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GRB111117A

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    GRB and Host Properties
    Attribute Values Telescope Ref
    $$\textrm{GRB Name}$$ $$\textrm{ GRB111117A }$$ $$-$$ $$-$$
    $$\textrm{Host RA}$$ $$\textrm{ 0:50:46.268 }$$ $$\textrm{ Gemini }$$ $$\textrm{ BRIGHT }$$
    $$\textrm{Host Dec}$$ $$\textrm{ +23:00:41.41 }$$ $$\textrm{ Gemini }$$ $$\textrm{ BRIGHT }$$
    $$z^{*}$$ \(2.211^{ + 0.001 }_{ -0.001 }\) $$-$$ $$\textrm{ Selsing 2018 }$$
    $$T_{90} \textrm{ } \textrm{(s)}$$ \(0.47\) $$-$$ $$-$$
    $$\textrm{Fluence} \textrm{ } (10^{-8} \textrm{erg} \times \textrm{cm}^{-2})$$ \(14.0^{ + 1.8 }_{ -1.8 }\) $$-$$ $$-$$
    $$\textrm{X-Ray Detection}$$ $$\textrm{ yes }$$ $$-$$ $$-$$
    $$\textrm{Optical Detection}$$ $$\textrm{ no }$$ $$-$$ $$-$$
    $$\textrm{Radio Detection}$$ $$\textrm{ no }$$ $$-$$ $$-$$
    $$\textrm{ g }$$ \(24.08^{ + 0.09 }_{ -0.09 }\) $$\textrm{ VLT }$$ $$\textrm{ Selsing 2018 }$$
    $$\textrm{ r }$$ \(23.789^{ + 0.11 }_{ -0.11 }\) $$\textrm{ Magellan }$$ $$\textrm{ Margutti 2012 }$$
    $$ i $$ $$\textrm{FITS}$$ \(23.711^{ + 0.08 }_{ -0.08 }\) $$\textrm{ Gemini-N }$$ $$\textrm{ Margutti 2012 }$$
    $$\textrm{ z }$$ \(23.078^{ + 0.18 }_{ -0.18 }\) $$\textrm{ Gemini-N }$$ $$\textrm{ Margutti 2012 }$$
    $$\textrm{ J }$$ \(23.13^{ + 0.18 }_{ -0.18 }\) $$\textrm{ VLT }$$ $$\textrm{ Selsing 2018 }$$
    $$\textrm{ H }$$ \(22.94^{ + 0.29 }_{ -0.29 }\) $$\textrm{ VLT }$$ $$\textrm{ Selsing 2018 }$$
    $$\textrm{ K }$$ \(23.07^{ + 0.32 }_{ -0.32 }\) $$\textrm{ VLT }$$ $$\textrm{ Selsing 2018 }$$
    $$\textrm{observed spectroscopy}$$ $$\textrm{Download CSV}$$ $$\textrm{ None }$$
    $$\textrm{model photometry}$$ $$\textrm{Download CSV}$$ $$-$$ $$-$$
    $$\textrm{model spectroscopy}$$ $$\textrm{Download CSV}$$ $$-$$ $$-$$

    * Spectroscopically determined redshift.


    Stellar Population Properties
    Attribute Values
    $$\textrm{Host Morphology}$$ $$-$$
    $$\textrm{Star Formation Classification}$$ \(\textrm{ Star-forming }\)
    $$\textrm{Offset (arcsec)}$$ \(1.25^{ + 0.2 }_{ -0.2 }\)
    $$\textrm{Offset (kpc)}$$ \(10.52^{ + 1.68 }_{ -1.68 }\)
    $$\textrm{Effective Radius } (r_{e})$$ $$-$$
    $$\textrm{Host Normalized Offset } (r_{e})$$ $$-$$
    $$\textrm{Probability of Chance Coincidence}$$ $$0.0238$$
    $$\textrm{log}(M_* / M_{\odot})$$ \(9.63^{ + 0.22 }_{ -0.22 }\)
    $$t_{m} \textrm{ } \textrm{(Gyr)}$$ \(0.19^{ + 0.21 }_{ -0.1 }\)
    $$\textrm{SFR} (M_{\odot} \times yr^{-1})$$ \(22.11^{ + 9.18 }_{ -6.99 }\)
    $$\log(Z_*/Z_{\odot})$$ \(-0.24^{ + 0.35 }_{ -0.61 }\)
    $$\log(Z_{\textrm{GAS}}/Z_{\odot})$$ $$-$$
    $$A_{V} \textrm{ } \textrm{(mag)}$$ \(0.3^{ + 0.1 }_{ -0.11 }\)