GRB Host Studies |
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GRB Host Studies (GHostS)
Glossary
Age: age of the stellar population in Myr.
Emission line fluxes: corrected for the Galactic dust extinction, expressed in units of 10-17ergs s-1 cm-2. Host dust extinction and stellar Balmer absorption corrections are not applied.
Galactic dust extinction: extinction due to dust in the Milky Way along the GRB line of sight , expressed as a color excess EB-V .
Luminosity distance: for the cosmology with H0= 70 km s-1 Ωm= 0.3 & ΩΛ= 0.7.
log M∗: stellar mass in solar units, as measured from the optical-NIR photometry.
Redshift: redshift of the host galaxy or GRB afterglow.
SED: spectral energy distribution of the host galaxy, corrected for the Galactic dust extinction.
