<filename>flarestack/analyses/ccsn/stasik_2017/ccsn_limits.py
"""Results from the CCSN analysis, performed by <NAME>.
Methods and results are detailed in https://edoc.hu-berlin.de/handle/18452/19442
Two methods were used, both a traditional fixed-weight analysis and a
fixed-weight analysis.
"""
from astropy import units as u
from astropy.table import Table
from flarestack.utils.neutrino_astronomy import calculate_astronomy
from flarestack.core.energy_pdf import EnergyPDF
import numpy as np

# Results

limit_units = 1.0 / (u.cm**2 * u.GeV * u.sr)

# Limits for 1b/c (Choked jet), given for a time window of -20 to 0 days

limits = {
    "Ibc": {"Fixed": 108.169653982, "Fit": 112.567370941},
    "IIn": {"Fixed": 903.46752, "Fit": 903.46752},
    "IIP": {"Fixed": 389.757926076, "Fit": 436.534453846},
}

# Limits are quoted assuming a reference distance of 1 Mpc for a source

ref_dist = 1 * u.Mpc

# Limits are calculated assuming the following Energy PDF

e_pdf_dict = {"energy_pdf_name": "power_law", "gamma": 2.5}

energy_PDF = EnergyPDF.create(e_pdf_dict)
e_integral = energy_PDF.fluence_integral() * u.GeV**2

for (sn, sn_dict) in limits.items():
    for llh_type in ["Fixed", "Fit"]:
        area = (ref_dist.to("cm")) ** 2
        energy = (
            sn_dict[llh_type] * 4 * np.pi * u.sr * limit_units * area * e_integral
        ).to("erg")
        sn_dict[llh_type + " Energy (erg)"] = energy

dt = {"names": ["t", "E"], "formats": ["<f8", "<f8"]}
dt_pvals = {"names": ["t", "pval"], "formats": ["<f8", "<f8"]}


p_vals = {
    "box": {
        "Ibc": np.array(
            [(20, 0.5), (100, 0.5), (300, 0.5), (1000, 0.348)], dtype=dt_pvals
        ),
        "IIp": np.array([(100, 0.317), (300, 0.5), (1000, 0.5)], dtype=dt_pvals),
        "IIn": np.array([(100, 0.064), (300, 0.473), (1000, 0.5)], dtype=dt_pvals),
    },
    "decay": {
        "IIn": np.array([(0.02, 0.016), (0.2, 0.426), (2.0, 0.5)], dtype=dt_pvals),
        "IIp": np.array([(0.02, 0.5), (0.2, 0.5), (2.0, 0.5)], dtype=dt_pvals),
    },
}

limits_figure_paper = {
    "box": {
        "Ibc": np.array(
            [(20, 1.5e48), (100, 1.8e48), (300, 2.6e48), (1000, 4.1e48)], dtype=dt
        ),
        "IIp": np.array([(100, 0.363e49), (300, 0.284e49), (1000, 0.401e49)], dtype=dt),
        "IIn": np.array([(100, 1.55e49), (300, 1.6e49), (1000, 1.53e49)], dtype=dt),
    },
    "decay": {
        "IIn": np.array([(0.02, 2.45e49), (0.2, 1.96e49), (2.0, 3.1e49)], dtype=dt),
        "IIp": np.array([(0.02, 0.355e49), (0.2, 0.263e49), (2.0, 1.38e49)], dtype=dt),
    },
}


limits_figure_sens = {
    "box": {
        "Ibc": np.array(
            [(20, 8e47), (100, 1e48), (300, 1.4e48), (1000, 1.7e48)], dtype=dt
        ),
        "IIp": np.array([(100, 2e48), (300, 1.8e48), (1000, 3e48)], dtype=dt),
        "IIn": np.array([(100, 6e48), (300, 7e48), (1000, 8e48)], dtype=dt),
    },
    "decay": {
        "IIn": np.array([(0.02, 1.1e49), (0.2, 1e49), (2.0, 9e48)], dtype=dt),
        "IIp": np.array([(0.02, 2.2e48), (0.2, 3e48), (2.0, 3.2e48)], dtype=dt),
    },
}


def get_figure_limits(sn_type, pdf_type, sens=False):
    if not sens:
        dictionary = limits_figure_paper
    else:
        dictionary = limits_figure_sens

    if sn_type == "IIP":
        return dictionary[pdf_type]["IIp"]
    else:
        return dictionary[pdf_type][sn_type]


if __name__ == "__main__":
    print("Limits", limits)
    print("limits from figure", limits_figure_paper)

<filename>flarestack/analyses/ccsn/stasik_2017/ccsn_limits.py
"""Results from the CCSN analysis, performed by <NAME>.
Methods and results are detailed in https://edoc.hu-berlin.de/handle/18452/19442
Two methods were used, both a traditional fixed-weight analysis and a
fixed-weight analysis.
"""
from astropy import units as u
from astropy.table import Table
from flarestack.utils.neutrino_astronomy import calculate_astronomy
from flarestack.core.energy_pdf import EnergyPDF
import numpy as np

# Results

limit_units = 1.0 / (u.cm**2 * u.GeV * u.sr)

# Limits for 1b/c (Choked jet), given for a time window of -20 to 0 days

limits = {
    "Ibc": {"Fixed": 108.169653982, "Fit": 112.567370941},
    "IIn": {"Fixed": 903.46752, "Fit": 903.46752},
    "IIP": {"Fixed": 389.757926076, "Fit": 436.534453846},
}

# Limits are quoted assuming a reference distance of 1 Mpc for a source

ref_dist = 1 * u.Mpc

# Limits are calculated assuming the following Energy PDF

e_pdf_dict = {"energy_pdf_name": "power_law", "gamma": 2.5}

energy_PDF = EnergyPDF.create(e_pdf_dict)
e_integral = energy_PDF.fluence_integral() * u.GeV**2

for (sn, sn_dict) in limits.items():
    for llh_type in ["Fixed", "Fit"]:
        area = (ref_dist.to("cm")) ** 2
        energy = (
            sn_dict[llh_type] * 4 * np.pi * u.sr * limit_units * area * e_integral
        ).to("erg")
        sn_dict[llh_type + " Energy (erg)"] = energy

dt = {"names": ["t", "E"], "formats": ["<f8", "<f8"]}
dt_pvals = {"names": ["t", "pval"], "formats": ["<f8", "<f8"]}


p_vals = {
    "box": {
        "Ibc": np.array(
            [(20, 0.5), (100, 0.5), (300, 0.5), (1000, 0.348)], dtype=dt_pvals
        ),
        "IIp": np.array([(100, 0.317), (300, 0.5), (1000, 0.5)], dtype=dt_pvals),
        "IIn": np.array([(100, 0.064), (300, 0.473), (1000, 0.5)], dtype=dt_pvals),
    },
    "decay": {
        "IIn": np.array([(0.02, 0.016), (0.2, 0.426), (2.0, 0.5)], dtype=dt_pvals),
        "IIp": np.array([(0.02, 0.5), (0.2, 0.5), (2.0, 0.5)], dtype=dt_pvals),
    },
}

limits_figure_paper = {
    "box": {
        "Ibc": np.array(
            [(20, 1.5e48), (100, 1.8e48), (300, 2.6e48), (1000, 4.1e48)], dtype=dt
        ),
        "IIp": np.array([(100, 0.363e49), (300, 0.284e49), (1000, 0.401e49)], dtype=dt),
        "IIn": np.array([(100, 1.55e49), (300, 1.6e49), (1000, 1.53e49)], dtype=dt),
    },
    "decay": {
        "IIn": np.array([(0.02, 2.45e49), (0.2, 1.96e49), (2.0, 3.1e49)], dtype=dt),
        "IIp": np.array([(0.02, 0.355e49), (0.2, 0.263e49), (2.0, 1.38e49)], dtype=dt),
    },
}


limits_figure_sens = {
    "box": {
        "Ibc": np.array(
            [(20, 8e47), (100, 1e48), (300, 1.4e48), (1000, 1.7e48)], dtype=dt
        ),
        "IIp": np.array([(100, 2e48), (300, 1.8e48), (1000, 3e48)], dtype=dt),
        "IIn": np.array([(100, 6e48), (300, 7e48), (1000, 8e48)], dtype=dt),
    },
    "decay": {
        "IIn": np.array([(0.02, 1.1e49), (0.2, 1e49), (2.0, 9e48)], dtype=dt),
        "IIp": np.array([(0.02, 2.2e48), (0.2, 3e48), (2.0, 3.2e48)], dtype=dt),
    },
}


def get_figure_limits(sn_type, pdf_type, sens=False):
    if not sens:
        dictionary = limits_figure_paper
    else:
        dictionary = limits_figure_sens

    if sn_type == "IIP":
        return dictionary[pdf_type]["IIp"]
    else:
        return dictionary[pdf_type][sn_type]


if __name__ == "__main__":
    print("Limits", limits)
    print("limits from figure", limits_figure_paper)

Results from the CCSN analysis, performed by <NAME>. Methods and results are detailed in https://edoc.hu-berlin.de/handle/18452/19442 Two methods were used, both a traditional fixed-weight analysis and a fixed-weight analysis. # Results # Limits for 1b/c (Choked jet), given for a time window of -20 to 0 days # Limits are quoted assuming a reference distance of 1 Mpc for a source # Limits are calculated assuming the following Energy PDF