Beyond Einstein:
From the Big Bang to Black Holes

Stanford Linear Accelerator Center,

Stanford University, 12-15 May 2004

Image of Einstein: Click to return to home page

GRIFFIN Hybrid Optic for the Constellation-X HXT

David Smith
University of California, Santa Cruz
dsmith@scipp.ucsc.edu

Additional authors: Michael Pivovaroff, (LLNL), Gordon Hurford (U. C. Berkeley), William Craig (LLNL), Finn Christensen (DSRI)

Gorenstein and Finoguenov (1994, SPIE 2280, 11) first suggested placing rotating modulation collimator (RMC) in front of a grazing-incidence optic to improve the angular resolution, while retaining the ability of focusing optics to reduce background. We have been studying this technique further, and suggest a way to improve the angular resolution of the Constellation-X HXT below 20 keV to a few arcsec FWHM. The configuration involves little disturbance to the mission plan and little loss of photons at higher energies.

 

return to list of abstracts