$$\textrm{GRB Name}$$ |
$$\textrm{ GRB120804A }$$ |
$$-$$ |
$$-$$ |
$$\textrm{Host RA}$$ |
$$\textrm{ 15:35:47.510 }$$ |
$$\textrm{ Gemini }$$ |
$$\textrm{ Berger 2013 }$$ |
$$\textrm{Host Dec}$$ |
$$\textrm{ -28:46:56.11 }$$ |
$$\textrm{ Gemini }$$ |
$$\textrm{ Berger 2013 }$$ |
$$z^{*}$$ |
\(1.05^{ + 0.23 }_{ -0.09 }\) |
$$-$$ |
$$\textrm{ BRIGHT }$$ |
$$T_{90} \textrm{ } \textrm{(s)}$$ |
\(0.81\) |
$$-$$ |
$$-$$ |
$$\textrm{Fluence} \textrm{ } (10^{-8} \textrm{erg} \times \textrm{cm}^{-2})$$ |
\(88.0^{ + 5.0 }_{ -5.0 }\) |
$$-$$ |
$$-$$ |
$$\textrm{X-Ray Detection}$$ |
$$\textrm{ yes }$$ |
$$-$$ |
$$-$$ |
$$\textrm{Optical Detection}$$ |
$$\textrm{ yes }$$ |
$$-$$ |
$$-$$ |
$$\textrm{Radio Detection}$$ |
$$\textrm{ no }$$ |
$$-$$ |
$$-$$ |
$$\textrm{ r }$$ |
\(26.406^{ + 0.2 }_{ -0.2 }\) |
$$\textrm{ Gemini }$$ |
$$\textrm{ Berger 2013 }$$ |
$$ i $$ $$\textrm{FITS}$$ |
\(25.176^{ + 0.15 }_{ -0.15 }\) |
$$\textrm{ Gemini }$$ |
$$\textrm{ Berger 2013 }$$ |
$$\textrm{ Y }$$ |
\(23.934^{ + 0.3 }_{ -0.3 }\) |
$$\textrm{ ESO/Hawk-1 }$$ |
$$\textrm{ Berger 2013 }$$ |
$$\textrm{ J }$$ |
\(23.157^{ + 0.2 }_{ -0.2 }\) |
$$\textrm{ LCO/Fourstar }$$ |
$$\textrm{ Berger 2013 }$$ |
$$\textrm{ K }$$ |
\(22.067^{ + 0.1 }_{ -0.1 }\) |
$$\textrm{ ESO-Hawk-1 }$$ |
$$\textrm{ Berger 2013 }$$ |
$$\textrm{observed spectroscopy}$$ |
$$\textrm{Download CSV}$$ |
$$\textrm{ None }$$ |
$$\textrm{model photometry}$$ |
$$\textrm{Download CSV}$$ |
$$-$$ |
$$-$$ |
$$\textrm{model spectroscopy}$$ |
$$\textrm{Download CSV}$$ |
$$-$$ |
$$-$$ |
* Photometric redshift from Prospector.
|