scopesim.effects.metis_ifu_simple.ifu_simple.LineSpreadFunction#
- class scopesim.effects.metis_ifu_simple.ifu_simple.LineSpreadFunction(**kwargs)#
Bases:
EffectCompute and apply line spread function to IFU cube.
The effect can be instantiated either with the single parameter
- lsfwidthfloat
Width of the line-spread function in pixels
or with the following set of parameters:
- wavelenfloat
Central wavelength of the LMS setting [um]
- fit_slope, fit_interceptfloat
Parameters of a linear fit of the mean dispersion (Delta lambda per pixel on the LMS detector) as a function of central wavelength. For METIS LMS, these values are obtained from TRACE_LMS.fits with the script fit_ifu_dispersion.py in irdb/METIS/code.
- slice_widthfloat
On-sky width of a slice of the LMS slicer [arcsec]
- pixel_scalefloat
On-sky angle covered by a pixel of the LMS detector array [arcsec]
- spec_binwidthfloat
Spectral bin width of the 3D detector of the lms_cube mode.
These values are set in METIS_LMS_SMPL.yaml.
Added in version 0.10.0.
- __init__(**kwargs)#
Methods
__init__(**kwargs)apply_to(obj, **kwargs)Apply the LSF.
get_from_meta(item)Build LSF kernel: box kernel smoothed with narrow Gauss.
Determine width of the LSF kernel at central wavelength.
info()Print basic information on the effect, notably the description.
report([filename, output, rst_title_chars])For Effect objects, generates a report based on the data and meta-data.
Attributes
datadisplay_nameincludemeta_stringreport_plot_includereport_table_includerequired_keystablez_order- apply_to(obj, **kwargs)#
Apply the LSF.
- get_kernel()#
Build LSF kernel: box kernel smoothed with narrow Gauss.
- get_lsf_width()#
Determine width of the LSF kernel at central wavelength.
- report(filename=None, output='rst', rst_title_chars='*+', **kwargs)#
For Effect objects, generates a report based on the data and meta-data.
This is to aid in the automation of the documentation process of the instrument packages in the IRDB.
Note
If the Effect can generate a plot, this will be saved to disc
- Parameters:
filename (str, optional) – Where to save the RST file
output (str, optional) – [“rst”, “latex”] Output file format
rst_title_chars (2-str, optional) – Two unique characters used to denote rst subsection headings. Options: = - ` : ‘ “ ~ ^ _ * + # < >
parameters (Additional)
---------------------
**kwargs (Either from the self.meta["report"] dictionary or via)
"report_table_include" (False)
"report_table_caption"
"report_plot_caption"
"report_plot_include" (False)
"report_plot_file_formats" (["png"]) – Multiple formats can be saved. The last entry is used for the RST.
"report_plot_filename" (None) – If None, uses self.meta[“name”] as the filename
"file_description" (str) – Taken from the header of a file, if available
"class_description" (str) – Taken from the docstring of the subclass
"changes_str" (list of str) – Take from the header of a file, if available
- Returns:
rst_str – The full reStructureText string
- Return type:
Notes
The format of the RST output is as follows:
<ClassType>: <effect name> ************************** File Description: <description for file meta data> Class Description: <description from class docstring> Changes: <list of changes from file meta data> Data ++++ .. figure:: <Figure_name>.png If the <Effect> object contains a ``.plot()`` function, add plot and write it to disc Figure caption Table caption Table If the <Effect> object contains a ``.table()`` function, add a pprint version of the table Meta-data +++++++++ :: A code block print out of the ``.meta`` dictionary