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GRB130603B

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    GRB and Host Properties
    Attribute Values Telescope Ref
    $$\textrm{GRB Name}$$ $$\textrm{ GRB130603B }$$ $$-$$ $$-$$
    $$\textrm{Host RA}$$ $$\textrm{ 11:28:48.231 }$$ $$\textrm{ HST/ACS }$$ $$\textrm{ Fong 2013 }$$
    $$\textrm{Host Dec}$$ $$\textrm{ +17:04:18.61 }$$ $$\textrm{ HST/ACS }$$ $$\textrm{ Fong 2013 }$$
    $$z^{*}$$ \(0.3568^{ + 0.0005 }_{ -0.0005 }\) $$-$$ $$\textrm{ Cucchiara 2013 }$$
    $$T_{90} \textrm{ } \textrm{(s)}$$ \(0.18\) $$-$$ $$-$$
    $$\textrm{Fluence} \textrm{ } (10^{-8} \textrm{erg} \times \textrm{cm}^{-2})$$ \(63.0^{ + 3.0 }_{ -3.0 }\) $$-$$ $$-$$
    $$\textrm{X-Ray Detection}$$ $$\textrm{ yes }$$ $$-$$ $$-$$
    $$\textrm{Optical Detection}$$ $$\textrm{ yes }$$ $$-$$ $$-$$
    $$\textrm{Radio Detection}$$ $$\textrm{ yes }$$ $$-$$ $$-$$
    $$\textrm{ UVM2 }$$ \(22.85^{ + 0.32 }_{ -0.32 }\) $$\textrm{ Swift/UVOT }$$ $$\textrm{ deUgartePostigo 2014 }$$
    $$\textrm{ UVW1 }$$ \(23.19^{ + 0.28 }_{ -0.28 }\) $$\textrm{ Swift/UVOT }$$ $$\textrm{ deUgartePostigo 2014 }$$
    $$\textrm{ U }$$ \(23.21^{ + 0.49 }_{ -0.49 }\) $$\textrm{ Swift/UVOT }$$ $$\textrm{ deUgartePostigo 2014 }$$
    $$\textrm{ g }$$ \(22.11^{ + 0.06 }_{ -0.06 }\) $$\textrm{ HST }$$ $$\textrm{ deUgartePostigo 2014 }$$
    $$\textrm{ r }$$ \(21.06^{ + 0.06 }_{ -0.06 }\) $$\textrm{ HST }$$ $$\textrm{ deUgartePostigo 2014 }$$
    $$\textrm{ i }$$ \(20.72^{ + 0.06 }_{ -0.06 }\) $$\textrm{ HST }$$ $$\textrm{ deUgartePostigo 2014 }$$
    $$\textrm{ z }$$ \(20.36^{ + 0.06 }_{ -0.06 }\) $$\textrm{ HST }$$ $$\textrm{ deUgartePostigo 2014 }$$
    $$\textrm{ J }$$ \(20.12^{ + 0.07 }_{ -0.07 }\) $$\textrm{ HST }$$ $$\textrm{ deUgartePostigo 2014 }$$
    $$\textrm{ H }$$ \(19.82^{ + 0.06 }_{ -0.06 }\) $$\textrm{ HST }$$ $$\textrm{ deUgartePostigo 2014 }$$
    $$\textrm{ K }$$ \(19.59^{ + 0.07 }_{ -0.07 }\) $$\textrm{ HST/WFC3 }$$ $$\textrm{ deUgartePostigo 2014 }$$
    $$ F160W $$ $$\textrm{FITS}$$ \(19.84^{ + 0.02 }_{ -0.02 }\) $$\textrm{ HST/ACS }$$ $$\textrm{ Fong 2013 }$$
    $$\textrm{observed spectroscopy}$$ $$\textrm{Download CSV}$$ $$\textrm{ Gemini/GMOS-S }$$ $$\textrm{ Cucchiara 2013 }$$
    $$\textrm{model photometry}$$ $$\textrm{Download CSV}$$ $$-$$ $$-$$
    $$\textrm{model spectroscopy}$$ $$\textrm{Download CSV}$$ $$-$$ $$-$$

    * Spectroscopically determined redshift.


    Stellar Population Properties
    Attribute Values
    $$\textrm{Host Morphology}$$ $$-$$
    $$\textrm{Star Formation Classification}$$ \(\textrm{ Star-forming }\)
    $$\textrm{Offset (arcsec)}$$ \(1.07^{ + 0.04 }_{ -0.04 }\)
    $$\textrm{Offset (kpc)}$$ \(5.4^{ + 0.2 }_{ -0.2 }\)
    $$\textrm{Effective Radius } (r_{e})$$ $$-$$
    $$\textrm{Host Normalized Offset } (r_{e})$$ $$0.71$$
    $$\textrm{Probability of Chance Coincidence}$$ $$0.002$$
    $$\textrm{log}(M_* / M_{\odot})$$ \(9.82^{ + 0.05 }_{ -0.04 }\)
    $$t_{m} \textrm{ } \textrm{(Gyr)}$$ \(1.63^{ + 0.43 }_{ -0.53 }\)
    $$\textrm{SFR} (M_{\odot} \times yr^{-1})$$ \(0.44^{ + 0.22 }_{ -0.09 }\)
    $$\log(Z_*/Z_{\odot})$$ \(-0.4^{ + 0.44 }_{ -0.07 }\)
    $$\log(Z_{\textrm{GAS}}/Z_{\odot})$$ \(0.24^{ + 0.16 }_{ -1.5 }\)
    $$A_{V} \textrm{ } \textrm{(mag)}$$ \(0.29^{ + 0.16 }_{ -0.11 }\)