Automated Detection of Short Optical Transients of Astrophysical Origin in Real Time

<table class="table-group" id="tab1"><tr><td><table class="table"><tr><td class="thead-hr" colspan="2"><hr/></td></tr><tr class="thead"><td align="left"> Site separation [km]</td><td align="center"> Maximum distance [km]</td></tr><tr><td class="thead-hr" colspan="2"><hr/></td></tr><tr><td align="left"> 18</td><td align="center"> 103,000</td></tr><tr><td align="left">50</td><td align="center"> 286,000</td></tr><tr><td align="left">100</td><td align="center"> 572,000</td></tr><tr class="table-tr"><td colspan="2"><hr class="tbody-hr"/></td></tr></table></td></tr></table>

Maximal distance from the Earth allowing for the rejection of artificial satellites with the parallax, for the angular size of a pixel of 36 arcsecondo.

Advances in Astronomy

tab1

Table 1

Table 1: Automated Detection of Short Optical Transients of Astrophysical Origin in Real Time 