gSeaGen: the KM3NeT GENIE-based code for neutrino telescopes. (arXiv:2003.14040v1 [astro-ph.IM])
<a href="http://arxiv.org/find/astro-ph/1/au:+Aiello_S/0/1/0/all/0/1">Sebastiano Aiello</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Albert_A/0/1/0/all/0/1">Arnauld Albert</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Garre_S/0/1/0/all/0/1">Sergio Alves Garre</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Aly_Z/0/1/0/all/0/1">Zineb Aly</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ameli_F/0/1/0/all/0/1">Fabrizio Ameli</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Andre_M/0/1/0/all/0/1">Michel Andre</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Androulakis_G/0/1/0/all/0/1">Giorgos Androulakis</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Anghinolfi_M/0/1/0/all/0/1">Marco Anghinolfi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Anguita_M/0/1/0/all/0/1">Mancia Anguita</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Anton_G/0/1/0/all/0/1">Gisela Anton</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Ardid_M/0/1/0/all/0/1">Miquel Ardid</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Aublin_J/0/1/0/all/0/1">Julien Aublin</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bagatelas_C/0/1/0/all/0/1">Christos Bagatelas</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Barbarino_G/0/1/0/all/0/1">Giancarlo Barbarino</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Baret_B/0/1/0/all/0/1">Bruny Baret</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Pree_S/0/1/0/all/0/1">Suzan Basegmez du Pree</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bendahman_M/0/1/0/all/0/1">Meriem Bendahman</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Berbee_E/0/1/0/all/0/1">Edward Berbee</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bertin_V/0/1/0/all/0/1">Vincent Bertin</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Biagi_S/0/1/0/all/0/1">Simone Biagi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Biagioni_A/0/1/0/all/0/1">Andrea Biagioni</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bissinger_M/0/1/0/all/0/1">Matthias Bissinger</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Boettcher_M/0/1/0/all/0/1">Markus Boettcher</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Boumaaza_J/0/1/0/all/0/1">Jihad Boumaaza</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bourret_S/0/1/0/all/0/1">Simon Bourret</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bouta_M/0/1/0/all/0/1">Mohammed Bouta</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bouwhuis_M/0/1/0/all/0/1">Mieke Bouwhuis</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bozza_C/0/1/0/all/0/1">Cristiano Bozza</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Branzas_H/0/1/0/all/0/1">Horea Branzas</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bruchner_M/0/1/0/all/0/1">Marc Bruchner</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bruijn_R/0/1/0/all/0/1">Ronald Bruijn</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Brunner_J/0/1/0/all/0/1">J&#xfc;rgen Brunner</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Buis_E/0/1/0/all/0/1">Ernst-Jan Buis</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Buompane_R/0/1/0/all/0/1">Raffaele Buompane</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Busto_J/0/1/0/all/0/1">Jose Busto</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Calvo_D/0/1/0/all/0/1">David Calvo</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Capone_A/0/1/0/all/0/1">Antonio Capone</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Carretero_V/0/1/0/all/0/1">V&#xed;ctor Carretero</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Castaldi_P/0/1/0/all/0/1">Paolo Castaldi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Celli_S/0/1/0/all/0/1">Silvia Celli</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Chabab_M/0/1/0/all/0/1">Mohamed Chabab</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Chau_N/0/1/0/all/0/1">Nhan Chau</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Chen_A/0/1/0/all/0/1">Andrew Chen</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Cherubini_S/0/1/0/all/0/1">Silvio Cherubini</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Chiarella_V/0/1/0/all/0/1">Vitaliano Chiarella</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Chiarusi_T/0/1/0/all/0/1">Tommaso Chiarusi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Circella_M/0/1/0/all/0/1">Marco Circella</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Cocimano_R/0/1/0/all/0/1">Rosanna Cocimano</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Coelho_J/0/1/0/all/0/1">Joao Coelho</a>, et al. (187 additional authors not shown)

The gSeaGen code is a GENIE-based application developed to efficiently
generate high statistics samples of events, induced by neutrino interactions,
detectable in a neutrino telescope. The gSeaGen code is able to generate events
induced by all neutrino flavours, considering topological differences between
track-type and shower-like events. Neutrino interactions are simulated taking
into account the density and the composition of the media surrounding the
detector. The main features of gSeaGen are presented together with some
examples of its application within the KM3NeT project.

The gSeaGen code is a GENIE-based application developed to efficiently
generate high statistics samples of events, induced by neutrino interactions,
detectable in a neutrino telescope. The gSeaGen code is able to generate events
induced by all neutrino flavours, considering topological differences between
track-type and shower-like events. Neutrino interactions are simulated taking
into account the density and the composition of the media surrounding the
detector. The main features of gSeaGen are presented together with some
examples of its application within the KM3NeT project.

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