Shift a cube spatially
esorex kmo_shift [OPTIONS] FILE.sof
This recipe shifts a cube spatially. A positive x-shift shifts the data to the left, a positive y-shift shifts upwards, where a shift of one pixel equals 0.2arcsec. The output will still have the same dimensions, but the borders will be filled with NaNs accordingly.
To adjust only the WCS without moving the data the --wcs-only parameter has to be set to TRUE. The WCS is updated in the same way as if the data would have moved as well. This means that the point at (x,y) has the same coordinates as the point (x+1,y+1) after updating the WCS (the WCS moved in the opposite direction).
--shifts This parameter must be supplied. It contains the amount of shift to apply. The unit is in arcsec. If the --shifts parameter contains only two values (x,y), all IFUs will be shifted by the same amount. If it contains 48 values (x1,y1;x2,y2;...;x24,y24), the IFUs are shifted individually.
--imethod The interpolation method to apply when the shift value isn’t a multiple of the pixel scale. There are two methods available:
* BCS: Bicubic spline * NN: Nearest Neighbor
--ifu If a single IFU should be shifted, it can be defined using the --ifu parameter (--shifts parameter contains only two values).
--flux Specify if flux conservation should be applied.
--extrapolate By default no extrapolation is applied. This means that the output frame will shrink at most one pixel, because the data is shifted out of the frame. When turning extrapolation on, the size of the output frame stays the same as for the input frame.
--wcs-only By default data and WCS are shifted in sync. If this parameter is set to TRUE only the WCS is updated (i.e. if someone thinks that the IFU isn\'t pointing exactly to the correct coordinates.)
Input files:
DO KMOS category Type Explanation Required #Frames -------- ----- ----------- -------- ------- <none or any> F3I data frame Y 1
Output files:
DO KMOS category Type Explanation -------- ----- ----------- SHIFT F3I Shifted data cube
--imethod <str>
Method to use for interpolation. ["BCS" (bicubic spline, default), "NN" (nearest neighbor)] (str; default: \'BCS\'). The full name of this option for the EsoRex configuration file is kmos.kmo_shift.imethod [default = BCS].
--extrapolate <bool>
Applies only to \'method=BCS\' when doing sub-pixel shifts: FALSE: shifted IFU will be filled with NaN\'s at the borders,TRUE: shifted IFU will be extrapolated at the borders (bool; default: False). The full name of this option for the EsoRex configuration file is kmos.kmo_shift.extrapolate [default = False].
--shifts <str>
The shifts for each spatial dimension for all specified IFUs."x1,y1;x2,y2;..." (arcsec) (str; default: \'\'). The full name of this option for the EsoRex configuration file is kmos.kmo_shift.shifts [default = ].
--ifu <long>
The IFU to shift [1 to 24] or shift all IFUs Default value of 0 applies shift to all IFUs. (long; default: 0). The full name of this option for the EsoRex configuration file is kmos.kmo_shift.ifu [default = 0].
--flux <bool>
Apply flux conservation: (TRUE (apply) or FALSE (don\'t apply) (bool; default: False). The full name of this option for the EsoRex configuration file is kmos.kmo_shift.flux [default = False].
--wcs-only <bool>
FALSE: if data and wcs should be updated.TRUE: if only wcs should be corrected (bool; default: False). The full name of this option for the EsoRex configuration file is kmos.kmo_shift.wcs-only [default = False].
Note that it is possible to create a configuration file containing these options, along with suitable default values. Please refer to the details provided by the 'esorex --help' command.
The full documentation for the kmos pipeline can be downloaded as a PDF file using the following URL:
ftp://ftp.eso.org/pub/dfs/pipelines/kmos/kmos-pipeline-manual-2.9.pdf
An overview over the existing ESO pipelines can be found on the web page http://www.eso.org/sci/software/pipelines/.
Basic documentation about the EsoRex program can be found at the esorex (1) man page.
It is possible to call the pipelines from python using the python-cpl package. See http://packages.python.org/python-cpl/index.html for further information.
The other recipes of the kmos pipeline are kmo_copy(7), kmo_fits_check(7), kmo_sci_red(7), kmo_fits_stack(7), kmo_noise_map(7), kmo_rotate(7), kmo_extract_spec(7), kmo_multi_reconstruct(7), kmo_sky_tweak(7), kmos_gen_reflines(7), kmo_stats(7), kmo_arithmetic(7), kmos_dark(7), kmo_fits_strip(7), kmo_combine(7), kmo_std_star(7), kmo_illumination_flat(7), kmo_make_image(7), kmos_flat(7), kmo_fit_profile(7), kmo_sky_mask(7), kmos_illumination(7), kmos_wave_cal(7), kmo_reconstruct(7)
kmo_shift 1.3.5
Alex Agudo Berbel <[email protected]>
Please report any problems to [email protected]. Alternatively, you may send a report to the ESO User Support Department <[email protected]>.
This file is part of the CRIRES Instrument Pipeline Copyright (C) 2002,2003 European Southern Observatory
This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 2 of the License, or (at your option) any later version.
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