Update on the Micro-X Sounding Rocket Payload

被引：0

作者：

Figueroa-Feliciano, E. ^{[1
,2
]}

Adams, J. S. ^{[3
,4
]}

Baker, R. ^{[3
]}

Bandler, S. R. ^{[3
,4
]}

Dewey, D. ^{[1
]}

Doriese, W. B. ^{[5
]}

Eckart, M. E. ^{[3
,4
]}

Hamersma, R.

Hilton, G. C. ^{[5
]}

Hwang, U. ^{[3
]}

Irwin, K. D. ^{[5
]}

Kelley, R. L. ^{[3
]}

Kilbourne, C. A. ^{[3
]}

Kissel, S. E. ^{[2
]}

Leman, S. W. ^{[2
]}

McCammon, D. ^{[6
]}

Oakley, P. H. H. ^{[2
]}

Okajima, T. ^{[3
]}

O'Neal, R. H., Jr. ^{[7
]}

Petre, R. ^{[3
]}

Porter, F. S. ^{[3
]}

Reintsema, C. D. ^{[5
]}

Rutherford, J. M. ^{[1
]}

Saab, T. ^{[8
]}

Serlemitsos, P. ^{[3
]}

Soong, Y. ^{[3
]}

Trowbridge, S. N. ^{[1
]}

Wikus, P. ^{[2
]}

机构：

[1] MIT, Dept Phys, Cambridge, MA 02139 USA

[2] MIT, Kavli Inst Astrophys & Space Res, Cambridge, MA 02139 USA

[3] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20770 USA

[4] Univ Maryland, Dept Astron, College Pk, MD 20742 USA

[5] Natl Inst Stand & Technol, Boulder, CO 80305 USA

[6] Univ Wisconsin, Dept Phys, Madison, WI 53706 USA

[7] Florida A&M Univ, Dept Phys, Tallahassee, FL 32304 USA

[8] Univ Florida, Dept Phys, Gainesville, FL 32611 USA

来源：

SPACE TELESCOPES AND INSTRUMENTATION 2012: ULTRAVIOLET TO GAMMA RAY | 2012年 / 8443卷

关键词：

Supernova Remnants; Puppis A; X-ray; Transition Edge Sensor; Microcalorimeter; Sounding Rockets; SUPERNOVA REMNANT PUPPIS; COSMIC-RAY ACCELERATION; HIGH-SPECTRAL-RESOLUTION; TRANSITION-EDGE SENSORS; EMITTING EJECTA; XMM-NEWTON; DISCOVERY; CHANDRA; EMISSION; SHOCK;

D O I：

10.1117/12.927167

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

The Micro-X High Resolution Microcalorimeter X-ray Imaging Rocket is a sounding rocket experiment that will combine a transition-edge-sensor X-ray-microcalorimeter array with a conical imaging mirror to obtain highspectral-resolution images of extended X-ray sources. The target for Micro-X's first flight (slated for January 2013) is the Puppis A supernova remnant. The Micro-X observation of the bright eastern knot of Puppis A will obtain a line-dominated spectrum with up to 27,000 counts collected in 300 seconds at 2 eV resolution across the 0.3-2.5 keV band. Micro-X will determine the thermodynamic and ionization state of the plasma, search for line shifts and broadening associated with dynamical processes, and seek evidence of ejecta enhancement. We describe the progress made in developing this payload, including the detector, cryogenics, and electronics assemblies.

引用

页数：17

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