CUBIC: x-ray CCD spectroscopy of the diffuse x-ray background

David Nelson Burrows; Mark A. Skinner; Patrick Sean Broos; Mark A. Catalano; Laura J. Cawley; Eric J. Cocklin; Leland G. Engel; Timothy J. Entingh; Gordon P. Garmire; Roland Green; Diego Janches; Douglas A. Kelly

CUBIC: x-ray CCD spectroscopy of the diffuse x-ray background

David Nelson Burrows, Mark A. Skinner, Patrick Sean Broos, Mark A. Catalano, Laura J. Cawley, Eric J. Cocklin, Leland G. Engel, Timothy J. Entingh, Gordon P. Garmire, Roland Green, Diego Janches, Douglas A. Kelly

Astronomy & Astrophysics

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

3 Scopus citations

Abstract

The cosmic unresolved background instrument using CCDs (CUBIC) is currently scheduled for launch on the Argentine/US SAC-B satellite late this year. This instrument is designed to perform moderate resolution nondispersive x-ray spectroscopy of the diffuse x-ray background over the band 0.2 - 10.0 keV using state-of-the-art photon-counting CCDs. The instrument is optimized for spectroscopy of diffuse emission with a field of view of 5 degrees by 5 degrees below 1 keV and 10 degrees by 10 degrees above 3 keV. Observations will typically last 1 - 3 days, and will obtain high quality CCD spectra of the diffuse background, nearby superbubbles and supernova remnants, and the brightest x-ray point sources. This paper gives an overview of the instrument design and CCD detectors.

Original language	English (US)
Title of host publication	Proceedings of SPIE - The International Society for Optical Engineering
Editors	Oswald H. Siegmund, John V. Vallerga
Pages	141-162
Number of pages	22
Volume	2518
State	Published - Dec 1 1995
Event	EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy VI - San Diego, CA, USA Duration: Jul 12 1995 → Jul 14 1995

Other

Other	EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy VI
City	San Diego, CA, USA
Period	7/12/95 → 7/14/95

All Science Journal Classification (ASJC) codes

Electronic, Optical and Magnetic Materials
Condensed Matter Physics
Computer Science Applications
Applied Mathematics
Electrical and Electronic Engineering

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Burrows, D. N., Skinner, M. A., Broos, P. S., Catalano, M. A., Cawley, L. J., Cocklin, E. J., Engel, L. G., Entingh, T. J., Garmire, G. P., Green, R., Janches, D., & Kelly, D. A. (1995). CUBIC: x-ray CCD spectroscopy of the diffuse x-ray background. In O. H. Siegmund, & J. V. Vallerga (Eds.), Proceedings of SPIE - The International Society for Optical Engineering (Vol. 2518, pp. 141-162)

Burrows, David Nelson ; Skinner, Mark A. ; Broos, Patrick Sean ; Catalano, Mark A. ; Cawley, Laura J. ; Cocklin, Eric J. ; Engel, Leland G. ; Entingh, Timothy J. ; Garmire, Gordon P. ; Green, Roland ; Janches, Diego ; Kelly, Douglas A. / CUBIC : x-ray CCD spectroscopy of the diffuse x-ray background. Proceedings of SPIE - The International Society for Optical Engineering. editor / Oswald H. Siegmund ; John V. Vallerga. Vol. 2518 1995. pp. 141-162

@inproceedings{047fd69ae2234d32baaaaf4e940492f6,

title = "CUBIC: x-ray CCD spectroscopy of the diffuse x-ray background",

abstract = "The cosmic unresolved background instrument using CCDs (CUBIC) is currently scheduled for launch on the Argentine/US SAC-B satellite late this year. This instrument is designed to perform moderate resolution nondispersive x-ray spectroscopy of the diffuse x-ray background over the band 0.2 - 10.0 keV using state-of-the-art photon-counting CCDs. The instrument is optimized for spectroscopy of diffuse emission with a field of view of 5 degrees by 5 degrees below 1 keV and 10 degrees by 10 degrees above 3 keV. Observations will typically last 1 - 3 days, and will obtain high quality CCD spectra of the diffuse background, nearby superbubbles and supernova remnants, and the brightest x-ray point sources. This paper gives an overview of the instrument design and CCD detectors.",

author = "Burrows, {David Nelson} and Skinner, {Mark A.} and Broos, {Patrick Sean} and Catalano, {Mark A.} and Cawley, {Laura J.} and Cocklin, {Eric J.} and Engel, {Leland G.} and Entingh, {Timothy J.} and Garmire, {Gordon P.} and Roland Green and Diego Janches and Kelly, {Douglas A.}",

year = "1995",

month = dec,

day = "1",

language = "English (US)",

isbn = "0819418773",

volume = "2518",

pages = "141--162",

editor = "Siegmund, {Oswald H.} and Vallerga, {John V.}",

booktitle = "Proceedings of SPIE - The International Society for Optical Engineering",

note = "EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy VI ; Conference date: 12-07-1995 Through 14-07-1995",

}

Burrows, DN, Skinner, MA, Broos, PS, Catalano, MA, Cawley, LJ, Cocklin, EJ, Engel, LG, Entingh, TJ, Garmire, GP, Green, R, Janches, D & Kelly, DA 1995, CUBIC: x-ray CCD spectroscopy of the diffuse x-ray background. in OH Siegmund & JV Vallerga (eds), Proceedings of SPIE - The International Society for Optical Engineering. vol. 2518, pp. 141-162, EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy VI, San Diego, CA, USA, 7/12/95.

CUBIC : x-ray CCD spectroscopy of the diffuse x-ray background. / Burrows, David Nelson; Skinner, Mark A.; Broos, Patrick Sean; Catalano, Mark A.; Cawley, Laura J.; Cocklin, Eric J.; Engel, Leland G.; Entingh, Timothy J.; Garmire, Gordon P.; Green, Roland; Janches, Diego; Kelly, Douglas A.

Proceedings of SPIE - The International Society for Optical Engineering. ed. / Oswald H. Siegmund; John V. Vallerga. Vol. 2518 1995. p. 141-162.

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

TY - GEN

T1 - CUBIC

T2 - EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy VI

AU - Burrows, David Nelson

AU - Skinner, Mark A.

AU - Broos, Patrick Sean

AU - Catalano, Mark A.

AU - Cawley, Laura J.

AU - Cocklin, Eric J.

AU - Engel, Leland G.

AU - Entingh, Timothy J.

AU - Garmire, Gordon P.

AU - Green, Roland

AU - Janches, Diego

AU - Kelly, Douglas A.

PY - 1995/12/1

Y1 - 1995/12/1

N2 - The cosmic unresolved background instrument using CCDs (CUBIC) is currently scheduled for launch on the Argentine/US SAC-B satellite late this year. This instrument is designed to perform moderate resolution nondispersive x-ray spectroscopy of the diffuse x-ray background over the band 0.2 - 10.0 keV using state-of-the-art photon-counting CCDs. The instrument is optimized for spectroscopy of diffuse emission with a field of view of 5 degrees by 5 degrees below 1 keV and 10 degrees by 10 degrees above 3 keV. Observations will typically last 1 - 3 days, and will obtain high quality CCD spectra of the diffuse background, nearby superbubbles and supernova remnants, and the brightest x-ray point sources. This paper gives an overview of the instrument design and CCD detectors.

AB - The cosmic unresolved background instrument using CCDs (CUBIC) is currently scheduled for launch on the Argentine/US SAC-B satellite late this year. This instrument is designed to perform moderate resolution nondispersive x-ray spectroscopy of the diffuse x-ray background over the band 0.2 - 10.0 keV using state-of-the-art photon-counting CCDs. The instrument is optimized for spectroscopy of diffuse emission with a field of view of 5 degrees by 5 degrees below 1 keV and 10 degrees by 10 degrees above 3 keV. Observations will typically last 1 - 3 days, and will obtain high quality CCD spectra of the diffuse background, nearby superbubbles and supernova remnants, and the brightest x-ray point sources. This paper gives an overview of the instrument design and CCD detectors.

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M3 - Conference contribution

AN - SCOPUS:0029546078

SN - 0819418773

SN - 9780819418777

VL - 2518

SP - 141

EP - 162

BT - Proceedings of SPIE - The International Society for Optical Engineering

A2 - Siegmund, Oswald H.

A2 - Vallerga, John V.

Y2 - 12 July 1995 through 14 July 1995

ER -