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J. Kaminski

Researcher at University of Bonn

Publications -  8
Citations -  462

J. Kaminski is an academic researcher from University of Bonn. The author has contributed to research in topics: Axion & Helioscope. The author has an hindex of 7, co-authored 8 publications receiving 357 citations.

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Conceptual design of the International Axion Observatory (IAXO)

Eric Armengaud, +87 more
TL;DR: The International Axion Observatory (IAXO) as mentioned in this paper is the most powerful axion helioscope, reaching sensitivity to axion-photon couplings down to a few × 10−12 GeV−1 and thus probing a large fraction of the currently unexplored axion and ALP parameter space.
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Conceptual Design of BabyIAXO, the intermediate stage towards the International Axion Observatory

A. Abeln, +131 more
TL;DR: The BabyIAXO project as mentioned in this paper is an intermediate experimental stage of the International Axion Observatory (IAAXO) proposed to be sited at DESY, which is a large-scale axion helioscope that will look for axions and axion-like particles produced in the Sun, with unprecedented sensitivity.
Journal ArticleDOI

Conceptual Design of BabyIAXO, the intermediate stage towards the International Axion Observatory

A. Abeln, +131 more
TL;DR: The BabyIAXO project as mentioned in this paper is an intermediate experimental stage of the International Axion Observatory (IAAXO) proposed to be sited at DESY, which is a large-scale axion helioscope that will look for axions and axion-like particles produced in the Sun, with unprecedented sensitivity.
Journal ArticleDOI

First results on the search for chameleons with the KWISP detector at CAST

TL;DR: In this paper, the authors report on the first measurement with a sensitive opto-mechanical force sensor designed for the direct detection of coupling of real chameleons to matter.
Journal ArticleDOI

Conceptual Design of the International Axion Observatory (IAXO)

Eric Armengaud, +87 more
TL;DR: The International Axion Observatory (IAXO) as discussed by the authors is the most powerful axion helioscope to date in terms of signal-to-noise ratio, reaching sensitivity to axion-photon couplings down to a few times 10 − 12 − 1 − 2 GeV$ − 1 /ε − 1/ε 2 ) and thus probing a large fraction of the currently unexplored axion and ALP parameter space.