astro.setupGW

nucleardatapy.astro.setup_gw.gw_hyps(source)

Return a list of observations for a given source and print them all on the prompt.

Parameters:

source (str.) – The source for which there are different hypotheses.

Returns:

The list of hypotheses. If source == ‘GW170817’: 1, 2, 3, 4, 5.

Return type:

list[str].

nucleardatapy.astro.setup_gw.gw_sources()

Return a list of the astrophysical sources for which a mass is given

Returns:

The list of sources.

Return type:

list[str].

class nucleardatapy.astro.setup_gw.setupGW(source='GW170817', hyp=1)

Instantiate the tidal deformability for a given source and obs.

This choice is defined in the variables source and obs.

source can chosen among the following ones: ‘GW170817’.

obs depends on the chosen source.

Parameters:

• source (str, optional.) – Fix the name of source. Default value: ‘GW170817’.

• obs (str, optional.) – Fix the obs. Default value: 1.

Attributes:

init_self()

Initialize variables in self.

label

Attribute providing the label the data is references for figures.

note

Attribute providing additional notes about the data.

print_latex()

Method which print outputs in table format (latex) on terminal’s screen.

print_output()

Method which print outputs on terminal’s screen.

ref

Attribute providing the full reference to the paper to be citted.

class nucleardatapy.astro.setup_gw.setupGWAverage(source='GW170817')

Instantiate the total mass for a given source and averaged over hypotheses.

This choice is defined in the variable source.

source can chosen among the following ones: ‘GW170817’.

Parameters:

source (str, optional.) – Fix the name of source. Default value: ‘GW170817’.

Attributes:

init_self()

Initialize variables in self.

print_latex()

Method which print outputs in table format (latex) on terminal’s screen.

print_output()

Method which print outputs on terminal’s screen.

Here is a figure which is produced with the Python sample: /nucleardatapy_sample/astro_setupGW_plot.py

Estimation of the effective tidal deformability from difference sources (different colors) and different hypotheses on the pulsar spin and the waveform employed for match filtering.