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@ARTICLE{Abeln:449789,
      author       = {Abeln, A. and Altenmüller, K. and Arguedas Cuendis, S. and
                      Armengaud, E. and Attié, D. and Aune, S. and Basso, S. and
                      Bergé, L. and Biasuzzi, B. and Borges De Sousa, P. T. C.
                      and Brun, P. and Bykovskiy, N. and Calvet, D. and Carmona,
                      J. M. and Castel, J. F. and Cebrián, S. and Chernov, V. and
                      Christensen, F. E. and Civitani, M. M. and Cogollos, C. and
                      Dafní, T. and Derbin, A. and Desch, K. and Díez, D. and
                      Dinter, M. and Döbrich, B. and Drachnev, I. and Dudarev, A.
                      and Dumoulin, L. and Ferreira, D. D. M. and Ferrer-Ribas, E.
                      and Fleck, I. and Galán, J. and Gascón, D. and Gastaldo,
                      L. and Giannotti, M. and Giomataris, Y. and Giuliani, A. and
                      Gninenko, S. and Golm, J. and Golubev, N. and Hagge, L. and
                      Hahn, J. and Hailey, C. J. and Hengstler, D. and Henriksen,
                      P. L. and Houdy, T. and Iglesias-Marzoa, R. and
                      Iguaz-Gutierrez, F. J. and Irastorza, I. G. and Iñiguez, C.
                      and Jakovčić, K. and Kaminski, J. and Kanoute, B. and
                      Karstensen, S. and Kravchuk, L. and Lakić, B. and Lasserre,
                      T. and Laurent, P. and Limousin, O. and Lindner, Axel and
                      Loidl, M. and Lomskaya, I. and López-Alegre, G. and
                      Lubsandorzhiev, B. and Ludwig, Kai and Luzón, G. and
                      Malbrunot, C. and Margalejo, C. and Marin-Franch, A. and
                      Marnieros, S. and Marutzky, F. and Mauricio, J. and
                      Menesguen, Y. and Mentink, M. and Mertens, S. and Mescia, F.
                      and Miralda-Escudé, J. and Mirallas, H. and Mols, J. P. and
                      Muratova, V. and Navick, X. F. and Nones, C. and Notari, A.
                      and Nozik, A. and Obis, L. and Oriol, C. and Orsini, F. and
                      Ortiz de Solórzano, A. and Oster, S. and Pais Da Silva, H.
                      P. and Pantuev, V. and Papaevangelou, T. and Pareschi, G.
                      and Perez, K. and Pérez, O. and Picatoste, E. and
                      Pivovaroff, M. J. and Poda, D. V. and Redondo, J. and
                      Ringwald, A. and Rodrigues, M. and Rueda-Teruel, F. and
                      Rueda-Teruel, S. and Ruiz-Choliz, E. and Ruz, J. and
                      Saemann, E. O. and Salvado, J. and Schiffer, T. and Schmidt,
                      S. and Schneekloth, U. and Schott, M. and Segui, L. and
                      Tavecchio, F. and ten Kate, H. H. J. and Tkachev, I. and
                      Troitsky, S. and Unger, D. and Unzhakov, E. and Ushakov, N.
                      and Vogel, J. K. and Voronin, D. and Weltman, A. and
                      Werthenbach, U. and Wuensch, W. and Yanes-Díaz, A.},
      collaboration = {{IAXO Collaboration}},
      title        = {{C}onceptual {D}esign of {B}aby{IAXO}, the intermediate
                      stage towards the {I}nternational {A}xion {O}bservatory},
      reportid     = {PUBDB-2020-04016, arXiv:2010.12076. arXiv:2010.12076},
      year         = {2020},
      note         = {76 pages, 47 figures},
      abstract     = {This article describes BabyIAXO, an intermediate
                      experimental stage of the International Axion Observatory
                      (IAXO), proposed to be sited at DESY. IAXO is a large-scale
                      axion helioscope that will look for axions and axion-like
                      particles (ALPs), produced in the Sun, with unprecedented
                      sensitivity. BabyIAXO is conceived to test all IAXO
                      subsystems (magnet, optics and detectors) at a relevant
                      scale for the final system and thus serve as prototype for
                      IAXO, but at the same time as a fully-fledged helioscope
                      with relevant physics reach itself, and with potential for
                      discovery. The BabyIAXO magnet will feature two 10 m long,
                      70 cm diameter bores, and will host two detection lines
                      (optics and detector) of dimensions similar to the final
                      ones foreseen for IAXO. BabyIAXO will detect or reject solar
                      axions or ALPs with axion-photon couplings down to
                      $g_{a\gamma} \sim 1.5 \times 10^{-11}$ GeV$^{-1}$, and
                      masses up to $m_a\sim 0.25$ eV. BabyIAXO will offer
                      additional opportunities for axion research in view of IAXO,
                      like the development of precision x-ray detectors to
                      identify particular spectral features in the solar axion
                      spectrum, and the implementation of
                      radiofrequency-cavity-based axion dark matter setups.},
      cin          = {T / ALPS},
      cid          = {I:(DE-H253)T-20120731 / I:(DE-H253)ALPS-20130318},
      pnm          = {611 - Fundamental Particles and Forces (POF3-611)},
      pid          = {G:(DE-HGF)POF3-611},
      experiment   = {EXP:(DE-MLZ)NOSPEC-20140101},
      typ          = {PUB:(DE-HGF)25},
      eprint       = {2010.12076},
      howpublished = {arXiv:2010.12076},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:2010.12076;\%\%$},
      doi          = {10.3204/PUBDB-2020-04016},
      url          = {https://bib-pubdb1.desy.de/record/449789},
}