The slewing mirror telescope and the data-acquisition system for the UFFO-pathfinder

H. Lim; S. Ahmad; P. Barrillon; S. Brandt; C. Budtz-Jørgensen; A. J. Castro-Tirado; P. Chen; Y. J. Choi; P. Connell; S. Dagoret-Campagne; C. Eyles; B. Grossan; M. H.A.Huang Huang; A. Jung; S. Jeong; J. E. Kim; M. B. Kim; S. W. Kim; Y. W. Kim; A. S. Krasnov; J. Lee; E. V. Linder; T. C. Liu; N. Lund; K. W. Min; G. W. Na; J. W. Nam; M. I. Panasyuk; I. H. Park; J. Ripa; V. Reglero; J. M. Rodrigo; G. F. Smoot; J. E. Suh; S. Svertilov; N. Vedenkin; M. Z. Wang; I. Yashin

doi:10.1051/eas/1361087

The slewing mirror telescope and the data-acquisition system for the UFFO-pathfinder

H. Lim^*, S. Ahmad, P. Barrillon, S. Brandt, C. Budtz-Jørgensen, A. J. Castro-Tirado, P. Chen, Y. J. Choi, P. Connell, S. Dagoret-Campagne, C. Eyles, B. Grossan, M. H.A.Huang Huang, A. Jung, S. Jeong, J. E. Kim, M. B. Kim, S. W. Kim, Y. W. Kim, A. S. KrasnovJ. Lee, E. V. Linder, T. C. Liu, N. Lund, K. W. Min, G. W. Na, J. W. Nam, M. I. Panasyuk, I. H. Park, J. Ripa, V. Reglero, J. M. Rodrigo, G. F. Smoot, J. E. Suh, S. Svertilov, N. Vedenkin, M. Z. Wang, I. Yashin

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電子物理學系

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摘要

The Ultra-Fast Flash Observatory (UFFO) aims to detect the earliest moment of Gamma-Ray Bursts (GRBs) which is not well known, resulting into the enhancement of GRB mechanism understanding. The pathfinder mission was proposed to be a scaled-down version of UFFO, and only contains the UFFO Burst Alert & Trigger Telescope (UBAT) measuring the X-ray/gamma-ray with the wide-field of view and the Slewing Mirror Telescope (SMT) with a rapid-response for the UV/optical photons. Once the UBAT detects a GRB candidate with the position accuracy of 10 arcmin, the SMT steers the UV/optical photons from the candidate to the telescope by the fast rotatable mirror and provides the early UV/optical photons measurements with 4 arcsec accuracy. The SMT has a modified Ritchey-Chrètien telescope with the aperture size of 10 cm diameter including the rotatable mirror and the image readout by the intensified charge-coupled device. There is a key board called the UFFO Data Acquisition system (UDAQ) that manages the communication of each telescope and also of the satellite and the UFFO overall operation. This pathfinder is designed and built within the limited size and weight of ∼20 kg and the low power consumption up to ∼30 W. We will discuss the design and performance of the UFFO-pathfinder, and its integration to the Lomonosov satellite.

原文	English
頁（從 - 到）	537-543
頁數	7
期刊	EAS Publications Series
卷	61
DOIs	https://doi.org/10.1051/eas/1361087
出版狀態	Published - 2013
事件	2012 Gamma-Ray Burst Symposium, GRB 2012 - Malaga, 西班牙持續時間: 8 10月 2012 → 12 10月 2012

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Lim, H., Ahmad, S., Barrillon, P., Brandt, S., Budtz-Jørgensen, C., Castro-Tirado, A. J., Chen, P., Choi, Y. J., Connell, P., Dagoret-Campagne, S., Eyles, C., Grossan, B., Huang, M. H. A. H., Jung, A., Jeong, S., Kim, J. E., Kim, M. B., Kim, S. W., Kim, Y. W., ... Yashin, I. (2013). The slewing mirror telescope and the data-acquisition system for the UFFO-pathfinder. EAS Publications Series, 61, 537-543. https://doi.org/10.1051/eas/1361087

@article{c0b8962b246c4c11b3f20bdb3cefcc7d,

title = "The slewing mirror telescope and the data-acquisition system for the UFFO-pathfinder",

abstract = "The Ultra-Fast Flash Observatory (UFFO) aims to detect the earliest moment of Gamma-Ray Bursts (GRBs) which is not well known, resulting into the enhancement of GRB mechanism understanding. The pathfinder mission was proposed to be a scaled-down version of UFFO, and only contains the UFFO Burst Alert & Trigger Telescope (UBAT) measuring the X-ray/gamma-ray with the wide-field of view and the Slewing Mirror Telescope (SMT) with a rapid-response for the UV/optical photons. Once the UBAT detects a GRB candidate with the position accuracy of 10 arcmin, the SMT steers the UV/optical photons from the candidate to the telescope by the fast rotatable mirror and provides the early UV/optical photons measurements with 4 arcsec accuracy. The SMT has a modified Ritchey-Chr{\`e}tien telescope with the aperture size of 10 cm diameter including the rotatable mirror and the image readout by the intensified charge-coupled device. There is a key board called the UFFO Data Acquisition system (UDAQ) that manages the communication of each telescope and also of the satellite and the UFFO overall operation. This pathfinder is designed and built within the limited size and weight of ∼20 kg and the low power consumption up to ∼30 W. We will discuss the design and performance of the UFFO-pathfinder, and its integration to the Lomonosov satellite.",

author = "H. Lim and S. Ahmad and P. Barrillon and S. Brandt and C. Budtz-J{\o}rgensen and Castro-Tirado, {A. J.} and P. Chen and Choi, {Y. J.} and P. Connell and S. Dagoret-Campagne and C. Eyles and B. Grossan and Huang, {M. H.A.Huang} and A. Jung and S. Jeong and Kim, {J. E.} and Kim, {M. B.} and Kim, {S. W.} and Kim, {Y. W.} and Krasnov, {A. S.} and J. Lee and Linder, {E. V.} and Liu, {T. C.} and N. Lund and Min, {K. W.} and Na, {G. W.} and Nam, {J. W.} and Panasyuk, {M. I.} and Park, {I. H.} and J. Ripa and V. Reglero and Rodrigo, {J. M.} and Smoot, {G. F.} and Suh, {J. E.} and S. Svertilov and N. Vedenkin and Wang, {M. Z.} and I. Yashin",

year = "2013",

doi = "10.1051/eas/1361087",

language = "English",

volume = "61",

pages = "537--543",

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",

}

Lim, H, Ahmad, S, Barrillon, P, Brandt, S, Budtz-Jørgensen, C, Castro-Tirado, AJ, Chen, P, Choi, YJ, Connell, P, Dagoret-Campagne, S, Eyles, C, Grossan, B, Huang, MHAH, Jung, A, Jeong, S, Kim, JE, Kim, MB, Kim, SW, Kim, YW, Krasnov, AS, Lee, J, Linder, EV, Liu, TC, Lund, N, Min, KW, Na, GW, Nam, JW, Panasyuk, MI, Park, IH, Ripa, J, Reglero, V, Rodrigo, JM, Smoot, GF, Suh, JE, Svertilov, S, Vedenkin, N, Wang, MZ & Yashin, I 2013, 'The slewing mirror telescope and the data-acquisition system for the UFFO-pathfinder', EAS Publications Series, 卷 61, 頁 537-543. https://doi.org/10.1051/eas/1361087

TY - JOUR

T1 - The slewing mirror telescope and the data-acquisition system for the UFFO-pathfinder

AU - Lim, H.

AU - Ahmad, S.

AU - Barrillon, P.

AU - Brandt, S.

AU - Budtz-Jørgensen, C.

AU - Castro-Tirado, A. J.

AU - Chen, P.

AU - Choi, Y. J.

AU - Connell, P.

AU - Dagoret-Campagne, S.

AU - Eyles, C.

AU - Grossan, B.

AU - Huang, M. H.A.Huang

AU - Jung, A.

AU - Jeong, S.

AU - Kim, J. E.

AU - Kim, M. B.

AU - Kim, S. W.

AU - Kim, Y. W.

AU - Krasnov, A. S.

AU - Lee, J.

AU - Linder, E. V.

AU - Liu, T. C.

AU - Lund, N.

AU - Min, K. W.

AU - Na, G. W.

AU - Nam, J. W.

AU - Panasyuk, M. I.

AU - Park, I. H.

AU - Ripa, J.

AU - Reglero, V.

AU - Rodrigo, J. M.

AU - Smoot, G. F.

AU - Suh, J. E.

AU - Svertilov, S.

AU - Vedenkin, N.

AU - Wang, M. Z.

AU - Yashin, I.

PY - 2013

Y1 - 2013

N2 - The Ultra-Fast Flash Observatory (UFFO) aims to detect the earliest moment of Gamma-Ray Bursts (GRBs) which is not well known, resulting into the enhancement of GRB mechanism understanding. The pathfinder mission was proposed to be a scaled-down version of UFFO, and only contains the UFFO Burst Alert & Trigger Telescope (UBAT) measuring the X-ray/gamma-ray with the wide-field of view and the Slewing Mirror Telescope (SMT) with a rapid-response for the UV/optical photons. Once the UBAT detects a GRB candidate with the position accuracy of 10 arcmin, the SMT steers the UV/optical photons from the candidate to the telescope by the fast rotatable mirror and provides the early UV/optical photons measurements with 4 arcsec accuracy. The SMT has a modified Ritchey-Chrètien telescope with the aperture size of 10 cm diameter including the rotatable mirror and the image readout by the intensified charge-coupled device. There is a key board called the UFFO Data Acquisition system (UDAQ) that manages the communication of each telescope and also of the satellite and the UFFO overall operation. This pathfinder is designed and built within the limited size and weight of ∼20 kg and the low power consumption up to ∼30 W. We will discuss the design and performance of the UFFO-pathfinder, and its integration to the Lomonosov satellite.

AB - The Ultra-Fast Flash Observatory (UFFO) aims to detect the earliest moment of Gamma-Ray Bursts (GRBs) which is not well known, resulting into the enhancement of GRB mechanism understanding. The pathfinder mission was proposed to be a scaled-down version of UFFO, and only contains the UFFO Burst Alert & Trigger Telescope (UBAT) measuring the X-ray/gamma-ray with the wide-field of view and the Slewing Mirror Telescope (SMT) with a rapid-response for the UV/optical photons. Once the UBAT detects a GRB candidate with the position accuracy of 10 arcmin, the SMT steers the UV/optical photons from the candidate to the telescope by the fast rotatable mirror and provides the early UV/optical photons measurements with 4 arcsec accuracy. The SMT has a modified Ritchey-Chrètien telescope with the aperture size of 10 cm diameter including the rotatable mirror and the image readout by the intensified charge-coupled device. There is a key board called the UFFO Data Acquisition system (UDAQ) that manages the communication of each telescope and also of the satellite and the UFFO overall operation. This pathfinder is designed and built within the limited size and weight of ∼20 kg and the low power consumption up to ∼30 W. We will discuss the design and performance of the UFFO-pathfinder, and its integration to the Lomonosov satellite.

UR - http://www.scopus.com/inward/record.url?scp=84887103275&partnerID=8YFLogxK

U2 - 10.1051/eas/1361087

DO - 10.1051/eas/1361087

M3 - Conference article

AN - SCOPUS:84887103275

SN - 1633-4760

VL - 61

SP - 537

EP - 543

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 -

The slewing mirror telescope and the data-acquisition system for the UFFO-pathfinder

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