Spectroscopic Classification of Extragalactic Transients from CRTS
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arXiv
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2025
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| author | Drake, A. J. Djorgovski, S. G. Graham, M. J. Stern, D. Mahabal, A. A. Catelan, M. Prieto, J. L. Larson, S. |
| author_facet | Drake, A. J. Djorgovski, S. G. Graham, M. J. Stern, D. Mahabal, A. A. Catelan, M. Prieto, J. L. Larson, S. |
| contents | The Catalina Real-time Transient Survey (CRTS) carried out a public survey for optical transients between 2007 and 2019, discovering more than 16,000 transient candidates. Here we present the spectra and highlight the results of the spectroscopic follow-up of CRTS extragalactic transients. As expected, we find that the bulk of these transients are normal supernovae. However, as we prioritised transients exhibiting unusual features or environments during our spectroscopic follow-up, we focus on the rarer types of transients. These objects include more than a dozen type-I superluminous supernovae and dozens of type-I and II supernovae that underwent circumstellar medium interactions. We highlight several specific supernovae, including a new analysis of SN 2008iy, a type-IIn which exhibited a bright pre-supernova outburst event similar to SN 2009ip and lasted more than 1800 days; CSS111225:140122+161705, a type-I supernova that showed an extreme 2.5 magnitude rebrightening event more than 200 days after its initial outburst; and SN 2009ny, a type-Ibn supernova that exhibited strong helium emission lines similar to SN 2002ao. We confirm our previous finding that numerous CRTS transients are associated with galaxies of extremely low luminosity. We discuss the difficulty in determining the origin of transients associated with outbursts in active galactic nuclei (AGN), tidal disruption events, and type-IIn supernovae. As an example, we present CSS150120:110008+385352, a CRTS transient similar to CSS100217:102913+404220 that occurred within a quiescent AGN and peaked at Mv = -23.6. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2510_20989 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Spectroscopic Classification of Extragalactic Transients from CRTS Drake, A. J. Djorgovski, S. G. Graham, M. J. Stern, D. Mahabal, A. A. Catelan, M. Prieto, J. L. Larson, S. High Energy Astrophysical Phenomena Astrophysics of Galaxies The Catalina Real-time Transient Survey (CRTS) carried out a public survey for optical transients between 2007 and 2019, discovering more than 16,000 transient candidates. Here we present the spectra and highlight the results of the spectroscopic follow-up of CRTS extragalactic transients. As expected, we find that the bulk of these transients are normal supernovae. However, as we prioritised transients exhibiting unusual features or environments during our spectroscopic follow-up, we focus on the rarer types of transients. These objects include more than a dozen type-I superluminous supernovae and dozens of type-I and II supernovae that underwent circumstellar medium interactions. We highlight several specific supernovae, including a new analysis of SN 2008iy, a type-IIn which exhibited a bright pre-supernova outburst event similar to SN 2009ip and lasted more than 1800 days; CSS111225:140122+161705, a type-I supernova that showed an extreme 2.5 magnitude rebrightening event more than 200 days after its initial outburst; and SN 2009ny, a type-Ibn supernova that exhibited strong helium emission lines similar to SN 2002ao. We confirm our previous finding that numerous CRTS transients are associated with galaxies of extremely low luminosity. We discuss the difficulty in determining the origin of transients associated with outbursts in active galactic nuclei (AGN), tidal disruption events, and type-IIn supernovae. As an example, we present CSS150120:110008+385352, a CRTS transient similar to CSS100217:102913+404220 that occurred within a quiescent AGN and peaked at Mv = -23.6. |
| title | Spectroscopic Classification of Extragalactic Transients from CRTS |
| topic | High Energy Astrophysical Phenomena Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2510.20989 |