A closer look at dwarf galaxies exhibiting MIR variability: AGN confirmation and comparison with non-variable dwarf galaxies. Aravindan, A., Canalizo, G., Secrest, N., Satyapal, S., & Bohn, T. arXiv e-prints, August, 2024.
doi  bibtex   
@ARTICLE{2024arXiv240800666A,
       author = {{Aravindan}, Archana and {Canalizo}, Gabriela and {Secrest}, Nathan and {Satyapal}, Shobita and {Bohn}, Thomas},
        title = "{A closer look at dwarf galaxies exhibiting MIR variability: AGN confirmation and comparison with non-variable dwarf galaxies}",
      journal = {arXiv e-prints},
     keywords = {Astrophysics - Astrophysics of Galaxies},
         year = 2024,
        month = aug,
          eid = {arXiv:2408.00666},
        pages = {arXiv:2408.00666},
          doi = {10.48550/arXiv.2408.00666},
archivePrefix = {arXiv},
       eprint = {2408.00666},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2024arXiv240800666A},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

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