$$\textrm{GRB Name}$$ |
$$\textrm{ GRB170127B }$$ |
$$-$$ |
$$-$$ |
$$\textrm{Host RA}$$ |
$$\textrm{ 1:19:54.415 }$$ |
$$\textrm{ Keck/LRIS }$$ |
$$\textrm{ BRIGHT }$$ |
$$\textrm{Host Dec}$$ |
$$\textrm{ -30:21:29.615 }$$ |
$$\textrm{ Keck/LRIS }$$ |
$$\textrm{ BRIGHT }$$ |
$$z^{*}$$ |
\(2.21^{ + 0.22 }_{ -0.64 }\) |
$$-$$ |
$$\textrm{ BRIGHT }$$ |
$$T_{90} \textrm{ } \textrm{(s)}$$ |
\(0.51\) |
$$-$$ |
$$-$$ |
$$\textrm{Fluence} \textrm{ } (10^{-8} \textrm{erg} \times \textrm{cm}^{-2})$$ |
\(10.0^{ + 2.0 }_{ -2.0 }\) |
$$-$$ |
$$-$$ |
$$\textrm{X-Ray Detection}$$ |
$$\textrm{ yes }$$ |
$$-$$ |
$$-$$ |
$$\textrm{Optical Detection}$$ |
$$\textrm{ no }$$ |
$$-$$ |
$$-$$ |
$$\textrm{Radio Detection}$$ |
$$\textrm{ no }$$ |
$$-$$ |
$$-$$ |
$$ G $$ $$\textrm{FITS}$$ |
\(25.264^{ + 0.162 }_{ -0.162 }\) |
$$\textrm{ Keck/LRIS }$$ |
$$\textrm{ BRIGHT }$$ |
$$ r $$ $$\textrm{FITS}$$ |
\(25.32^{ + 0.29 }_{ -0.29 }\) |
$$\textrm{ Magellan/LDSS3 }$$ |
$$\textrm{ BRIGHT }$$ |
$$ I $$ $$\textrm{FITS}$$ |
\(25.809^{ + 0.334 }_{ -0.334 }\) |
$$\textrm{ Keck/LRIS }$$ |
$$\textrm{ BRIGHT }$$ |
$$ z $$ $$\textrm{FITS}$$ |
\(24.275^{ + 0.215 }_{ -0.215 }\) |
$$\textrm{ Magellan/IMACS }$$ |
$$\textrm{ BRIGHT }$$ |
$$ J $$ $$\textrm{FITS}$$ |
>\(23.4\) |
$$\textrm{ Keck/MOSFIRE }$$ |
$$\textrm{ BRIGHT }$$ |
$$ K $$ $$\textrm{FITS}$$ |
>\(22.8\) |
$$\textrm{ Magellan/Fourstar }$$ |
$$\textrm{ BRIGHT }$$ |
$$\textrm{observed spectroscopy}$$ |
$$\textrm{Download CSV}$$ |
$$\textrm{ None }$$ |
$$\textrm{model photometry}$$ |
$$\textrm{Download CSV}$$ |
$$-$$ |
$$-$$ |
$$\textrm{model spectroscopy}$$ |
$$\textrm{Download CSV}$$ |
$$-$$ |
$$-$$ |
* Photometric redshift from Prospector
|