$$\textrm{GRB Name}$$ |
$$\textrm{ GRB070429B }$$ |
$$-$$ |
$$-$$ |
$$\textrm{Host RA}$$ |
$$\textrm{ 21:52:03.691 }$$ |
$$\textrm{ HST/WFC3 }$$ |
$$\textrm{ Fong 2013 }$$ |
$$\textrm{Host Dec}$$ |
$$\textrm{ -38:49:42.82 }$$ |
$$\textrm{ HST/WFC3 }$$ |
$$\textrm{ Fong 2013 }$$ |
$$z^{*}$$ |
\(0.902^{ + 0.001 }_{ -0.001 }\) |
$$-$$ |
$$\textrm{ Cenko 2008 }$$ |
$$T_{90} \textrm{ } \textrm{(s)}$$ |
\(0.47\) |
$$-$$ |
$$-$$ |
$$\textrm{Fluence} \textrm{ } (10^{-8} \textrm{erg} \times \textrm{cm}^{-2})$$ |
\(6.3^{ + 1.0 }_{ -1.0 }\) |
$$-$$ |
$$-$$ |
$$\textrm{X-Ray Detection}$$ |
$$\textrm{ yes }$$ |
$$-$$ |
$$-$$ |
$$\textrm{Optical Detection}$$ |
$$\textrm{ yes }$$ |
$$-$$ |
$$-$$ |
$$\textrm{Radio Detection}$$ |
$$\textrm{ no }$$ |
$$-$$ |
$$-$$ |
$$\textrm{ g }$$ |
\(24.401^{ + 0.2 }_{ -0.2 }\) |
$$\textrm{ Magellan/LDSS3 }$$ |
$$\textrm{ Leibler 2010 }$$ |
$$\textrm{ r }$$ |
\(23.283^{ + 0.04 }_{ -0.04 }\) |
$$\textrm{ Magellan/LDSS3 }$$ |
$$\textrm{ Leibler 2010 }$$ |
$$\textrm{ i }$$ |
\(21.895^{ + 0.09 }_{ -0.09 }\) |
$$\textrm{ Magellan/LDSS3 }$$ |
$$\textrm{ Leibler 2010 }$$ |
$$\textrm{ z }$$ |
\(21.759^{ + 0.12 }_{ -0.12 }\) |
$$\textrm{ Magellan/LDSS3 }$$ |
$$\textrm{ Leibler 2010 }$$ |
$$ F160W $$ $$\textrm{FITS}$$ |
\(20.604^{ + 0.03 }_{ -0.03 }\) |
$$\textrm{ HST/WFC3 }$$ |
$$\textrm{ Cenko 2008 }$$ |
$$\textrm{observed spectroscopy}$$ |
$$\textrm{Download CSV}$$ |
$$\textrm{ Keck/LRIS }$$ |
$$\textrm{ BRIGHT }$$ |
$$\textrm{model photometry}$$ |
$$\textrm{Download CSV}$$ |
$$-$$ |
$$-$$ |
$$\textrm{model spectroscopy}$$ |
$$\textrm{Download CSV}$$ |
$$-$$ |
$$-$$ |
* Spectroscopically determined redshift.
|