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@INPROCEEDINGS{Minowa:297014,
author = {Minowa, M. and Inoue, Y. and Akimoto, Y. and Ohta, R. and
Mizumoto, T. and Yamamoto, A.},
title = {{T}okyo {A}xion {H}elioscope},
address = {Hamburg},
publisher = {Deutsches Elektronen-Synchrotron, DESY},
reportid = {PUBDB-2016-01767, arXiv:0809.0596. RESCEU-53-08},
pages = {39-42},
year = {2009},
abstract = {A new search result of the Tokyo axion helioscope is
presented. The axion helioscope consists of a dedicated
cryogen-free 4T superconducting magnet with an effective
length of 2.3 m and PIN photodiodes as x-ray detectors.
Solar axions, if exist, would be converted into X-ray
photons through the inverse Primakoff process in the
magnetic field. Conversion is coherently enhanced even for
massive axions by filling the conversion region with helium
gas. The present third phase measurement sets a new limit of
$g_{a\gamma\gamma}<(5.6--13.4)\times10^{-10}$ $GeV^{-1}$ for
the axion mass of $0.84<m_a<1.0$ eV at $95\%$ confidence
level.},
month = {Jun},
date = {2008-06-18},
organization = {4th Patras Workshop on Axions, WIMPs
and WISPs, Hamburg (Germany), 18 Jun
2008 - 21 Jun 2008},
cin = {L},
cid = {I:(DE-H253)L-20120731},
pnm = {899 - ohne Topic (POF3-899)},
pid = {G:(DE-HGF)POF3-899},
experiment = {EXP:(DE-H253)HERA(machine)-20150101},
typ = {PUB:(DE-HGF)8 / PUB:(DE-HGF)15},
eprint = {0809.0596},
howpublished = {arXiv:0809.0596},
archivePrefix = {arXiv},
SLACcitation = {$\%\%CITATION$ = $arXiv:0809.0596;\%\%$},
UT = {WOS:00},
doi = {10.3204/DESY-PROC-2008-02/minowa_makoto},
url = {https://bib-pubdb1.desy.de/record/297014},
}