$$\textrm{GRB Name}$$ |
$$\textrm{ GRB060614 }$$ |
$$-$$ |
$$-$$ |
$$\textrm{Host RA}$$ |
$$\textrm{ 21:23:32.102 }$$ |
$$\textrm{ HST/ACS }$$ |
$$\textrm{Host Dec}$$ |
$$\textrm{ -53:01:36.436 }$$ |
$$\textrm{ HST/ACS }$$ |
$$z^{*}$$ |
\(0.125^{ + 0.002 }_{ -0.002 }\) |
$$-$$ |
$$T_{90} \textrm{ } \textrm{(s)}$$ |
\(108.7\) |
$$-$$ |
$$-$$ |
$$\textrm{Fluence} \textrm{ } (10^{-8} \textrm{erg} \times \textrm{cm}^{-2})$$ |
\(2040.0^{ + 36.3 }_{ -36.3 }\) |
$$-$$ |
$$-$$ |
$$\textrm{X-Ray Detection}$$ |
$$\textrm{ None }$$ |
$$-$$ |
$$-$$ |
$$\textrm{Optical Detection}$$ |
$$\textrm{ None }$$ |
$$-$$ |
$$-$$ |
$$\textrm{Radio Detection}$$ |
$$\textrm{ None }$$ |
$$-$$ |
$$-$$ |
$$\textrm{ U }$$ |
\(22.384^{ + 0.1 }_{ -0.1 }\) |
$$\textrm{ Gemini/GMOS }$$ |
$$\textrm{ Gal-Yam 2006 }$$ |
$$\textrm{ B }$$ |
\(23.019^{ + 0.1 }_{ -0.1 }\) |
$$\textrm{ Gemini/GMOS }$$ |
$$\textrm{ Gal-Yam 2006 }$$ |
$$\textrm{ V }$$ |
\(22.769^{ + 0.1 }_{ -0.1 }\) |
$$\textrm{ Gemini/GMOS }$$ |
$$\textrm{ Gal-Yam 2006 }$$ |
$$\textrm{ R }$$ |
\(22.567^{ + 0.1 }_{ -0.1 }\) |
$$\textrm{ Gemini/GMOS }$$ |
$$\textrm{ Gal-Yam 2006 }$$ |
$$\textrm{ I }$$ |
\(21.953^{ + 0.1 }_{ -0.1 }\) |
$$\textrm{ Gemini/GMOS }$$ |
$$\textrm{ Gal-Yam 2006 }$$ |
$$ F606W $$ $$\textrm{FITS}$$ |
\(22.764^{ + 0.1 }_{ -0.1 }\) |
$$\textrm{ HST/ACS }$$ |
$$\textrm{ Gal-Yam 2006 }$$ |
$$ F814W $$ $$\textrm{FITS}$$ |
\(21.953^{ + 0.1 }_{ -0.1 }\) |
$$\textrm{ HST/ACS }$$ |
$$\textrm{ Gal-Yam 2006 }$$ |
$$\textrm{ Ch 1 }$$ |
\(23.0^{ + 0.13 }_{ -0.13 }\) |
$$\textrm{ Spitzer }$$ |
$$\textrm{observed spectroscopy}$$ |
$$\textrm{Download CSV}$$ |
$$\textrm{ Gemini/GMOS-S }$$ |
$$\textrm{ Yuu 2017 }$$ |
$$\textrm{model photometry}$$ |
$$\textrm{Download CSV}$$ |
$$-$$ |
$$-$$ |
$$\textrm{model spectroscopy}$$ |
$$\textrm{Download CSV}$$ |
$$-$$ |
$$-$$ |
* Spectroscopically determined redshift.
|