You probably mean Winchell Chung's Project Rho site, at
http://www.projectrho.com/rocket/ .
By all means, please post a direct link to a page that explains exactly how a easy it is to detect a point source with a flux density (at detector) of 1e-15 W/m². You were the one making that claim, it's your job to prove it. And please directly explain how easy it is to make a full sky survey from a moving spacecraft in order to detect this energy source.
Incidentally the flux density from the star Alpha Centauri, which is about 4.3
lightyears (~ 270,000 AU) away, is about eight orders of magnitude (100 million times) brighter that our 1 gigawatt reactor at 1 AU (again, assuming the star's entire luminosity is in the infrared, which it isn't). So a reactor is hardly going to stand out from the background stars either.
And of course, the reactor example assumes that the energy is radiating out equally in all directions. If it is somehow focussed (e.g. a drive plume), then it's even less likely to be visible unless the detector is directly in the path of the output.
Assuming that a ship (as described in Traveller) always emits enough radiation to be detectable at interplanetary distances is simply false. And even if it was, assuming that the detector can necessarily know where to look is also false.