The Swift Ultra-Violet/Optical Telescope

Peter W.A. Roming; S. D. Hunsberger; Keith O. Mason; John A. Nousek; Patrick S. Broos; Mary J. Carter; Barry K. Hancock; Howard E. Huckle; Tom E. Kennedy; Ronnie Killough; T. Scott Koch; Michael K. McLelland; Michael S. Pryzby; Phil J. Smith; Juan Carlos Soto; Joseph Stock; Patricia T. Boyd; Martin D. Still

doi:10.1117/12.504554

The Swift Ultra-Violet/Optical Telescope

Peter W.A. Roming
, S. D. Hunsberger
, Keith O. Mason
, John A. Nousek
, Patrick S. Broos
, Mary J. Carter
, Barry K. Hancock
, Howard E. Huckle
, Tom E. Kennedy
, Ronnie Killough
, T. Scott Koch
, Michael K. McLelland
, Michael S. Pryzby
, Phil J. Smith
, Juan Carlos Soto
, Joseph Stock
, Patricia T. Boyd
, Martin D. Still

Astronomy & Astrophysics

Research output: Contribution to journal › Conference article › peer-review

49 Scopus citations

Abstract

The UV/optical telescope (UVOT) is one of three instruments flying aboard the Swift Gamma-ray Observatory. It is designed to capture the early (∼1 minute) UV and optical photons from the afterglow of gamma-ray bursts as well as long term observations of these afterglows. This is accomplished through the use of UV and optical broadband filters and grisms. The UVOT has a modified Ritchey-Chrétien design with micro-channel plate intensified charged-coupled device detectors that provide sub-arcsecond imaging. Unlike most UV/optical telescopes the UVOT can operate in a photon-counting mode as well as an imaging mode. We discuss some of the science to be pursued by the UVOT and the overall design of the instrument.

Original language	English (US)
Pages (from-to)	262-276
Number of pages	15
Journal	Proceedings of SPIE - The International Society for Optical Engineering
Volume	5165
DOIs	https://doi.org/10.1117/12.504554
State	Published - 2004
Event	X-Ray and Gamma-Ray Instrumentation for Astronomy XIII - San Diego, CA, United States Duration: Aug 3 2003 → Aug 5 2003

All Science Journal Classification (ASJC) codes

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

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10.1117/12.504554

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Roming, P. W. A., Hunsberger, S. D., Mason, K. O., Nousek, J. A., Broos, P. S., Carter, M. J., Hancock, B. K., Huckle, H. E., Kennedy, T. E., Killough, R., Koch, T. S., McLelland, M. K., Pryzby, M. S., Smith, P. J., Soto, J. C., Stock, J., Boyd, P. T., & Still, M. D. (2004). The Swift Ultra-Violet/Optical Telescope. Proceedings of SPIE - The International Society for Optical Engineering, 5165, 262-276. https://doi.org/10.1117/12.504554

@article{3cc6b180e9ad4760b13cc30d4816cf11,

title = "The Swift Ultra-Violet/Optical Telescope",

abstract = "The UV/optical telescope (UVOT) is one of three instruments flying aboard the Swift Gamma-ray Observatory. It is designed to capture the early (∼1 minute) UV and optical photons from the afterglow of gamma-ray bursts as well as long term observations of these afterglows. This is accomplished through the use of UV and optical broadband filters and grisms. The UVOT has a modified Ritchey-Chr{\'e}tien design with micro-channel plate intensified charged-coupled device detectors that provide sub-arcsecond imaging. Unlike most UV/optical telescopes the UVOT can operate in a photon-counting mode as well as an imaging mode. We discuss some of the science to be pursued by the UVOT and the overall design of the instrument.",

author = "Roming, \{Peter W.A.\} and Hunsberger, \{S. D.\} and Mason, \{Keith O.\} and Nousek, \{John A.\} and Broos, \{Patrick S.\} and Carter, \{Mary J.\} and Hancock, \{Barry K.\} and Huckle, \{Howard E.\} and Kennedy, \{Tom E.\} and Ronnie Killough and Koch, \{T. Scott\} and McLelland, \{Michael K.\} and Pryzby, \{Michael S.\} and Smith, \{Phil J.\} and Soto, \{Juan Carlos\} and Joseph Stock and Boyd, \{Patricia T.\} and Still, \{Martin D.\}",

year = "2004",

doi = "10.1117/12.504554",

language = "English (US)",

volume = "5165",

pages = "262--276",

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

issn = "0277-786X",

publisher = "SPIE",

note = "X-Ray and Gamma-Ray Instrumentation for Astronomy XIII ; Conference date: 03-08-2003 Through 05-08-2003",

}

Roming, PWA, Hunsberger, SD, Mason, KO, Nousek, JA, Broos, PS, Carter, MJ, Hancock, BK, Huckle, HE, Kennedy, TE, Killough, R, Koch, TS, McLelland, MK, Pryzby, MS, Smith, PJ, Soto, JC, Stock, J, Boyd, PT & Still, MD 2004, 'The Swift Ultra-Violet/Optical Telescope', Proceedings of SPIE - The International Society for Optical Engineering, vol. 5165, pp. 262-276. https://doi.org/10.1117/12.504554

TY - JOUR

T1 - The Swift Ultra-Violet/Optical Telescope

AU - Roming, Peter W.A.

AU - Hunsberger, S. D.

AU - Mason, Keith O.

AU - Nousek, John A.

AU - Broos, Patrick S.

AU - Carter, Mary J.

AU - Hancock, Barry K.

AU - Huckle, Howard E.

AU - Kennedy, Tom E.

AU - Killough, Ronnie

AU - Koch, T. Scott

AU - McLelland, Michael K.

AU - Pryzby, Michael S.

AU - Smith, Phil J.

AU - Soto, Juan Carlos

AU - Stock, Joseph

AU - Boyd, Patricia T.

AU - Still, Martin D.

PY - 2004

Y1 - 2004

N2 - The UV/optical telescope (UVOT) is one of three instruments flying aboard the Swift Gamma-ray Observatory. It is designed to capture the early (∼1 minute) UV and optical photons from the afterglow of gamma-ray bursts as well as long term observations of these afterglows. This is accomplished through the use of UV and optical broadband filters and grisms. The UVOT has a modified Ritchey-Chrétien design with micro-channel plate intensified charged-coupled device detectors that provide sub-arcsecond imaging. Unlike most UV/optical telescopes the UVOT can operate in a photon-counting mode as well as an imaging mode. We discuss some of the science to be pursued by the UVOT and the overall design of the instrument.

AB - The UV/optical telescope (UVOT) is one of three instruments flying aboard the Swift Gamma-ray Observatory. It is designed to capture the early (∼1 minute) UV and optical photons from the afterglow of gamma-ray bursts as well as long term observations of these afterglows. This is accomplished through the use of UV and optical broadband filters and grisms. The UVOT has a modified Ritchey-Chrétien design with micro-channel plate intensified charged-coupled device detectors that provide sub-arcsecond imaging. Unlike most UV/optical telescopes the UVOT can operate in a photon-counting mode as well as an imaging mode. We discuss some of the science to be pursued by the UVOT and the overall design of the instrument.

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DO - 10.1117/12.504554

M3 - Conference article

AN - SCOPUS:11144358206

SN - 0277-786X

VL - 5165

SP - 262

EP - 276

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

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

T2 - X-Ray and Gamma-Ray Instrumentation for Astronomy XIII

Y2 - 3 August 2003 through 5 August 2003

ER -

The Swift Ultra-Violet/Optical Telescope

Abstract

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