A search for solar axion induced signals with COSINE-100. (arXiv:1904.06860v1 [hep-ex])
<a href="http://arxiv.org/find/hep-ex/1/au:+Adhikari_P/0/1/0/all/0/1">P. Adhikari</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Adhikari_G/0/1/0/all/0/1">G. Adhikari</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Souza_E/0/1/0/all/0/1">E. Barbosa de Souza</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Carlin_N/0/1/0/all/0/1">N. Carlin</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Choi_S/0/1/0/all/0/1">S. Choi</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Djamal_M/0/1/0/all/0/1">M. Djamal</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Ezeribe_A/0/1/0/all/0/1">A.C. Ezeribe</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Ha_C/0/1/0/all/0/1">C. Ha</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Hahn_I/0/1/0/all/0/1">I.S. Hahn</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Jeon_E/0/1/0/all/0/1">E.J. Jeon</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Jo_J/0/1/0/all/0/1">J.H. Jo</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Joo_H/0/1/0/all/0/1">H.W. Joo</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Kang_W/0/1/0/all/0/1">W.G. Kang</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Kang_W/0/1/0/all/0/1">W. Kang</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Kauer_M/0/1/0/all/0/1">M. Kauer</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Kim_G/0/1/0/all/0/1">G.S. Kim</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Kim_H/0/1/0/all/0/1">H. Kim</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Kim_H/0/1/0/all/0/1">H.J. Kim</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Kim_K/0/1/0/all/0/1">K.W. Kim</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Kim_N/0/1/0/all/0/1">N.Y. Kim</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Kim_S/0/1/0/all/0/1">S.K. Kim</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Kim_Y/0/1/0/all/0/1">Y.D. Kim</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Kim_Y/0/1/0/all/0/1">Y.H. Kim</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Ko_Y/0/1/0/all/0/1">Y.J. Ko</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Kudryavtsev_V/0/1/0/all/0/1">V.A. Kudryavtsev</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Lee_H/0/1/0/all/0/1">H.S. Lee</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Lee_J/0/1/0/all/0/1">J. Lee</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Lee_J/0/1/0/all/0/1">J.Y. Lee</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Lee_M/0/1/0/all/0/1">M.H. Lee</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Leonard_D/0/1/0/all/0/1">D.S. Leonard</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Lynch_W/0/1/0/all/0/1">W.A. Lynch</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Maruyama_R/0/1/0/all/0/1">R.H. Maruyama</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Mouton_F/0/1/0/all/0/1">F. Mouton</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Olsen_S/0/1/0/all/0/1">S.L. Olsen</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Park_B/0/1/0/all/0/1">B.J. Park</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Park_H/0/1/0/all/0/1">H.K. Park</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Park_H/0/1/0/all/0/1">H.S. Park</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Park_K/0/1/0/all/0/1">K.S. Park</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Pitta_R/0/1/0/all/0/1">R.L.C. Pitta</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Prihtiadi_H/0/1/0/all/0/1">H. Prihtiadi</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Ra_S/0/1/0/all/0/1">S. Ra</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Rott_C/0/1/0/all/0/1">C. Rott</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Shin_K/0/1/0/all/0/1">K.A. Shin</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Scar_A/0/1/0/all/0/1">A. Scar</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Spooner_N/0/1/0/all/0/1">N.J.C. Spooner</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Thompson_W/0/1/0/all/0/1">W.G. Thompson</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Yang_L/0/1/0/all/0/1">L. Yang</a>, <a href="http://arxiv.org/find/hep-ex/1/au:+Yu_G/0/1/0/all/0/1">G.H. Yu</a>

We present results from a search for solar axions with the COSINE-100
detector. We find no evidence of solar axion events from a data set of 6,303.9
kg$cdot$days exposure and set a 90,% confidence level upper limit on the
axion-electron coupling, $g_{ae}$, at 1.70~$times$~$10^{-11}$ for an axion
mass less than 1,keV/c$^2$. This limit excludes QCD axions heavier than
0.59,eV/c$^2$ in the DFSZ model and 168.1,eV/c$^2$ in the KSVZ model.

We present results from a search for solar axions with the COSINE-100
detector. We find no evidence of solar axion events from a data set of 6,303.9
kg$cdot$days exposure and set a 90,% confidence level upper limit on the
axion-electron coupling, $g_{ae}$, at 1.70~$times$~$10^{-11}$ for an axion
mass less than 1,keV/c$^2$. This limit excludes QCD axions heavier than
0.59,eV/c$^2$ in the DFSZ model and 168.1,eV/c$^2$ in the KSVZ model.

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