Description of the payload

The High Energy X-ray Imaging Spectrometer (HEXIS) program is developing position sensitive Cadmium Zinc Telluride (CZT) X-Ray detectors for use in X-ray astronomy and mission concepts for both balloon and satellite based telescopes.

In a balloon based version of HEXIS, the scientific objectives are to study hot plasmas, non-thermal and accelerated particles, and nuclear and electromagnetic processes in the hard X-ray regime (20-200keV). These processes occur in astrophysical source regions characterized by compact objects, high magnetic fields, high gravitational potentials and general relativistic phenomena. Such sources are known to occur in X-ray pulsars, black hole candidates, active galactic nuclei (AGN) and regions emitting nucleosynthetic gamma rays. CZT detectors are capable of very fine position resolution, to detect this sources.

Details of the balloon flight and scientific outcome


Launch site: Scientific Flight Balloon Facility, New Mexico, US  
Balloon launched by: National Scientific Balloon Facility (NSBF)
Balloon manufacturer/size/composition: Zero Pressure Balloon Raven 4.0 - 113.000 m3 - SF3-4.001-.8/.8-NA
Balloon serial number: R4.001-1-09
Flight identification number: 441N
Payload weight: 1212 lbs

As part of the program development, this was the first balloon flight carriying both a cross strip and a standard planar detector, of dimensions 12 mm x 12 mm x 2 mm, were flown in various passive shield configurations with their cathodes facing earthward.

These detectors, along with the HV bias supply were housed in an aluminum pressure vessel.

This series of balloon flights had significantly improved the understanding of the background properties of CZT, including background rejection techniques based on the physics of CZT detectors. Shielding effects are being extensively studied with this unique data set comprising seven different shielding configurations using the same two detectors and readout systems. These data will contribute great insight into optimal shielding for the next generation hard X-ray instruments.

External references and bibliographical sources

Images of the mission