Retrospective Search for Strongly Lensed Supernovae in the DESI Legacy Imaging Surveys
arXiv:2301.03578 · doi:10.3847/1538-4357/acd1e4
Abstract
The introduction of deep wide-field surveys in recent years and the adoption of machine learning techniques have led to the discoveries of strong gravitational lensing systems and candidates. However, the discovery of multiply lensed transients remains a rarity. Lensed transients and especially lensed supernovae are invaluable tools to cosmology as they allow us to constrain cosmological parameters via lens modeling and the measurements of their time delays. In this paper, we develop a pipeline to perform a targeted lensed transient search. We apply this pipeline to 5807 strong lenses and candidates, identified in the literature, in the DESI Legacy Imaging Surveys Data Release 9 (DR9) footprint. For each system, we analyze every exposure in all observed bands (DECam , , and ). Our pipeline finds, groups, and ranks detections that are in sufficient proximity temporally and spatially. After the first round of inspection, for promising candidate systems, we further examine the newly available DR10 data (with additional and bands). Here we present our targeted lensed supernova search pipeline and seven new lensed supernova candidates, including a very likely lensed supernova probably a Type Ia in a system with an Einstein radius of .
53 pages, 50 figures, 3 tables
References in corpus (27)
- Array Programming with NumPy
- Cosmic Star Formation History
- The Pantheon+ Analysis: The Full Dataset and Light-Curve Release
- Cosmic Distances Calibrated to 1% Precision with Gaia EDR3 Parallaxes and Hubble Space Telescope Photometry of 75 Milky Way Cepheids Confirm Tension with LambdaCDM
- Measurements of the Hubble Constant: Tensions in Perspective
- The Dark Energy Survey Data Release 2
- Multiple Images of a Highly Magnified Supernova Formed by an Early-Type Cluster Galaxy Lens
- Star Formation and the Growth of Stellar Mass
- A New Algorithm For Difference Image Analysis
- The Clustering of DESI-like Luminous Red Galaxies Using Photometric Redshifts
- SALT3: An Improved Type Ia Supernova Model for Measuring Cosmic Distances
- Absolute-Magnitude Distributions of Supernovae
- A Highly Magnified Star at Redshift 6.2
- The Sloan Lens ACS Survey. XIII. Discovery of 40 New Galaxy-Scale Strong Lenses
- Detection of the Gravitational Lens Magnifying a Type Ia Supernova
- Discovering New Strong Gravitational Lenses in the DESI Legacy Imaging Surveys
- HOLISMOKES -- II. Identifying galaxy-scale strong gravitational lenses in Pan-STARRS using convolutional neural networks
- On the accuracy of time-delay cosmography in the Frontier Fields Cluster MACS J1149.5+2223 with supernova Refsdal
- HOLISMOKES -- I. Highly Optimised Lensing Investigations of Supernovae, Microlensing Objects, and Kinematics of Ellipticals and Spirals
- Image Subtraction in Fourier Space
- HOLISMOKES. VI. New galaxy-scale strong lens candidates from the HSC-SSP imaging survey
- Mining for Strong Gravitational Lenses with Self-supervised Learning
- HOLISMOKES. VIII. High-redshift, strong-lens search in the Hyper Suprime-Cam Subaru Strategic Program
- The Hubble constant from strongly lensed supernovae with standardizable magnifications
- Shock cooling of a red-supergiant supernova at redshift 3 in lensed images
- LensWatch: I. Resolved HST Observations and Constraints on the Strongly-Lensed Type Ia Supernova 2022qmx ("SN Zwicky")
- VLT/Magellan spectroscopy of 29 strong lensing selected galaxy clusters
Cited by in corpus (6)
- Strong gravitational lensing and microlensing of supernovae
- New Strong Gravitational Lenses from the DESI Legacy Imaging Surveys Data Release 9
- Project Dinos II: Redshift evolution of dark and luminous matter density profiles in strong-lensing elliptical galaxies across 0.1 < z < 0.9
- A Targeted Search for Variable Gravitationally Lensed Quasars
- Differencing and Coadding JWST Images with Matched Point Spread Function
- Detection of Unresolved Strongly Lensed Supernovae with 7-Dimensional Telescope