Candidate strongly lensed type Ia supernovae in the Zwicky Transient Facility archive
Creators: name: Townsend, A.
name: Nordin, J.
name: Carracedo, A. Sagués
name: Kowalski, M.
name: Arendse, N.
name: Dhawan, S.
name: Goobar, A.
name: Johansson, J.
name: Mörtsell, E.
name: Schulze, S.
name: Andreoni, I.
name: Fernández, E.
name: Kim, A. G.
name: Nugent, P. E.
name: Prada, F.
name: Rigault, M.
name: Sarin, N.
name: Sharma, D.
name: Bellm, E. C.
name: Coughlin, M. W.
name: Dekany, R.
name: Groom, S. L.
name: Lacroix, L.
name: Laher, R. R.
name: Riddle, R.
name: Aguilar, J.
name: Ahlen, S.
name: Bailey, S.
name: Brooks, D.
name: Claybaugh, T.
name: de la Macorra, A.
name: Dey, A.
name: Dey, B.
name: Doel, P.
name: Fanning, K.
name: Forero-Romero, J. E.
name: Gaztañaga, E.
name: Gontcho, S. Gontcho A
name: Honscheid, K.
name: Howlett, C.
name: Kisner, T.
name: Kremin, A.
name: Lambert, A.
name: Landriau, M.
name: Guillou, L. Le
name: Levi, M. E.
name: Manera, M.
name: Meisner, A.
name: Miquel, R.
name: Moustakas, J.
name: Mueller, E.
name: Myers, A. D.
name: Nie, J.
name: Palanque-Delabrouille, N.
name: Poppett, C.
name: Rezaie, M.
name: Rossi, G.
name: Sanchez, E.
name: Schlegel, D.
name: Schubnell, M.
name: Seo, H.
name: Sprayberry, D.
name: Tarlé, G.
name: Zou, H.
Publisher: name: arXiv
Year: 2024
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences
subject: FOS: Physical sciences

description: Gravitationally lensed type Ia supernovae (glSNe Ia) are unique astronomical tools that can be used to study cosmological parameters, distributions of dark matter, the astrophysics of the supernovae, and the intervening lensing galaxies themselves. A small number of highly magnified glSNe Ia have been discovered by ground-based telescopes such as the Zwicky Transient Facility (ZTF), but simulations predict that a fainter population may also exist. We present a systematic search for glSNe Ia in the ZTF archive of alerts distributed from June 1 2019 to September 1 2022. Using the AMPEL platform, we developed a pipeline that distinguishes candidate glSNe Ia from other variable sources. Initial cuts were applied to the ZTF alert photometry before forced photometry was obtained for the remaining candidates. Additional cuts were applied to refine the candidates based on their light curve colours, lens galaxy colours, and the resulting parameters from fits to the SALT2 SN Ia template. The candidates were also cross-matched with the DESI spectroscopic catalogue. Seven transients were identified that had an associated galaxy DESI redshift, which we present as glSN Ia candidates. Although superluminous supernovae (SLSNe) cannot be fully rejected as contaminants, two events, ZTF19abpjicm and ZTF22aahmovu, are significantly different from typical SLSNe and their light curves can be modelled as two-image glSN Ia systems. From this two-image modelling, we estimate time delays of 22 $\pm$ 3 and 34 $\pm$ 1 days for the two events, respectively, which suggests that we have uncovered a population of glSNe Ia with longer time delays. The pipeline is currently being applied to the live ZTF alert stream to identify and follow-up future candidates while active, and it could be the foundation for glSNe Ia searches in future surveys, such as the Rubin Observatory Legacy Survey of Space and Time.
description: 29 pages, 15 figures. Accepted in A&amp;A