Author/Authors :
Rocks، نويسنده , , L. and Anderson، نويسنده , , M.B. and Bilgri، نويسنده , , N. and Brekosky، نويسنده , , R. and Gwynne Crowder، نويسنده , , S. and Figueroa-Feliciano، نويسنده , , E. and Kelley، نويسنده , , Amy R. and Kilbourne، نويسنده , , C.A. and Lai، نويسنده , , Daniel T. and Lindeman، نويسنده , , M.A. and Man، نويسنده , , J. and McCammon، نويسنده , , D. and Nelms، نويسنده , , K.L. and Porter، نويسنده , , F.S. and Sivananthan، نويسنده ,
Abstract :
The X-ray Quantum Calorimeter (XQC) sounding rocket experiment utilizes a microcalorimeter array for observing the diffuse soft X-ray background. Observations of such low surface-brightness targets require a large-area detector. We will be using an array of large absorbers. Good absorbers must rapidly and completely thermalize photons, have small heat capacity for high stopping efficiency and have good lateral thermal transport. For observing the soft X-ray background (energies <1 keV), the volume and heat capacity of absorber material can be kept to a minimum by making the absorbers only as thick as needed for high quantum efficiency at these low energies. These thin, large-area absorbers are not self-supporting and have poor lateral heat transport. Depositing the absorber material on a Si substrate provides support and improves lateral thermal conduction. We present heat capacity results for thin HgTe and thin Bi, each on Si substrates. We also describe the HgTe absorber fabrication.
Keywords :
Bismuth , HgTe , Microcalorimeters , BI , Mercury telluride