scopesim.effects.electronic.exposure.AutoExposure#
- class scopesim.effects.electronic.exposure.AutoExposure(**kwargs)#
Bases:
EffectDetermine DIT and NDIT automatically from ImagePlane.
DIT is determined such that the maximum value in the incident photon flux (including astronomical source, sky and thermal backgrounds) fills the full well of the detector (
!DET.full_well) to a given fraction (!OBS.autoexposure.fill_frac). NDIT is determined such thatDIT*NDITresults in the requested exposure time.The requested exposure time is taken from
!OBS.exptime.The effects sets the parameters !OBS.dit and !OBS.ndit.
The effect is the first detector effect, hence essentially operates on the ImagePlane, mapped to the detector array.
Examples
The parameters !OBS.exptime, !DET.full_well and !DET.mindit should be defined as properties in the respective subsections.
name: auto_exposure description: automatic determination of DIT and NDIT class: AutoExposure include: True kwargs: fill_frac: "!OBS.auto_exposure.fill_frac"
- __init__(**kwargs)#
Methods
__init__(**kwargs)apply_to(obj, **kwargs)Apply the effect to the corresponding object.
estimate_dit_ndit(exptime, image_plane_max, ...)Automatically determine DIT and NDIT from exposure time.
get_from_meta(item)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_stringrequired_keystablez_order- apply_to(obj, **kwargs)#
Apply the effect to the corresponding object.
- estimate_dit_ndit(exptime: float, image_plane_max: float, **kwargs) tuple[float, int]#
Automatically determine DIT and NDIT from exposure time.
- 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