Development of slewing mirror telescope optical system for the uffo-pathfinder

S. Jeong; J. W. Nam; K. B. Ahn; I. H. Park; S. W. Kim; J. Lee; H. Lim; S. Brandt; C. 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:10.1051/eas/1361090

Development of slewing mirror telescope optical system for the uffo-pathfinder

S. Jeong, J. W. Nam, K. B. Ahn, I. H. Park, S. W. Kim, J. Lee, H. Lim, S. Brandt, C. 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. LinderK. W. Min, G. W. Na, M. I. Panasyuk, J. Ripa, V. Reglero, G. F. Smoot, J. E. Suh, S. Svertilov, N. Vedenkin, I. Yashin

Institute of Earth·Atmosphere·Astronomy(BK21+)

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

Abstract

The Slewing Mirror Telescope (SMT) is the UV/optical telescope of UFFO-pathfinder. The SMT optical system is a Ritchey-Chrétien (RC) telescope of 100 mm diameter pointed by means of a gimbal-mounted flat mirror in front of the telescope. The RC telescope has a 17 × 17arcmin² in Field of View and 4.3 arcsec resolution (full width half maximum of the point spread function) The beam-steering mirror enables the SMT to access a 35 × 35degree region and point and settle within 1 sec. All mirrors were fabricated to about 0.02 wavelengths RMS in wave front error (WFE) and 84.7% average reflectivity over 200 nm ∼ 650 nm. The RC telescope was aligned to 0.05 wavelengths RMS in WFE (test wavelength 632.8 nm). In this paper, the technical details of the RC telescope and slewing mirror system assembly, integration, and testing are given shortly, and performance tests of the full SMT optical system are reported.

Original language	English
Pages (from-to)	561-565
Number of pages	5
Journal	EAS Publications Series
Volume	61
DOIs	https://doi.org/10.1051/eas/1361090
Publication status	Published - 2013
Event	2012 Gamma-Ray Burst Symposium, GRB 2012 - Malaga, Spain Duration: 2012 Oct 8 → 2012 Oct 12

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Engineering(all)
Space and Planetary Science

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10.1051/eas/1361090

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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). Development of slewing mirror telescope optical system for the uffo-pathfinder. EAS Publications Series, 61, 561-565. https://doi.org/10.1051/eas/1361090

@article{4e1d9a6041f9430a8ce9f7861941c4ce,

title = "Development of slewing mirror telescope optical system for the uffo-pathfinder",

abstract = "The Slewing Mirror Telescope (SMT) is the UV/optical telescope of UFFO-pathfinder. The SMT optical system is a Ritchey-Chr{\'e}tien (RC) telescope of 100 mm diameter pointed by means of a gimbal-mounted flat mirror in front of the telescope. The RC telescope has a 17 × 17arcmin2 in Field of View and 4.3 arcsec resolution (full width half maximum of the point spread function) The beam-steering mirror enables the SMT to access a 35 × 35degree region and point and settle within 1 sec. All mirrors were fabricated to about 0.02 wavelengths RMS in wave front error (WFE) and 84.7% average reflectivity over 200 nm ∼ 650 nm. The RC telescope was aligned to 0.05 wavelengths RMS in WFE (test wavelength 632.8 nm). In this paper, the technical details of the RC telescope and slewing mirror system assembly, integration, and testing are given shortly, and performance tests of the full SMT optical system are reported.",

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. Brandt and C. 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 = "10.1051/eas/1361090",

language = "English",

volume = "61",

pages = "561--565",

journal = "EAS Publications Series",

issn = "1633-4760",

publisher = "EDP Sciences",

note = "2012 Gamma-Ray Burst Symposium, GRB 2012 ; Conference date: 08-10-2012 Through 12-10-2012",

}

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, 'Development of slewing mirror telescope optical system for the uffo-pathfinder', EAS Publications Series, vol. 61, pp. 561-565. https://doi.org/10.1051/eas/1361090

TY - JOUR

T1 - Development of slewing mirror telescope optical system for the uffo-pathfinder

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, S.

AU - Budtz-Jørgensen, C.

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 - The Slewing Mirror Telescope (SMT) is the UV/optical telescope of UFFO-pathfinder. The SMT optical system is a Ritchey-Chrétien (RC) telescope of 100 mm diameter pointed by means of a gimbal-mounted flat mirror in front of the telescope. The RC telescope has a 17 × 17arcmin2 in Field of View and 4.3 arcsec resolution (full width half maximum of the point spread function) The beam-steering mirror enables the SMT to access a 35 × 35degree region and point and settle within 1 sec. All mirrors were fabricated to about 0.02 wavelengths RMS in wave front error (WFE) and 84.7% average reflectivity over 200 nm ∼ 650 nm. The RC telescope was aligned to 0.05 wavelengths RMS in WFE (test wavelength 632.8 nm). In this paper, the technical details of the RC telescope and slewing mirror system assembly, integration, and testing are given shortly, and performance tests of the full SMT optical system are reported.

AB - The Slewing Mirror Telescope (SMT) is the UV/optical telescope of UFFO-pathfinder. The SMT optical system is a Ritchey-Chrétien (RC) telescope of 100 mm diameter pointed by means of a gimbal-mounted flat mirror in front of the telescope. The RC telescope has a 17 × 17arcmin2 in Field of View and 4.3 arcsec resolution (full width half maximum of the point spread function) The beam-steering mirror enables the SMT to access a 35 × 35degree region and point and settle within 1 sec. All mirrors were fabricated to about 0.02 wavelengths RMS in wave front error (WFE) and 84.7% average reflectivity over 200 nm ∼ 650 nm. The RC telescope was aligned to 0.05 wavelengths RMS in WFE (test wavelength 632.8 nm). In this paper, the technical details of the RC telescope and slewing mirror system assembly, integration, and testing are given shortly, and performance tests of the full SMT optical system are reported.

UR - http://www.scopus.com/inward/record.url?scp=84887086086&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84887086086&partnerID=8YFLogxK

U2 - 10.1051/eas/1361090

DO - 10.1051/eas/1361090

M3 - Conference article

AN - SCOPUS:84887086086

SN - 1633-4760

VL - 61

SP - 561

EP - 565

JO - EAS Publications Series

JF - EAS Publications Series

T2 - 2012 Gamma-Ray Burst Symposium, GRB 2012

Y2 - 8 October 2012 through 12 October 2012

ER -

Development of slewing mirror telescope optical system for the uffo-pathfinder

Abstract

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