000_calib.pkl|R7000]] | [[http://www.mso.anu.edu.au/~mjc/wifes_redux/calibration_files/wifes_I7000_calib.pkl|I7000]] | | |
| ^ Telluric Correction<sup>2</sup> | N/A | [[http://www.mso.anu.edu.au/~mjc/wifes_redux/calibration_files/wifes_R3000_tellcorr.pkl|R3000]] | N/A | N/A | [[http://www.mso.anu.edu.au/~mjc/wifes_redux/calibration_files/wifes_R7000_tellcorr.pkl|R7000]] | [[http://www.mso.anu.edu.au/~mjc/wifes_redux/calibration_files/wifes_I7000_tellcorr.pkl|I7000]] | | |
| |
| <sup>1</sup> Be **very** cautious, the physical location of the slitlets on the detector tends to change, so which pixels are being sampled will be different perhaps each night. You really should **always** take quartz lamp flats, the use the twilight (sky) flats for the illumination correction (which typically does not change). These flat response files should really only be used for quick reductions. | |
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| <sup>2</sup> These are not binning dependent. | |
