The impact of ultraviolet suppression on the rates and properties of strongly lensed Type IIn supernovae detected by LSST
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| Format: | Preprint |
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2025
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| author | Pérez, Andrés I. Ponte Smith, Graham P. Nicholl, Matt Arendse, Nikki Ryczanowski, Dan Dhawan, Suhail Collaboration, the LSST Strong Lensing Science |
| author_facet | Pérez, Andrés I. Ponte Smith, Graham P. Nicholl, Matt Arendse, Nikki Ryczanowski, Dan Dhawan, Suhail Collaboration, the LSST Strong Lensing Science |
| contents | Upcoming wide-field time-domain surveys, such as the Vera C. Rubin Observatory's Legacy Survey of Space and Time (LSST) are expected to discover up to two orders of magnitude more strongly lensed supernovae per year than have so far been observed. Of these, Type IIn supernovae have been predicted to be detected more frequently than any other supernova type, despite their small relative detection fraction amongst non-lensed supernovae. However, previous studies that predict a large population of lensed Type IIn supernova detections model their time evolving spectrum as a pure blackbody. In reality, there is a deficit in the UV flux of supernovae relative to the blackbody continuum due to line-blanketing from iron-group elements in the ejecta and scattering effects. In this work we quantify the effect of this UV suppression on the detection rates by LSST of a simulated population of strongly lensed Type IIn supernovae, relative to a pure blackbody model, using a mock LSST observing run. With a blackbody model, we predict to detect $\sim$70 lensed Type IIn supernova per year with LSST. By modelling a similar UV deficit to that seen in superluminous supernovae, we recover 60 - 80% of the detections obtained using a pure blackbody model, of which $\sim$10 detections per year are sufficiently bright ($m_\textrm{i} < 22.5$ mag) and detected early enough (> 5 observations before lightcurve peak) to enable high-cadence spectroscopic follow up. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2504_14433 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | The impact of ultraviolet suppression on the rates and properties of strongly lensed Type IIn supernovae detected by LSST Pérez, Andrés I. Ponte Smith, Graham P. Nicholl, Matt Arendse, Nikki Ryczanowski, Dan Dhawan, Suhail Collaboration, the LSST Strong Lensing Science High Energy Astrophysical Phenomena Cosmology and Nongalactic Astrophysics Upcoming wide-field time-domain surveys, such as the Vera C. Rubin Observatory's Legacy Survey of Space and Time (LSST) are expected to discover up to two orders of magnitude more strongly lensed supernovae per year than have so far been observed. Of these, Type IIn supernovae have been predicted to be detected more frequently than any other supernova type, despite their small relative detection fraction amongst non-lensed supernovae. However, previous studies that predict a large population of lensed Type IIn supernova detections model their time evolving spectrum as a pure blackbody. In reality, there is a deficit in the UV flux of supernovae relative to the blackbody continuum due to line-blanketing from iron-group elements in the ejecta and scattering effects. In this work we quantify the effect of this UV suppression on the detection rates by LSST of a simulated population of strongly lensed Type IIn supernovae, relative to a pure blackbody model, using a mock LSST observing run. With a blackbody model, we predict to detect $\sim$70 lensed Type IIn supernova per year with LSST. By modelling a similar UV deficit to that seen in superluminous supernovae, we recover 60 - 80% of the detections obtained using a pure blackbody model, of which $\sim$10 detections per year are sufficiently bright ($m_\textrm{i} < 22.5$ mag) and detected early enough (> 5 observations before lightcurve peak) to enable high-cadence spectroscopic follow up. |
| title | The impact of ultraviolet suppression on the rates and properties of strongly lensed Type IIn supernovae detected by LSST |
| topic | High Energy Astrophysical Phenomena Cosmology and Nongalactic Astrophysics |
| url | https://arxiv.org/abs/2504.14433 |