$$\textrm{GRB Name}$$ |
$$\textrm{ GRB150423A }$$ |
$$-$$ |
$$-$$ |
$$\textrm{Host RA}$$ |
$$\textrm{ None }$$ |
$$\textrm{ None }$$ |
$$\textrm{Host Dec}$$ |
$$\textrm{ None }$$ |
$$\textrm{ None }$$ |
$$z^{*}$$ |
\(1.394^{ + 0.0 }_{ 0.0 }\) |
$$-$$ |
$$\textrm{ Selsing 2019 }$$ |
$$T_{90} \textrm{ } \textrm{(s)}$$ |
\(0.22\) |
$$-$$ |
$$-$$ |
$$\textrm{Fluence} \textrm{ } (10^{-8} \textrm{erg} \times \textrm{cm}^{-2})$$ |
\(6.3^{ + 1.0 }_{ -1.0 }\) |
$$-$$ |
$$-$$ |
$$\textrm{X-Ray Detection}$$ |
$$\textrm{ yes }$$ |
$$-$$ |
$$-$$ |
$$\textrm{Optical Detection}$$ |
$$\textrm{ yes }$$ |
$$-$$ |
$$-$$ |
$$\textrm{Radio Detection}$$ |
$$\textrm{ no }$$ |
$$-$$ |
$$-$$ |
$$ g $$ $$\textrm{FITS}$$ |
>\(-1.0\) |
$$\textrm{ Magellan/IMACS }$$ |
$$\textrm{ BRIGHT }$$ |
$$ r $$ $$\textrm{FITS}$$ |
>\(-1.0\) |
$$\textrm{ MMT/MMTCam }$$ |
$$\textrm{ BRIGHT }$$ |
$$ i $$ $$\textrm{FITS}$$ |
>\(-1.0\) |
$$\textrm{ Magellan/IMACS }$$ |
$$\textrm{ BRIGHT }$$ |
$$ z $$ $$\textrm{FITS}$$ |
>\(-1.0\) |
$$\textrm{ Magellan/IMACS }$$ |
$$\textrm{ BRIGHT }$$ |
$$ J $$ $$\textrm{FITS}$$ |
>\(-1.0\) |
$$\textrm{ Magellan/Fourstar }$$ |
$$\textrm{ BRIGHT }$$ |
$$ K $$ $$\textrm{FITS}$$ |
>\(-1.0\) |
$$\textrm{ Magellan/Fourstar }$$ |
$$\textrm{ BRIGHT }$$ |
$$ F110W $$ $$\textrm{FITS}$$ |
>\(28.1\) |
$$\textrm{ HST/WFC3 }$$ |
$$\textrm{ BRIGHT }$$ |
$$\textrm{observed spectroscopy}$$ |
$$\textrm{Download CSV}$$ |
$$\textrm{ None }$$ |
$$\textrm{model photometry}$$ |
$$\textrm{Download CSV}$$ |
$$-$$ |
$$-$$ |
$$\textrm{model spectroscopy}$$ |
$$\textrm{Download CSV}$$ |
$$-$$ |
$$-$$ |
* Spectroscopic redshift from afterglow.
|