Abstract
Micro-X is a sounding rocket borne X-ray telescope that utilizes transition edge sensors to perform imaging spectroscopy with a high level of energy resolution. Its 2.1m focal length X-ray optic has an effective area of 300 cm2, a field of view of 11.8 arcmin, and a bandpass of 0.1-2.5 keV. The detector array has 128 pixels and an intrinsic energy resolution of 4.5 eV FWHM. The integration of the system has progressed with functional tests of the detectors and electronics complete, and performance characterization of the detectors is underway. We present an update of ongoing progress in preparation for the upcoming launch of the instrument.
Original language | English (US) |
---|---|
Title of host publication | Space Telescopes and Instrumentation 2016 |
Subtitle of host publication | Ultraviolet to Gamma Ray |
Editors | Marshall Bautz, Tadayuki Takahashi, Jan-Willem A. den Herder |
Publisher | SPIE |
ISBN (Electronic) | 9781510601895 |
DOIs | |
State | Published - 2016 |
Event | Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray - Edinburgh, United Kingdom Duration: Jun 26 2016 → Jul 1 2016 |
Publication series
Name | Proceedings of SPIE - The International Society for Optical Engineering |
---|---|
Volume | 9905 |
ISSN (Print) | 0277-786X |
ISSN (Electronic) | 1996-756X |
Other
Other | Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray |
---|---|
Country/Territory | United Kingdom |
City | Edinburgh |
Period | 6/26/16 → 7/1/16 |
Funding
This work was supported by a NASA Space Technology Research Fellowship. The Micro-X project is conducted under NASA grant NNX10AE25G.
Keywords
- Cryogenics
- Micro-X
- Microcalorimeter
- Sounding Rocket
- Transition Edge Sensors
- X-ray astronomy
ASJC Scopus subject areas
- Electronic, Optical and Magnetic Materials
- Condensed Matter Physics
- Computer Science Applications
- Applied Mathematics
- Electrical and Electronic Engineering