Editing CERN Axion Solar Telescope (section)

=== KWISP detector ===
KWISP at CAST is designed to detect the coupling of solar chameleons with matter particles. It uses a very sensitive [[Optomechanics|optomechanical]] force sensor, capable of detecting a displacement in a thin membrane caused by the mechanical effects from the solar chameleon interactions.<ref name=":7">{{cite journal | last1=Arguedas Cuendis | first1=S. | last2=Baier | first2=J. | last3=Barth | first3=K. | last4=Baum | first4=S. | last5=Bayirli | first5=A. | last6=Belov | first6=A. | last7=Bräuninger | first7=H. | last8=Cantatore | first8=G. | last9=Carmona | first9=J.M. | last10=Castel | first10=J.F. | last11=Cetin | first11=S.A. | last12=Dafni | first12=T. | last13=Davenport | first13=M. | last14=Dermenev | first14=A. | last15=Desch | first15=K. | last16=Döbrich | first16=B. | last17=Fischer | first17=H. | last18=Funk | first18=W. | last19=García | first19=J.A. | last20=Gardikiotis | first20=A. | last21=Garza | first21=J.G. | last22=Gninenko | first22=S. | last23=Hasinoff | first23=M.D. | last24=Hoffmann | first24=D.H.H. | last25=Iguaz | first25=F.J. | last26=Irastorza | first26=I.G. | last27=Jakovčić | first27=K. | last28=Kaminski | first28=J. | last29=Karuza | first29=M. | last30=Krieger | first30=C. | last31=Lakić | first31=B. | last32=Laurent | first32=J.M. | last33=Luzón | first33=G. | last34=Maroudas | first34=M. | last35=Miceli | first35=L. | last36=Neff | first36=S. | last37=Ortega | first37=I. | last38=Ozbey | first38=A. | last39=Pivovaroff | first39=M.J. | last40=Rosu | first40=M. | last41=Ruz | first41=J. | last42=Chóliz | first42=E. Ruiz | last43=Schmidt | first43=S. | last44=Schumann | first44=M. | last45=Semertzidis | first45=Y.K. | last46=Solanki | first46=S.K. | last47=Stewart | first47=L. | last48=Tsagris | first48=I. | last49=Vafeiadis | first49=T. | last50=Vogel | first50=J.K. | last51=Vretenar | first51=M. | last52=Yildiz | first52=S.C. | last53=Zioutas | first53=K. | title=First results on the search for chameleons with the KWISP detector at CAST | journal=Physics of the Dark Universe | publisher=Elsevier BV | volume=26 | year=2019 | issn=2212-6864 | doi=10.1016/j.dark.2019.100367 | page=100367 |arxiv=1906.01084|bibcode=2019PDU....2600367A|s2cid=174798025 |display-authors=3}}</ref><ref>{{cite journal | last1=Karuza | first1=M. | last2=Cantatore | first2=G. | last3=Gardikiotis | first3=A. | last4=Hoffmann | first4=D.H.H. | last5=Semertzidis | first5=Y.K. | last6=Zioutas | first6=K. | title=KWISP: An ultra-sensitive force sensor for the Dark Energy sector | journal=Physics of the Dark Universe | publisher=Elsevier BV | volume=12 | year=2016 | issn=2212-6864 | doi=10.1016/j.dark.2016.02.004 | pages=100–104|arxiv=1509.04499|bibcode=2016PDU....12..100K|s2cid=119255228}}</ref><ref name=":2" />