ligo.em_bright
This library provides the tools to compute the possibility of merging gravitational-wave binaries to have an electromagnetic counterpart or having a component in the lower mass-gap region. The data products are source properties
HasNS: The mass of at least one of the compact binary coalescence is consistent with a neutron star.HasRemnant: A non-zero amount of remnant matter remained outside the final compact object (a necessary but not sufficient condition to produce certain kinds of electromagnetic emission such as a short GRB or a kilonova).HasMassGap: The mass of at least one of the compact binary coalescence is consistent with lower mass-gap region i.e. between 3-5 solar mass.
The HasNS and HasRemnant quantities depend on, and are marginalized over, several neutron star equations of state (EOS). The marginalization is done using data from GW170817.
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Release files for ligo.em-bright 1.2.2
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Source distribution (sdist)
| File | Size | Uploaded | Provenance | Actions |
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| ligo_em_bright-1.2.2.tar.gz | 26.5 kB | Without provenance | Details for ligo_em_bright-1.2.2.tar.gz |
Built distribution (wheel)
| File | Interpreter | ABI | Platform | Actions Reset |
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| ligo_em_bright-1.2.2-py3-none-any.whl | Python 3 | none | any | Details for ligo_em_bright-1.2.2-py3-none-any.whl |
Total release size: 56.8 kB
Release files / ligo_em_bright-1.2.2.tar.gz
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Release files / ligo_em_bright-1.2.2-py3-none-any.whl
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