$$\textrm{GRB Name}$$ |
$$\textrm{ GRB090510 }$$ |
$$-$$ |
$$-$$ |
$$\textrm{Host RA}$$ |
$$\textrm{ 22:14:12.623 }$$ |
$$\textrm{ HST/WFC3 }$$ |
$$\textrm{ Fong 2013 }$$ |
$$\textrm{Host Dec}$$ |
$$\textrm{ -26:34:58.55 }$$ |
$$\textrm{ HST/WFC3 }$$ |
$$\textrm{ Fong 2013 }$$ |
$$z^{*}$$ |
\(0.903^{ + 0.001 }_{ -0.001 }\) |
$$-$$ |
$$\textrm{ McBreen 2010 }$$ |
$$T_{90} \textrm{ } \textrm{(s)}$$ |
\(5.66\) |
$$-$$ |
$$-$$ |
$$\textrm{Fluence} \textrm{ } (10^{-8} \textrm{erg} \times \textrm{cm}^{-2})$$ |
\(34.0^{ + 4.0 }_{ -4.0 }\) |
$$-$$ |
$$-$$ |
$$\textrm{X-Ray Detection}$$ |
$$\textrm{ yes }$$ |
$$-$$ |
$$-$$ |
$$\textrm{Optical Detection}$$ |
$$\textrm{ yes }$$ |
$$-$$ |
$$-$$ |
$$\textrm{Radio Detection}$$ |
$$\textrm{ no }$$ |
$$-$$ |
$$-$$ |
$$\textrm{ g }$$ |
\(23.86^{ + 0.08 }_{ -0.08 }\) |
$$\textrm{ Magellan/LDSS3 }$$ |
$$\textrm{ Leibler 2010 }$$ |
$$\textrm{ i }$$ |
\(22.45^{ + 0.14 }_{ -0.14 }\) |
$$\textrm{ Magellan/LDSS3 }$$ |
$$\textrm{ Leibler 2010 }$$ |
$$\textrm{ z }$$ |
\(22.69^{ + 0.17 }_{ -0.17 }\) |
$$\textrm{ Magellan/LDSS3 }$$ |
$$\textrm{ Leibler 2010 }$$ |
$$\textrm{ J }$$ |
\(21.81^{ + 0.15 }_{ -0.15 }\) |
$$\textrm{ Magellan/PANIC }$$ |
$$\textrm{ Leibler 2010 }$$ |
$$ F160W $$ $$\textrm{FITS}$$ |
\(21.8^{ + 0.01 }_{ -0.01 }\) |
$$\textrm{ HST/WFC3 }$$ |
$$\textrm{ Fong 2013 }$$ |
$$\textrm{observed spectroscopy}$$ |
$$\textrm{Download CSV}$$ |
$$\textrm{ VLT/FORS2 }$$ |
$$\textrm{ BRIGHT }$$ |
$$\textrm{model photometry}$$ |
$$\textrm{Download CSV}$$ |
$$-$$ |
$$-$$ |
$$\textrm{model spectroscopy}$$ |
$$\textrm{Download CSV}$$ |
$$-$$ |
$$-$$ |
* Spectroscopically determined redshift.
|