TemperatureResponseFundamental

class xrtpy.response.TemperatureResponseFundamental(filter_name, observation_date, abundance_model='coronal')

Bases: object

Produce the temperature response for each XRT x-ray channel, assuming a spectral emission model.

Attributes Summary

CHIANTI_temperature	Emission model temperatures in kelvin.
abundance_model_information	A brief description of what abundance model was used in the creation of the emission spectra.
abundances	Defined the name of the requested abundance model as a string.
ccd_gain_right	Provide the camera gain in electrons per data number.
channel_wavelength	Array of wavelengths for every X-ray channel in Å.
chianti_abundance_version	Version of the chianti abundance model.
density_model	A brief description of the plasma density, emission measure,or differential emission measure that was used in the creation of the emission spectra.
ev_per_electron	Amount of energy it takes to dislodge 1 electron in the CCD.
file_spectra	Emission model file spectra.
filter_name	Name of searched filter.
focal_len	Focal length of the telescope in units of cm.
get_abundance_data	Returning the requested abundance data that is used to calculate the temperature response.
ionization_model	A brief description of that ionization equilibrium model was used in the creation of the emission spectra.
observation_date	Date of observation.
pixel_size	CCD pixel size.
solid_angle_per_pixel	This quantity represents the solid angle, which is given in units of steradians over pixel.
wavelength	Emission model file wavelength values in Å.

Methods Summary

effective_area()
integration()
spectra()	Interpolation between the spectra wavelength onto the channel wavelength.
temperature_response()	Apply gain value to the Temperature Response in units of DN cm5 s-1 pix-1.

Attributes Documentation

CHIANTI_temperature

Emission model temperatures in kelvin.

abundance_model_information

A brief description of what abundance model was used in the creation of the emission spectra.

abundances

Defined the name of the requested abundance model as a string.

ccd_gain_right

Provide the camera gain in electrons per data number.

channel_wavelength

Array of wavelengths for every X-ray channel in Å.

chianti_abundance_version

Version of the chianti abundance model.

density_model

A brief description of the plasma density, emission measure,or differential emission measure that was used in the creation of the emission spectra.

ev_per_electron

Amount of energy it takes to dislodge 1 electron in the CCD.

file_spectra

Emission model file spectra.

filter_name

Name of searched filter.

focal_len

Focal length of the telescope in units of cm.

get_abundance_data

Returning the requested abundance data that is used to calculate the temperature response.

ionization_model

A brief description of that ionization equilibrium model was used in the creation of the emission spectra.

observation_date

Date of observation.

pixel_size

CCD pixel size. Units converted from μm to cm.

solid_angle_per_pixel

This quantity represents the solid angle, which is given in units of steradians over pixel.

wavelength

Emission model file wavelength values in Å.

Methods Documentation

effective_area()

integration()

spectra()

Interpolation between the spectra wavelength onto the channel wavelength.

temperature_response()

Apply gain value to the Temperature Response in units of DN cm⁵ s^-1 pix^-1.