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@ARTICLE{Ahyoune:618944,
      author       = {Ahyoune, S. and Altenmüller, K. and Antolín, I. and
                      Basso, S. and Brun, P. and Candon, F. R. and Castel, J. F.
                      and Cebrián, S. and Chouhan, D. and Della Ceca, R. and
                      Cervera-Cortés, M. and Chernov, V. and Civitani, M. M. and
                      Cogollos, C. and Costa, E. and Cotroneo, V. and Dafní, T.
                      and Derbin, A. and Desch, K. and Díaz-Martín, M. C. and
                      Díaz-Morcillo, A. and Díez-Ibáñez, D. and Pardos, C.
                      Diez and Dinter, M. and Döbrich, B. and Drachnev, I. and
                      Dudarev, A. and Ezquerro, A. and Fabiani, S. and
                      Ferrer-Ribas, E. and Finelli, F. and Fleck, I. and Galán,
                      J. and Galanti, G. and Galaverni, M. and García, J. A. and
                      García-Barceló, J. M. and Gastaldo, L. and Giannotti, M.
                      and Giganon, A. and Goblin, C. and Goyal, N. and Gu, Y. and
                      Hagge, L. and Helary, L. and Hengstler, D. and Heuchel, D.
                      and Hoof, S. and Iglesias-Marzoa, R. and Iguaz, F. J. and
                      Iñiguez, C. and Irastorza, I. G. and Jakovčíc, K. and
                      Käfer, D. and Kaminski, J. and Karstensen, S. and Law, M.
                      and Lindner, A. and Loidl, M. and Loiseau, C. and
                      López-Alegre, G. and Lozano-Guerrero, A. and
                      Lubsandorzhiev, B. and Luzón, G. and Manthos, I. and
                      Margalejo, C. and Marín-Franch, A. and Marqués, J. and
                      Marutzky, F. and Menneglier, C. and Mentink, M. and Mertens,
                      S. and Miralda-Escudé, J. and Mirallas, H. and Muleri, F.
                      and Muratova, V. and Navarro-Madrid, J. R. and Navick, X. F.
                      and Nikolopoulos, K. and Notari, A. and Nozik, A. and Obis,
                      L. and Ortiz-de-Solórzano, A. and O'Shea, T. and von Oy, J.
                      and Pareschi, G. and Papaevangelou, T. and Perez, K. and
                      Pérez, O. and Picatoste, E. and Pivovaroff, M. J. and
                      Porrón, J. and Puyuelo, M. J. and Quintana, A. and Redondo,
                      J. and Reuther, D. and Ringwald, A. and Rodrigues, M. and
                      Rubini, A. and Rueda-Teruel, S. and Rueda-Teruel, F. and
                      Ruiz-Chóliz, E. and Ruz, J. and Schaffran, J. and Schiffer,
                      T. and Schmidt, S. and Schneekloth, U. and Schönfeld, L.
                      and Schott, M. and Segui, L. and Singh, U. R. and Soffitta,
                      P. and Spiga, D. and Stern, M. and Straniero, O. and
                      Tavecchio, F. and Unzhakov, E. and Ushakov, N. A. and
                      Vecchi, G. and Vogel, J. K. and Voronin, D. M. and Ward, R.
                      and Weltman, A. and Wiesinger, C. and Wolf, R. and
                      Yanes-Díaz, A. and Yu, Y.},
      collaboration = {{IAXO Collaboration}},
      title        = {{A}n accurate solar axions ray-tracing response of
                      {B}aby{IAXO}},
      reportid     = {PUBDB-2024-07255, arXiv:2411.13915},
      year         = {2024},
      note         = {36 pages, 18 figures, 4 tables, Submitted to JHEP},
      abstract     = {BabyIAXO is the intermediate stage of the International
                      Axion Observatory (IAXO) to be hosted at DESY. Its primary
                      goal is the detection of solar axions following the axion
                      helioscope technique. Axions are converted into photons in a
                      large magnet that is pointing to the sun. The resulting
                      X-rays are focused by appropriate X-ray optics and detected
                      by sensitive low-background detectors placed at the focal
                      spot. The aim of this article is to provide an accurate
                      quantitative description of the different components (such
                      as the magnet, optics, and X-ray detectors) involved in the
                      detection of axions. Our efforts have focused on developing
                      robust and integrated software tools to model these
                      helioscope components, enabling future assessments of
                      modifications or upgrades to any part of the IAXO axion
                      helioscope and evaluating the potential impact on the
                      experiment's sensitivity. In this manuscript, we demonstrate
                      the application of these tools by presenting a precise
                      signal calculation and response analysis of BabyIAXO's
                      sensitivity to the axion-photon coupling. Though focusing on
                      the Primakoff solar flux component, our virtual helioscope
                      model can be used to test different production mechanisms,
                      allowing for direct comparisons within a unified framework.},
      cin          = {Unive / ALPS},
      cid          = {I:(DE-H253)Unive-20240404 / I:(DE-H253)ALPS-20130318},
      pnm          = {611 - Fundamental Particles and Forces (POF4-611) / AxScale
                      - Axions and relatives across different mass scales (802836)
                      / IAXOplus - Towards the detection of the axion with the
                      International Axion Observatory (788781)},
      pid          = {G:(DE-HGF)POF4-611 / G:(EU-Grant)802836 /
                      G:(EU-Grant)788781},
      experiment   = {EXP:(DE-H253)BabyIAXO-20210101},
      typ          = {PUB:(DE-HGF)25},
      eprint       = {2411.13915},
      howpublished = {arXiv:2411.13915},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:2411.13915;\%\%$},
      doi          = {10.3204/PUBDB-2024-07255},
      url          = {https://bib-pubdb1.desy.de/record/618944},
}