llama.files.i3.tex module

FileHandler for making a nicely-formatted LaTeX table of IceCube neutrinos including their reconstructed properties and their joint significance when combined with a gravitational wave.

class llama.files.i3.tex.IceCubeNeutrinoListTex

Bases: llama.filehandler.FileHandler

Required input files for llama.files.i3.tex.IceCubeNeutrinoListTex (located on the far right of the graph). For a typical trigger, the leftmost files will be generated as triggers become available. They will be used as input for files to their right, eventually allowing llama.files.i3.tex.IceCubeNeutrinoListTex to be generated.

A list of neutrinos and their reconstructed properties as well as the significance of the joint event) in LaTeX format suitable for use in papers and coincident skymap summary plots.

DEPENDENCIES = (<class 'llama.files.i3.json.IceCubeNeutrinoList'>, <class 'llama.files.skymap_info.SkymapInfo'>, <class 'llama.files.coinc_significance.opa.CoincSignificanceI3Lvc'>)

FILENAME = 'IceCubeNeutrinoList.tex'

MANIFEST_TYPES = (<class 'llama.files.i3.tex.IceCubeNeutrinoListTex'>,)

UR_DEPENDENCIES = (<class 'llama.files.skymap_info.SkymapInfo'>, <class 'llama.files.lvc_skymap.LvcSkymapFits'>, <class 'llama.files.i3.json.IceCubeNeutrinoList'>, <class 'llama.files.gracedb.LVCGraceDbEventData'>, <class 'llama.files.lvc_skymap.LvcDistancesJson'>, <class 'llama.files.lvc_skymap.LvcSkymapHdf5'>, <class 'llama.files.gracedb.PAstro'>, <class 'llama.files.coinc_significance.opa.CoincSignificanceI3Lvc'>)

UR_DEPENDENCY_TREE = ImmutableDict({<class 'llama.files.coinc_significance.opa.CoincSignificanceI3Lvc'>: ImmutableDict({<class 'llama.files.gracedb.PAstro'>: ImmutableDict({<class 'llama.files.skymap_info.SkymapInfo'>: ImmutableDict({})}), <class 'llama.files.lvc_skymap.LvcSkymapHdf5'>: ImmutableDict({<class 'llama.files.lvc_skymap.LvcSkymapFits'>: ImmutableDict({<class 'llama.files.skymap_info.SkymapInfo'>: ImmutableDict({})})}), <class 'llama.files.lvc_skymap.LvcDistancesJson'>: ImmutableDict({<class 'llama.files.lvc_skymap.LvcSkymapFits'>: ImmutableDict({<class 'llama.files.skymap_info.SkymapInfo'>: ImmutableDict({})})}), <class 'llama.files.skymap_info.SkymapInfo'>: ImmutableDict({}), <class 'llama.files.gracedb.LVCGraceDbEventData'>: ImmutableDict({<class 'llama.files.skymap_info.SkymapInfo'>: ImmutableDict({})}), <class 'llama.files.i3.json.IceCubeNeutrinoList'>: ImmutableDict({<class 'llama.files.skymap_info.SkymapInfo'>: ImmutableDict({})})}), <class 'llama.files.i3.json.IceCubeNeutrinoList'>: ImmutableDict({<class 'llama.files.skymap_info.SkymapInfo'>: ImmutableDict({})}), <class 'llama.files.skymap_info.SkymapInfo'>: ImmutableDict({})})

llama.files.i3.tex.convert_json_neutrinos_to_latex(infilename, outfilename, gpstime=None, p_values=None)

Take a json-formatted input filename and an output filename (both full paths) as arguments. Convert the neutrino list in the infile into a LaTeX table that can be inserted into a LaTeX document and save it to the path specified in outfilename. If an optional gpstime is given, then the time column will be given as the time difference in seconds between the neutrino’s arrival and the GPS time provided, i.e. the neutrino detection time with t=0 defined as the GPS time. If a list of p_values corresponding to the neutrinos in infilename are provided, then an extra column is added with the P-values.

llama.files.i3.tex.latex_header(num_cols)

Return a header with the appropriate number of columns for a LaTeX table section.