Status of the micro-X sounding rocket x-ray spectrometer

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 cm 2 , a field of view of 11.8 arcmin, and a bandpass of 0.1-2.5 keV. The de...

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Hauptverfasser: Doriese, W. B., Eckart, M. E., Hilton, G. C., Hubbard, A. J. F., Kelley, R. L., Kilbourne, C. A., McCammon, D., Okajima, T., Porter, F. S., Reintsema, C. D., Serlemitsos, P., Smith, S. J., Wikus, P., Goldfinger, David C., Adams, Joseph S, Baker, Robert P, Bandler, Suri C., Danowski, Meredith E, Figueroa-Feliciano, Enectali, Heine, Sarah N.T., Wikus, Patrick
Weitere Verfasser: Lincoln Laboratory
Format: Artikel
Veröffentlicht: SPIE, the International Society of Optical Engineering 2018
Schlagworte:
Online Zugang:http://hdl.handle.net/1721.1/116367
https://orcid.org/0000-0001-5268-8423
https://orcid.org/0000-0001-9285-5556
https://orcid.org/0000-0003-4081-6322
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author Doriese, W. B.
Eckart, M. E.
Hilton, G. C.
Hubbard, A. J. F.
Kelley, R. L.
Kilbourne, C. A.
McCammon, D.
Okajima, T.
Porter, F. S.
Reintsema, C. D.
Serlemitsos, P.
Smith, S. J.
Wikus, P.
Goldfinger, David C.
Adams, Joseph S
Baker, Robert P
Bandler, Suri C.
Danowski, Meredith E
Figueroa-Feliciano, Enectali
Heine, Sarah N.T.
Wikus, Patrick
author2 Lincoln Laboratory
author_facet Lincoln Laboratory
Doriese, W. B.
Eckart, M. E.
Hilton, G. C.
Hubbard, A. J. F.
Kelley, R. L.
Kilbourne, C. A.
McCammon, D.
Okajima, T.
Porter, F. S.
Reintsema, C. D.
Serlemitsos, P.
Smith, S. J.
Wikus, P.
Goldfinger, David C.
Adams, Joseph S
Baker, Robert P
Bandler, Suri C.
Danowski, Meredith E
Figueroa-Feliciano, Enectali
Heine, Sarah N.T.
Wikus, Patrick
author_sort Doriese, W. B.
collection MIT
description 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 cm 2 , 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.
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spelling mit-1721.1/1163672022-10-01T01:08:09Z Status of the micro-X sounding rocket x-ray spectrometer Doriese, W. B. Eckart, M. E. Hilton, G. C. Hubbard, A. J. F. Kelley, R. L. Kilbourne, C. A. McCammon, D. Okajima, T. Porter, F. S. Reintsema, C. D. Serlemitsos, P. Smith, S. J. Wikus, P. Goldfinger, David C. Adams, Joseph S Baker, Robert P Bandler, Suri C. Danowski, Meredith E Figueroa-Feliciano, Enectali Heine, Sarah N.T. Wikus, Patrick Lincoln Laboratory Massachusetts Institute of Technology. Department of Electrical Engineering and Computer Science Massachusetts Institute of Technology. Department of Mathematics Massachusetts Institute of Technology. Department of Physics Goldfinger, David C. Adams, Joseph S Baker, Robert P Bandler, Suri C. Danowski, Meredith E Figueroa-Feliciano, Enectali Heine, Sarah N.T. Wikus, Patrick Microcalorimeter, Sounding Rocket, Transition Edge Sensors, Micro-X, X-ray astronomy, Cryogenics 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 cm 2 , 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. NASA Space Technology Research Fellowship United States. National Aeronautics and Space Administration (grant NNX10AE25G) 2018-06-18T17:46:39Z 2018-06-18T17:46:39Z 2016-08 2018-03-16T17:06:49Z Article http://purl.org/eprint/type/ConferencePaper http://hdl.handle.net/1721.1/116367 Goldfinger, D. C., J. S. Adams, R. Baker, S. R. Bandler, M. E. Danowski, W. B. Doriese, M. E. Eckart, et al. “Status of the Micro-X Sounding Rocket x-Ray Spectrometer.” Edited by Jan-Willem A. den Herder, Tadayuki Takahashi, and Marshall Bautz. Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray (August 26, 2016). https://orcid.org/0000-0001-5268-8423 https://orcid.org/0000-0001-9285-5556 https://orcid.org/0000-0003-4081-6322 http://dx.doi.org/10.1117/12.2233299 Proceedings of SPIE--the Society of Photo-Optical Instrumentation Engineers Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. application/pdf SPIE, the International Society of Optical Engineering SPIE
spellingShingle Microcalorimeter, Sounding Rocket, Transition Edge Sensors, Micro-X, X-ray astronomy, Cryogenics
Doriese, W. B.
Eckart, M. E.
Hilton, G. C.
Hubbard, A. J. F.
Kelley, R. L.
Kilbourne, C. A.
McCammon, D.
Okajima, T.
Porter, F. S.
Reintsema, C. D.
Serlemitsos, P.
Smith, S. J.
Wikus, P.
Goldfinger, David C.
Adams, Joseph S
Baker, Robert P
Bandler, Suri C.
Danowski, Meredith E
Figueroa-Feliciano, Enectali
Heine, Sarah N.T.
Wikus, Patrick
Status of the micro-X sounding rocket x-ray spectrometer
title Status of the micro-X sounding rocket x-ray spectrometer
title_full Status of the micro-X sounding rocket x-ray spectrometer
title_fullStr Status of the micro-X sounding rocket x-ray spectrometer
title_full_unstemmed Status of the micro-X sounding rocket x-ray spectrometer
title_short Status of the micro-X sounding rocket x-ray spectrometer
title_sort status of the micro x sounding rocket x ray spectrometer
topic Microcalorimeter, Sounding Rocket, Transition Edge Sensors, Micro-X, X-ray astronomy, Cryogenics
url http://hdl.handle.net/1721.1/116367
https://orcid.org/0000-0001-5268-8423
https://orcid.org/0000-0001-9285-5556
https://orcid.org/0000-0003-4081-6322
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