$$\textrm{GRB Name}$$ |
$$\textrm{ GRB070809 }$$ |
$$-$$ |
$$-$$ |
$$\textrm{Host RA}$$ |
$$\textrm{ 13:35:04.177 }$$ |
$$\textrm{ HST/WFC3 }$$ |
$$\textrm{ Fong 2013 }$$ |
$$\textrm{Host Dec}$$ |
$$\textrm{ -22:08:33.01 }$$ |
$$\textrm{ HST/WFC3 }$$ |
$$\textrm{ Fong 2013 }$$ |
$$z^{*}$$ |
\(0.473\) |
$$-$$ |
$$\textrm{ Berger 2010 }$$ |
$$T_{90} \textrm{ } \textrm{(s)}$$ |
\(1.3\) |
$$-$$ |
$$-$$ |
$$\textrm{Fluence} \textrm{ } (10^{-8} \textrm{erg} \times \textrm{cm}^{-2})$$ |
\(10.0^{ + 1.0 }_{ -1.0 }\) |
$$-$$ |
$$-$$ |
$$\textrm{X-Ray Detection}$$ |
$$\textrm{ yes }$$ |
$$-$$ |
$$-$$ |
$$\textrm{Optical Detection}$$ |
$$\textrm{ yes }$$ |
$$-$$ |
$$-$$ |
$$\textrm{Radio Detection}$$ |
$$\textrm{ no }$$ |
$$-$$ |
$$-$$ |
$$\textrm{ g }$$ |
\(22.148^{ + 0.05 }_{ -0.05 }\) |
$$\textrm{ Magellan/LDSS3 }$$ |
$$\textrm{ Leibler 2010 }$$ |
$$\textrm{ r }$$ |
\(20.142^{ + 0.02 }_{ -0.02 }\) |
$$\textrm{ Magellan/LDSS3 }$$ |
$$\textrm{ Leibler 2010 }$$ |
$$\textrm{ i }$$ |
\(19.461^{ + 0.05 }_{ -0.05 }\) |
$$\textrm{ Magellan/LDSS3 }$$ |
$$\textrm{ Leibler 2010 }$$ |
$$\textrm{ K }$$ |
\(17.994^{ + 0.04 }_{ -0.04 }\) |
$$\textrm{ Magellan/PANIC }$$ |
$$\textrm{ Leibler 2010 }$$ |
$$ F160W $$ $$\textrm{FITS}$$ |
\(18.261^{ + 0.01 }_{ -0.01 }\) |
$$\textrm{ HST/WFC3 }$$ |
$$\textrm{ Fong 2013 }$$ |
$$\textrm{ F606W }$$ |
\(20.68^{ + 0.03 }_{ -0.03 }\) |
$$\textrm{ HST/ACS }$$ |
$$\textrm{ Fong 2013 }$$ |
$$\textrm{observed spectroscopy}$$ |
$$\textrm{Download CSV}$$ |
$$\textrm{ None }$$ |
$$\textrm{model photometry}$$ |
$$\textrm{Download CSV}$$ |
$$-$$ |
$$-$$ |
$$\textrm{model spectroscopy}$$ |
$$\textrm{Download CSV}$$ |
$$-$$ |
$$-$$ |
* Spectroscopically determined redshift.
|