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In-Flight Calibrations of UFFO-Pathfinder

Published online by Cambridge University Press:  22 July 2013

J. Řípa ,
S. Ahmad ,
P. Barrillon ,
S. Brandt ,
C. Budtz-Jørgensen ,
A.J. Castro-Tirado ,
S.-H. Chang ,
Y.-Y. Chang ,
C.R. Chen  and
P. Chen
...Show all authors
J. Řípa
Affiliation:
Sungkyunkwan University, Suwon, South Korea;. e-mail: [email protected]
S. Ahmad
Affiliation:
Laboratoire de l’Accélérateur Linéaire, University of Paris-Sud 11, Orsay, France
P. Barrillon
Affiliation:
Laboratoire de l’Accélérateur Linéaire, University of Paris-Sud 11, Orsay, France
S. Brandt
Affiliation:
Technical University of Denmark, Copenhagen, Denmark
C. Budtz-Jørgensen
Affiliation:
Technical University of Denmark, Copenhagen, Denmark
A.J. Castro-Tirado
Affiliation:
Instituto de Astrofsica de Andalucía, CSIC, Granada, Spain
S.-H. Chang
Affiliation:
National Space Organization, Taiwan
Y.-Y. Chang
Affiliation:
LeCosPA, National Taiwan University, Taipei, Taiwan
C.R. Chen
Affiliation:
National Space Organization, Taiwan
P. Chen
Affiliation:
LeCosPA, National Taiwan University, Taipei, Taiwan
H.S. Choi
Affiliation:
Korea Institute of Industrial Technology, Cheonan, South Korea
Y.J. Choi
Affiliation:
Department of Physics, Korea Advanced Institute of Science and Technology, Daejeon, South Korea
P. Connell
Affiliation:
University of Valencia, Valencia, Spain
S. Dagoret-Campagne
Affiliation:
Laboratoire de l’Accélérateur Linéaire, University of Paris-Sud 11, Orsay, France
C. Eyles
Affiliation:
University of Valencia, Valencia, Spain
B. Grossan
Affiliation:
Institute for the Early Universe, Ewha Womans University, Seoul, South Korea
J.J. Huang
Affiliation:
LeCosPA, National Taiwan University, Taipei, Taiwan
M.-H.A. Huang
Affiliation:
National United University, Miao-Li, Taiwan
S. Jeong
Affiliation:
Department of Physics, Ewha Womans University, Seoul, South Korea
A. Jung
Affiliation:
Department of Physics, Ewha Womans University, Seoul, South Korea
J.-E. Kim
Affiliation:
Department of Physics, Ewha Womans University, Seoul, South Korea
M.-B. Kim
Affiliation:
Sungkyunkwan University, Suwon, South Korea;. e-mail: [email protected]
S.-W. Kim
Affiliation:
Department of Astronomy, Yonsei University, Seoul, South Korea
Y.-W. Kim
Affiliation:
Sungkyunkwan University, Suwon, South Korea;. e-mail: [email protected]
A.S. Krasnov
Affiliation:
SINP, Moscow State University, Moscow, Russia
J. Lee
Affiliation:
Sungkyunkwan University, Suwon, South Korea;. e-mail: [email protected]
H. Lim
Affiliation:
Sungkyunkwan University, Suwon, South Korea;. e-mail: [email protected]
C.-Y. Lin
Affiliation:
National Space Organization, Taiwan
E.V. Linder
Affiliation:
Institute for the Early Universe, Ewha Womans University, Seoul, South Korea
T.-C. Liu
Affiliation:
LeCosPA, National Taiwan University, Taipei, Taiwan
N. Lund
Affiliation:
Technical University of Denmark, Copenhagen, Denmark
K.W. Min
Affiliation:
Department of Physics, Korea Advanced Institute of Science and Technology, Daejeon, South Korea
G.-W. Na
Affiliation:
Department of Physics, Ewha Womans University, Seoul, South Korea
J.-W. Nam
Affiliation:
LeCosPA, National Taiwan University, Taipei, Taiwan
M.I. Panasyuk
Affiliation:
SINP, Moscow State University, Moscow, Russia
I.H. Park
Affiliation:
Sungkyunkwan University, Suwon, South Korea;. e-mail: [email protected]
V. Reglero
Affiliation:
University of Valencia, Valencia, Spain
J.M. Rodrigo
Affiliation:
University of Valencia, Valencia, Spain
G.F. Smoot
Affiliation:
Institute for the Early Universe, Ewha Womans University, Seoul, South Korea
J.-E. Suh
Affiliation:
Department of Physics, Ewha Womans University, Seoul, South Korea
S. Svertilov
Affiliation:
SINP, Moscow State University, Moscow, Russia
N. Vedenkin
Affiliation:
SINP, Moscow State University, Moscow, Russia
M.-Z. Wang
Affiliation:
LeCosPA, National Taiwan University, Taipei, Taiwan
I. Yashin
Affiliation:
SINP, Moscow State University, Moscow, Russia
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Abstract

The Ultra-Fast Flash Observatory (UFFO), which will be launched onboard theLomonosov spacecraft, contains two crucial instruments: UFFO BurstAlert & Trigger Telescope (UBAT) for detection and localization of Gamma-Ray Bursts(GRBs) and the fast-response Slewing Mirror Telescope (SMT) designed for the observationof the prompt optical/UV counterparts. Here we discuss the in-space calibrations of theUBAT detector and SMT telescope. After the launch, the observations of the standard X-raysources such as pulsar in Crab nebula will provide data for necessary calibrations ofUBAT. Several standard stars will be used for the photometric calibration of SMT. Thecelestial X-ray sources, e.g. X-ray binaries with bright optical sourcesin their close angular vicinity will serve for the cross-calibration of UBAT and SMT.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 61: Gamma-ray Bursts: 15 Years of GRB Afterglows – Progenitors, Environments and Host Galaxies from the Nearby to the Early Universe , 2013 , pp. 579 - 581
Copyright
© EAS, EDP Sciences 2013

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References

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