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GRB100206A

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    GRB and Host Properties
    Attribute Values Telescope Ref
    $$\textrm{GRB Name}$$ $$\textrm{ GRB100206A }$$ $$-$$ $$-$$
    $$\textrm{Host RA}$$ $$\textrm{ 3:08:39.142 }$$ $$\textrm{ None }$$
    $$\textrm{Host Dec}$$ $$\textrm{ +13:09:29.34 }$$ $$\textrm{ None }$$
    $$z^{*}$$ \(0.407^{ + 0.002 }_{ -0.002 }\) $$-$$ $$\textrm{ Perley 2012 }$$
    $$T_{90} \textrm{ } \textrm{(s)}$$ \(0.12\) $$-$$ $$-$$
    $$\textrm{Fluence} \textrm{ } (10^{-8} \textrm{erg} \times \textrm{cm}^{-2})$$ \(14.0^{ + 2.0 }_{ -2.0 }\) $$-$$ $$-$$
    $$\textrm{X-Ray Detection}$$ $$\textrm{ yes }$$ $$-$$ $$-$$
    $$\textrm{Optical Detection}$$ $$\textrm{ no }$$ $$-$$ $$-$$
    $$\textrm{Radio Detection}$$ $$\textrm{ no }$$ $$-$$ $$-$$
    $$\textrm{ g }$$ \(23.9^{ + 0.17 }_{ -0.17 }\) $$\textrm{ Keck/LRIS }$$ $$\textrm{ Perley 2012 }$$
    $$\textrm{ R }$$ \(21.53^{ + 0.09 }_{ -0.09 }\) $$\textrm{ Keck/LRIS }$$ $$\textrm{ Perley 2012 }$$
    $$ i $$ $$\textrm{FITS}$$ \(20.86^{ + 0.08 }_{ -0.08 }\) $$\textrm{ Gemini/GMOS-N }$$ $$\textrm{ Perley 2012 }$$
    $$\textrm{ z }$$ \(20.2^{ + 0.05 }_{ -0.05 }\) $$\textrm{ Gemini/GMOS-N }$$ $$\textrm{ Perley 2012 }$$
    $$\textrm{ J }$$ \(19.41^{ + 0.12 }_{ -0.12 }\) $$\textrm{ PAIRITEL }$$ $$\textrm{ Perley 2012 }$$
    $$\textrm{ H }$$ \(18.63^{ + 0.09 }_{ -0.09 }\) $$\textrm{ PAIRITEL }$$ $$\textrm{ Perley 2012 }$$
    $$\textrm{ K }$$ \(18.17^{ + 0.11 }_{ -0.11 }\) $$\textrm{ PAIRITEL }$$ $$\textrm{ Perley 2012 }$$
    $$\textrm{ W1 }$$ \(18.51^{ + 0.06 }_{ -0.06 }\) $$\textrm{ WISE }$$
    $$\textrm{ W2 }$$ \(18.54^{ + 0.11 }_{ -0.11 }\) $$\textrm{ WISE }$$
    $$\textrm{ W3 }$$ \(16.38^{ + 0.16 }_{ -0.16 }\) $$\textrm{ WISE }$$
    $$\textrm{ W4 }$$ >\(15.18\) $$\textrm{ WISE }$$
    $$\textrm{observed spectroscopy}$$ $$\textrm{Download CSV}$$ $$\textrm{ Keck/LRIS }$$ $$\textrm{ Perley 2012 }$$
    $$\textrm{model photometry}$$ $$\textrm{Download CSV}$$ $$-$$ $$-$$
    $$\textrm{model spectroscopy}$$ $$\textrm{Download CSV}$$ $$-$$ $$-$$

    * Spectroscopically determined redshift.


    Stellar Population Properties
    Attribute Values
    $$\textrm{Host Morphology}$$ $$-$$
    $$\textrm{Star Formation Classification}$$ \(\textrm{ Star-forming }\)
    $$\textrm{Offset (arcsec)}$$ \(4.59^{ + 2.37 }_{ -2.37 }\)
    $$\textrm{Offset (kpc)}$$ \(25.28^{ + 13.05 }_{ -13.05 }\)
    $$\textrm{Effective Radius } (r_{e})$$ $$-$$
    $$\textrm{Host Normalized Offset } (r_{e})$$ $$-$$
    $$\textrm{Probability of Chance Coincidence}$$ $$0.02$$
    $$\textrm{log}(M_* / M_{\odot})$$ \(10.72^{ + 0.02 }_{ -0.02 }\)
    $$t_{m} \textrm{ } \textrm{(Gyr)}$$ \(4.58^{ + 0.15 }_{ -0.2 }\)
    $$\textrm{SFR} (M_{\odot} \times yr^{-1})$$ \(7.64^{ + 0.95 }_{ -0.83 }\)
    $$\log(Z_*/Z_{\odot})$$ \(0.18^{ + 0.01 }_{ -0.01 }\)
    $$\log(Z_{\textrm{GAS}}/Z_{\odot})$$ \(0.3^{ + 0.13 }_{ -0.11 }\)
    $$A_{V} \textrm{ } \textrm{(mag)}$$ \(1.19^{ + 0.11 }_{ -0.1 }\)