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GRB050709

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    GRB and Host Properties
    Attribute Values Telescope Ref
    $$\textrm{GRB Name}$$ $$\textrm{ GRB050709 }$$ $$-$$ $$-$$
    $$\textrm{Host RA}$$ $$\textrm{ 23:01:26.765 }$$ $$\textrm{ HST/ACS }$$ $$\textrm{ Fong 2010 }$$
    $$\textrm{Host Dec}$$ $$\textrm{ -38:58:40.422 }$$ $$\textrm{ HST/ACS }$$ $$\textrm{ Fong 2010 }$$
    $$z^{*}$$ \(0.1607^{ + 0.0004 }_{ -0.0004 }\) $$-$$ $$\textrm{ Fox 2005 }$$
    $$T_{90} \textrm{ } \textrm{(s)}$$ \(0.07\) $$-$$ $$-$$
    $$\textrm{Fluence} \textrm{ } (10^{-8} \textrm{erg} \times \textrm{cm}^{-2})$$ \(29.0^{ + 4.0 }_{ -4.0 }\) $$-$$ $$-$$
    $$\textrm{X-Ray Detection}$$ $$\textrm{ yes }$$ $$-$$ $$-$$
    $$\textrm{Optical Detection}$$ $$\textrm{ yes }$$ $$-$$ $$-$$
    $$\textrm{Radio Detection}$$ $$\textrm{ yes }$$ $$-$$ $$-$$
    $$\textrm{ B }$$ \(22.045^{ + 0.1 }_{ -0.1 }\) $$\textrm{ Danish/DFOSC }$$ $$\textrm{ Hjorth 2005 }$$
    $$\textrm{ V }$$ \(21.344^{ + 0.07 }_{ -0.07 }\) $$\textrm{ VLT/FORS2 }$$ $$\textrm{ Covino 2006 }$$
    $$\textrm{ R }$$ \(21.258^{ + 0.07 }_{ -0.07 }\) $$\textrm{ VLT/FORS2 }$$ $$\textrm{ Covino 2006 }$$
    $$\textrm{ I }$$ \(21.01^{ + 0.08 }_{ -0.08 }\) $$\textrm{ VLT/FORS2 }$$ $$\textrm{ Covino 2006 }$$
    $$\textrm{ J }$$ \(20.759^{ + 0.08 }_{ -0.08 }\) $$\textrm{ Magellan/PANIC }$$ $$\textrm{ Leibler 2010 }$$
    $$\textrm{ K }$$ \(21.044^{ + 0.16 }_{ -0.16 }\) $$\textrm{ Magellan/PANIC }$$ $$\textrm{ Leibler 2010 }$$
    $$\textrm{ F450W }$$ \(21.475^{ + 0.05 }_{ -0.05 }\) $$\textrm{ HST/WFPC2 }$$ $$\textrm{ Fong 2010 }$$
    $$ F814W $$ $$\textrm{FITS}$$ \(21.11^{ + 0.05 }_{ -0.05 }\) $$\textrm{ HST/ACS }$$ $$\textrm{ Fong 2010 }$$
    $$\textrm{observed spectroscopy}$$ $$\textrm{Download CSV}$$ $$\textrm{ Gemini/GMOS-N }$$ $$\textrm{ BRIGHT }$$
    $$\textrm{model photometry}$$ $$\textrm{Download CSV}$$ $$-$$ $$-$$
    $$\textrm{model spectroscopy}$$ $$\textrm{Download CSV}$$ $$-$$ $$-$$

    * Spectroscopically determined redshift.


    Stellar Population Properties
    Attribute Values
    $$\textrm{Host Morphology}$$ \(\textrm{ Spiral }\)
    $$\textrm{Star Formation Classification}$$ \(\textrm{ Star-forming }\)
    $$\textrm{Offset (arcsec)}$$ \(1.35^{ + 0.02 }_{ -0.02 }\)
    $$\textrm{Offset (kpc)}$$ \(3.76^{ + 0.056 }_{ -0.056 }\)
    $$\textrm{Effective Radius } (r_{e})$$ $$-$$
    $$\textrm{Host Normalized Offset } (r_{e})$$ $$2.0$$
    $$\textrm{Probability of Chance Coincidence}$$ $$0.003$$
    $$\textrm{log}(M_* / M_{\odot})$$ \(8.55^{ + 0.01 }_{ -0.01 }\)
    $$t_{m} \textrm{ } \textrm{(Gyr)}$$ \(0.57^{ + 0.0 }_{ 0.0 }\)
    $$\textrm{SFR} (M_{\odot} \times yr^{-1})$$ \(0.02^{ + 0.0 }_{ 0.0 }\)
    $$\log(Z_*/Z_{\odot})$$ \(-0.25^{ + 0.01 }_{ -0.01 }\)
    $$\log(Z_{\textrm{GAS}}/Z_{\odot})$$ \(-0.58^{ + 0.03 }_{ 0.0 }\)
    $$A_{V} \textrm{ } \textrm{(mag)}$$ \(0.02^{ + 0.03 }_{ -0.02 }\)