@article{https://doi.org/10.48550/arxiv.2204.05060,<br/><span class="tab"></span>
  doi = {10.48550/ARXIV.2204.05060},<br/><span class="tab"></span>
  url = {https://arxiv.org/abs/2204.05060},<br/><span class="tab"></span>
  author = {Sahakyan,<br/><span class="tab"></span> N. and Giommi,<br/><span class="tab"></span> P. and Padovani,<br/><span class="tab"></span> P. and Petropoulou,<br/><span class="tab"></span> M. and Bégué,<br/><span class="tab"></span> D. and Boccardi,<br/><span class="tab"></span> B. and Gasparyan,<br/><span class="tab"></span> S.},<br/><span class="tab"></span>
  keywords = {High Energy Astrophysical Phenomena (astro-ph.HE),<br/><span class="tab"></span> Astrophysics of Galaxies (astro-ph.GA),<br/><span class="tab"></span> FOS: Physical sciences,<br/><span class="tab"></span> FOS: Physical sciences},<br/><span class="tab"></span>
  title = {A multi-messenger study of the blazar PKS 0735+178: a new major neutrino source candidate},<br/><span class="tab"></span>
  publisher = {arXiv},<br/><span class="tab"></span>
  year = {2022},<br/><span class="tab"></span>
  copyright = {Creative Commons Attribution 4.0 International}
}