scopesim.effects.apertures.ApertureMask#
- class scopesim.effects.apertures.ApertureMask(**kwargs)#
Bases:
EffectOnly provides the on-sky window coords of the Aperture.
- Case: Imaging
Covers the whole FOV of the detector
Round (with mask), square (without mask)
- CaseLS Spec
Covers the slit FOV
Polygonal (with mask), square (without mask)
- CaseIFU Spec
Covers the on-sky FOV of one slice of the IFU
Square (without mask)
- CaseMOS Spec
Covers a single MOS fibre FOV
Round, Polygonal (with mask), square (without mask)
The geometry of an
ApertureMaskcan be initialised with the standard DataContainer methods (see Parameters below). Regardless of which method is used, the following columns must be present:x y arcsec arcsec float float
Certain keywords need to also be included in the ascii header:
# id: <int> # conserve_image: <bool> # x_unit: <str> # y_unit: <str>
If
conserve_imageisFalse, the flux from all sources in the aperture is summed and distributed uniformly over the aperture area.- Parameters:
filename (str) – Path to ASCII file containing the columns listed above
table (astropy.Table) – An astropy Table containing the columns listed above
array_dict (dict) – A dictionary containing the columns listed above:
{x: [...], y: [...], id: <int>, conserve_image: <bool>}pixel_scale (float) – [arcsec] Defaults to
"!INST.pixel_scale"from the configid (int) – An integer to identify the
ApertureMaskin a list of apertures
- __init__(**kwargs)#
Methods
__init__(**kwargs)apply_to(obj, **kwargs)See parent docstring.
fov_grid([which])Return a header with the sky coordinates.
get_from_meta(item)get_header()get_mask()For placing over FOVs if the Aperture is rotated w.r.t.
info()Print basic information on the effect, notably the description.
plot([axes])report([filename, output, rst_title_chars])For Effect objects, generates a report based on the data and meta-data.
Attributes
datadisplay_namehduheaderincludemaskmeta_stringreport_plot_includereport_table_includereport_table_roundingrequired_keystablez_order- apply_to(obj, **kwargs)#
See parent docstring.
- fov_grid(which='edges', **kwargs)#
Return a header with the sky coordinates.
- get_mask()#
For placing over FOVs if the Aperture is rotated w.r.t. the field.
- 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