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@INPROCEEDINGS{Ruz:426141,
      author       = {Ruz, J. and Vogel, J. K. and Armengaud, E. and Attie, D.
                      and Basso, S. and Brun, P. and Bykovskiy, N. and Carmona, J.
                      M. and Castel, J. F. and Cebrian, S. and Civitani, M. and
                      Cogollos, C. and Costa, D. and Dafni, T. and Derbin, A. V.
                      and Descalle, M. A. and Desch, K. and Dobrich, B. and
                      Dratchnev, I. and Dudarev, A. and Ferrer-Ribas, E. and
                      Galan, J. and Galanti, G. and Gascon, D. and Gastaldo, L.
                      and Garrido, L. and Germani, C. and Ghisellini, G. and
                      Giannotti, M. and Giomataris, I. and Gninenko, S. and
                      Golubev, N. and Graciani, R. and Irastorza, I. G. and
                      Jakovcic, K. and Kaminski, J. and Krcmar, M. and Krieger, C.
                      and Lakic, B. and Lasserre, T. and Laurent, P. and Lomskaya,
                      I. and Unzhakov, E. and Limousin, O. and Lindner, Axel and
                      Luzon, G. and Mescia, F. and Miralda-Escude, J. and
                      Mirallas, H. and Muratova, V. N. and Navick, X. F. and
                      Nones, C. and Notari, A. and Nozik, A. and Nunez, A. and
                      Solorzano, A. Ortiz de and Pantuev, V. and Papaevangelou, T.
                      and Pareschi, G. and Picatoste, E. and Pivovaroff, M. J. and
                      Perez, K. and Redondo, J. and Ringwald, A. and Ruiz-Choliz,
                      E. and Salvado, J. and Schiffer, T. and Schmidt, S. and
                      Schneekloth, U. and Schott, M. and Silva, H. and
                      Tagliaferri, G. and Tavecchio, F. and Kate, H. ten and
                      Tkackev, I. and Troitsky, S. and Vedrine, P. and Weltman,
                      A.},
      title        = {{N}ext {G}eneration {S}earch for {A}xion and {ALP} {D}ark
                      {M}atter with the {I}nternational {A}xion {O}bservatory},
      publisher    = {IEEE},
      reportid     = {PUBDB-2019-03614},
      pages        = {1-4},
      year         = {2018},
      comment      = {2018 IEEE Nuclear Science Symposium and Medical Imaging
                      Conference Proceedings (NSS/MIC) - IEEE, 2018. - ISBN
                      978-1-5386-8494-8 - doi:10.1109/NSSMIC.2018.8824640},
      booktitle     = {2018 IEEE Nuclear Science Symposium
                       and Medical Imaging Conference
                       Proceedings (NSS/MIC) - IEEE, 2018. -
                       ISBN 978-1-5386-8494-8 -
                       doi:10.1109/NSSMIC.2018.8824640},
      abstract     = {More than 80 years after the postulation of dark matter,
                      its nature remains one of the fundamental questions in
                      cosmology. Axions are currently one of the leading
                      candidates for the hypothetical, non-baryonic dark matter
                      that is expected to account for about $25\%$ of the energy
                      density of the Universe. Especially in the light of the
                      Large Hadron Collider at CERN slowly closing in on
                      Weakly-Interacting Massive Particle (WIMP) searches, axions
                      and axion-like particles (ALPs) provide a viable alternative
                      approach to solving the dark matter problem. The fact that
                      makes them particularly appealing is that they were
                      initially introduced to solve a long-standing problem in
                      quantum chromodynamics and the Standard Model of particle
                      physics.Helioscopes are a type of axion experiment searching
                      for axions produced in the core of the Sun via the Primakoff
                      effect. The International Axion Observatory (IAXO) is a next
                      generation axion helioscope aiming at a sensitivity to the
                      axion-photon coupling of 1 − 1.5 orders of magnitude
                      beyond the current most sensitive axion helioscope, which is
                      the CERN Axion Solar Telescope (CAST). IAXO will be able to
                      challenge the stringent bounds from supernova SN1987A and
                      test the axion interpretation of anomalous white-dwarf
                      cooling. Beyond standard axions, this new experiment will
                      also be able to search for a large variety of axion-like
                      particles and other novel excitations at the low-energy
                      frontier of elementary particle physics. BabyIAXO is
                      proposed as an intermediate-scale experiment increasing the
                      sensitivity to axion-photon couplings down to a few
                      10−11GeV−1and thus delivering significant physics
                      results while demonstrating the feasibility of the
                      full-scale IAXO experiment. Here we introduce the IAXO and
                      BabyIAXO experiments, report on the current status of both
                      and outline the expected IAXO science reach.},
      month         = {Nov},
      date          = {2018-11-10},
      organization  = {2018 IEEE Nuclear Science Symposium
                       and Medical Imaging Conference
                       (NSS/MIC), Sydney (Australia), 10 Nov
                       2018 - 17 Nov 2018},
      cin          = {ALPS / T},
      cid          = {I:(DE-H253)ALPS-20130318 / I:(DE-H253)T-20120731},
      pnm          = {611 - Fundamental Particles and Forces (POF3-611)},
      pid          = {G:(DE-HGF)POF3-611},
      experiment   = {EXP:(DE-MLZ)NOSPEC-20140101},
      typ          = {PUB:(DE-HGF)8 / PUB:(DE-HGF)7},
      doi          = {10.1109/NSSMIC.2018.8824640},
      url          = {https://bib-pubdb1.desy.de/record/426141},
}