Slumped glass optics with interfacing ribs for high angular resolution x-ray astronomy: a progress report

To reduce the surface micro-roughness of the slumped glass foils, I have proven that the slumping technique with pressure application can also be suited in the indirect slumping,

The plot on the left considers charginos direct production (supposed to be a pure wino status): chargino mass is excluded up to 740 GeV; the right plot shows the exclusion limits

One possible signature for new physics is the production of a heavy resonance with the subsequent decay into a final state consisting of a pair of vector bosons (W W ,.. W

In the Geiger counters used, the cross section sensi- tive to cosmic rays exceeded the area of the window sensitive to x-rays by a factor greater than 20 (and possibly as large as

Since then, I worked in X-ray astronomy at Nagoya University and later at the Institute of Space and Astronautical Science (ISAS), first with balloons and rockets and later

April 1967 saw our first use of Skylark to explore the southern sky from Woomera in South Australia (Cooke et al. 1967), followed over the next 2 years by a larger and more sen-

As template spectra we use the eMILES single stellar popu- lations (SSPs) with a Kroupa (2001) initial mass function (IMF) and the Padova 2000 (Girardi et al. 2000) isochrones

Besides the observation of known sources, given the LHAASO capabilities in sky survey, new galactic sources will likely be discovered at high energy, since objects with fluxes at 1