Discovery of SN 2025wny: A Strongly Gravitationally Lensed Superluminous Supernova at <i>z</i> = 2.01

Abstract We present the discovery of SN 2025wny (ZTF25abnjznp/GOTO25gqt) and spectroscopic classification of this event as the first gravitationally lensed Type I superluminous supernova (SLSN-I). Deep ground-based follow-up observations resolve four images of the supernova with <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mo>∼</mml:mo> <mml:mn>1</mml:mn> <mml:mover accent="true"> <mml:mrow> <mml:mi>.</mml:mi> </mml:mrow> <mml:mrow> <mml:mi>″</mml:mi> </mml:mrow> </mml:mover> <mml:mn>7</mml:mn> </mml:math> angular separation from the main lens galaxy, each coincident with the lensed images of a background galaxy seen in archival imaging of the field. Spectroscopy of the brightest image shows narrow features matching absorption lines at a redshift of z = 2.010 and broad features matching those seen in superluminous SNe with far-UV coverage. We infer a magnification factor of μ ∼ 20–50 for the brightest image in the system, based on photometric and spectroscopic comparisons to other SLSNe-I. SN 2025wny demonstrates that gravitationally lensed SNe are in reach of ground-based facilities out to redshifts far higher than previously assumed, and provide a unique window into studying distant supernovae and the internal properties of dwarf galaxies, as well as for time-delay cosmography.

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Publication Details

Journal
The Astrophysical Journal Letters
Published
2025-12-05
DOI
https://doi.org/10.3847/2041-8213/ae1d61
Citations
1
Primary Topic
Gamma-ray bursts and supernovae
Type
article
Field-Weighted Citation Impact
1.15
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article

Discovery of SN 2025wny: A Strongly Gravitationally Lensed Superluminous Supernova at z = 2.01

Yu-Jing Qin, Reed Riddle, A. Mahabal, Edvard Mörtsell et al.
1 citations
The Astrophysical Journal Letters
Gamma-ray bursts and supernovae
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article

Discovery of SN 2025wny: A Strongly Gravitationally Lensed Superluminous Supernova at z = 2.01

Yu-Jing Qin, Reed Riddle, A. Mahabal, Edvard Mörtsell, Jacob Wise, Xander J. Hall, Claes Fransson, J. Nordin, A. Goobar, D. Gruen, Suhail Dhawan, Adam A. Miller, Alice Townsend, J. Sollerman, Richard Dekany, Cameron Lemon, Jacob Osman Hjortlund, M. J. Graham, R. Lunnan, R. Michael Rich, C. Fremling, Russ R. Laher, Lin Yan, D. A. Perley, J. S. Bloom, Igor Andreoni, Steve Schulze, G. Hélou, Eric C. Bellm, Avinash Singh, Steven L. Groom, J. Johansson, Anjasha Gangopadhyay, M. M. Kasliwal, K. Tsalapatas, Zoë McGrath
article en
1 citations

Abstract

Abstract We present the discovery of SN 2025wny (ZTF25abnjznp/GOTO25gqt) and spectroscopic classification of this event as the first gravitationally lensed Type I superluminous supernova (SLSN-I). Deep ground-based follow-up observations resolve four images of the supernova with <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mo>∼</mml:mo> <mml:mn>1</mml:mn> <mml:mover accent="true"> <mml:mrow> <mml:mi>.</mml:mi> </mml:mrow> <mml:mrow> <mml:mi>″</mml:mi> </mml:mrow> </mml:mover> <mml:mn>7</mml:mn> </mml:math> angular separation from the main lens galaxy, each coincident with the lensed images of a background galaxy seen in archival imaging of the field. Spectroscopy of the brightest image shows narrow features matching absorption lines at a redshift of z = 2.010 and broad features matching those seen in superluminous SNe with far-UV coverage. We infer a magnification factor of μ ∼ 20–50 for the brightest image in the system, based on photometric and spectroscopic comparisons to other SLSNe-I. SN 2025wny demonstrates that gravitationally lensed SNe are in reach of ground-based facilities out to redshifts far higher than previously assumed, and provide a unique window into studying distant supernovae and the internal properties of dwarf galaxies, as well as for time-delay cosmography.

The Astrophysical Journal LettersVol. 995(1)
Openalex Percentile: Top 14%
Gamma-ray bursts and supernovae
1.15
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