Slewing Mirror Telescope optics for the early observation of UV/optical photons from Gamma-Ray Bursts

S. Jeong; J. W. Nam; K. B. Ahn; I. H. Park; S. W. Kim; J. Lee; H. Lim; Søren Brandt; Carl Budtz-Jørgensen; A. J. Castro-Tirado; P. Chen; M. H. Cho; J. N. Choi; B. Grossan; M. A. Huang; A.  Jung; J. E. Kim; M. B. Kim; Y. W. Kim; E. V. Linder; K. W. Min; G. W. Na; M. I. Panasyuk; J. Ripa; V. Reglero; G. F. Smoot; J. E. Suh; S.  Svertilov; N.  Vedenkin; I. Yashin

doi:10.1364/OE.21.002263

Slewing Mirror Telescope optics for the early observation of UV/optical photons from Gamma-Ray Bursts

S. Jeong
, J. W. Nam
, K. B. Ahn
, I. H. Park
, S. W. Kim
, J. Lee
, H. Lim
, Søren Brandt
, Carl Budtz-Jørgensen
, A. J. Castro-Tirado
, P. Chen
, M. H. Cho
, J. N. Choi
, B. Grossan
, M. A. Huang
, A. Jung
, J. E. Kim
, M. B. Kim
, Y. W. Kim
, E. V. Linder

K. W. Min, G. W. Na, M. I. Panasyuk, J. Ripa, V. Reglero, G. F. Smoot, J. E. Suh, S. Svertilov, N. Vedenkin, I. Yashin

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Abstract

We report on design, manufacture, and testing of a Slewing Mirror Telescope (SMT), the first of its kind and a part of Ultra-Fast Flash Observatory-pathfinder (UFFO-p) for space-based prompt measurement of early UV/optical light curves from Gamma-Ray Bursts (GRBs). Using a fast slewing mirror of 150 mm diameter mounted on a 2 axis gimbal stage, SMT can deliver the images of GRB optical counterparts to the intensified CCD detector within 1.5~1.8 s over ± 35 degrees in the slewing field of view. Its Ritchey-Chrétien telescope of 100 mm diameter provides a 17 × 17 arcmin2 instantaneous field of view. Technical details of design, construction, the laboratory performance tests in space environments for this unique SMT are described in conjunction with the plan for in-orbit operation onboard the Lomonosov satellite in 2013.

© 2013 OSA

Original language	English
Journal	Optics Express
Volume	21
Issue number	2
Pages (from-to)	2263-2278
ISSN	1094-4087
DOIs	https://doi.org/10.1364/OE.21.002263
Publication status	Published - 2013

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UFFO: Ultra-Fast Flash Observatory, UFFO
Brandt, S. (Project Participant), Budtz-Jørgensen, C. (Project Participant) & Lund, N. (Project Participant)
01/01/2010 → …
Project: Research

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Jeong, S., Nam, J. W., Ahn, K. B., Park, I. H., Kim, S. W., Lee, J., Lim, H., Brandt, S., Budtz-Jørgensen, C., Castro-Tirado, A. J., Chen, P., Cho, M. H., Choi, J. N., Grossan, B., Huang, M. A., Jung, A., Kim, J. E., Kim, M. B., Kim, Y. W., ... Yashin, I. (2013). Slewing Mirror Telescope optics for the early observation of UV/optical photons from Gamma-Ray Bursts. Optics Express, 21(2), 2263-2278. https://doi.org/10.1364/OE.21.002263

@article{5b4559411d0541f884b39439551eb2aa,

title = "Slewing Mirror Telescope optics for the early observation of UV/optical photons from Gamma-Ray Bursts",

abstract = "We report on design, manufacture, and testing of a Slewing Mirror Telescope (SMT), the first of its kind and a part of Ultra-Fast Flash Observatory-pathfinder (UFFO-p) for space-based prompt measurement of early UV/optical light curves from Gamma-Ray Bursts (GRBs). Using a fast slewing mirror of 150 mm diameter mounted on a 2 axis gimbal stage, SMT can deliver the images of GRB optical counterparts to the intensified CCD detector within 1.5\textasciitilde{}1.8 s over ± 35 degrees in the slewing field of view. Its Ritchey-Chr{\'e}tien telescope of 100 mm diameter provides a 17 × 17 arcmin2 instantaneous field of view. Technical details of design, construction, the laboratory performance tests in space environments for this unique SMT are described in conjunction with the plan for in-orbit operation onboard the Lomonosov satellite in 2013. {\textcopyright} 2013 OSA",

author = "S. Jeong and Nam, \{J. W.\} and Ahn, \{K. B.\} and Park, \{I. H.\} and Kim, \{S. W.\} and J. Lee and H. Lim and S{\o}ren Brandt and Carl Budtz-J{\o}rgensen and Castro-Tirado, \{A. J.\} and P. Chen and Cho, \{M. H.\} and Choi, \{J. N.\} and B. Grossan and Huang, \{M. A.\} and A. Jung and Kim, \{J. E.\} and Kim, \{M. B.\} and Kim, \{Y. W.\} and Linder, \{E. V.\} and Min, \{K. W.\} and Na, \{G. W.\} and Panasyuk, \{M. I.\} and J. Ripa and V. Reglero and Smoot, \{G. F.\} and Suh, \{J. E.\} and S. Svertilov and N. Vedenkin and I. Yashin",

year = "2013",

doi = "10.1364/OE.21.002263",

language = "English",

volume = "21",

pages = "2263--2278",

journal = "Optics Express",

issn = "1094-4087",

publisher = "Optica Publishing Group (formerly OSA)",

number = "2",

}

Jeong, S, Nam, JW, Ahn, KB, Park, IH, Kim, SW, Lee, J, Lim, H, Brandt, S , Budtz-Jørgensen, C, Castro-Tirado, AJ, Chen, P, Cho, MH, Choi, JN, Grossan, B, Huang, MA, Jung, A, Kim, JE, Kim, MB, Kim, YW, Linder, EV, Min, KW, Na, GW, Panasyuk, MI, Ripa, J, Reglero, V, Smoot, GF, Suh, JE, Svertilov, S, Vedenkin, N & Yashin, I 2013, 'Slewing Mirror Telescope optics for the early observation of UV/optical photons from Gamma-Ray Bursts', Optics Express, vol. 21, no. 2, pp. 2263-2278. https://doi.org/10.1364/OE.21.002263

TY - JOUR

T1 - Slewing Mirror Telescope optics for the early observation of UV/optical photons from Gamma-Ray Bursts

AU - Jeong, S.

AU - Nam, J. W.

AU - Ahn, K. B.

AU - Park, I. H.

AU - Kim, S. W.

AU - Lee, J.

AU - Lim, H.

AU - Brandt, Søren

AU - Budtz-Jørgensen, Carl

AU - Castro-Tirado, A. J.

AU - Chen, P.

AU - Cho, M. H.

AU - Choi, J. N.

AU - Grossan, B.

AU - Huang, M. A.

AU - Jung, A.

AU - Kim, J. E.

AU - Kim, M. B.

AU - Kim, Y. W.

AU - Linder, E. V.

AU - Min, K. W.

AU - Na, G. W.

AU - Panasyuk, M. I.

AU - Ripa, J.

AU - Reglero, V.

AU - Smoot, G. F.

AU - Suh, J. E.

AU - Svertilov, S.

AU - Vedenkin, N.

AU - Yashin, I.

PY - 2013

Y1 - 2013

N2 - We report on design, manufacture, and testing of a Slewing Mirror Telescope (SMT), the first of its kind and a part of Ultra-Fast Flash Observatory-pathfinder (UFFO-p) for space-based prompt measurement of early UV/optical light curves from Gamma-Ray Bursts (GRBs). Using a fast slewing mirror of 150 mm diameter mounted on a 2 axis gimbal stage, SMT can deliver the images of GRB optical counterparts to the intensified CCD detector within 1.5~1.8 s over ± 35 degrees in the slewing field of view. Its Ritchey-Chrétien telescope of 100 mm diameter provides a 17 × 17 arcmin2 instantaneous field of view. Technical details of design, construction, the laboratory performance tests in space environments for this unique SMT are described in conjunction with the plan for in-orbit operation onboard the Lomonosov satellite in 2013. © 2013 OSA

AB - We report on design, manufacture, and testing of a Slewing Mirror Telescope (SMT), the first of its kind and a part of Ultra-Fast Flash Observatory-pathfinder (UFFO-p) for space-based prompt measurement of early UV/optical light curves from Gamma-Ray Bursts (GRBs). Using a fast slewing mirror of 150 mm diameter mounted on a 2 axis gimbal stage, SMT can deliver the images of GRB optical counterparts to the intensified CCD detector within 1.5~1.8 s over ± 35 degrees in the slewing field of view. Its Ritchey-Chrétien telescope of 100 mm diameter provides a 17 × 17 arcmin2 instantaneous field of view. Technical details of design, construction, the laboratory performance tests in space environments for this unique SMT are described in conjunction with the plan for in-orbit operation onboard the Lomonosov satellite in 2013. © 2013 OSA

U2 - 10.1364/OE.21.002263

DO - 10.1364/OE.21.002263

M3 - Journal article

SN - 1094-4087

VL - 21

SP - 2263

EP - 2278

JO - Optics Express

JF - Optics Express

IS - 2

ER -

Slewing Mirror Telescope optics for the early observation of UV/optical photons from Gamma-Ray Bursts

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Projects

UFFO: Ultra-Fast Flash Observatory, UFFO

Cite this