Lensing in the Blue IV: The First Weak Gravitational Lensing Maps from the Stratosphere
astro-ph.CO
Submitted: 2026-10-05
Updated: 2026-10-05
Comments: Submitted to ApJL
Code: https://github.com/GeorgeVassilakis/SMPy
License: http://creativecommons.org/licenses/by/4.0/
The gist: The Super-Pressure Balloon-borne Imaging Telescope (SuperBIT) completed its science flight in April 2023, obtaining imaging data for 30 galaxy clusters.
Terminology
Abstract
The Super-Pressure Balloon-borne Imaging Telescope (SuperBIT) completed its science flight in April 2023, obtaining imaging data for 30 galaxy clusters. In this work, we present the first weak-lensing convergence maps from these observations, using six clusters selected from the 30 targets. We construct background-galaxy catalogs using SuperBIT's three-band photometry and a color-color-based method to separate foreground and background galaxies, and use the calibrated galaxy shapes presented in Lensing in the Blue III to reconstruct the weak-lensing convergence field using Kaiser-Squires inversion. We compare the convergence signal-to-noise maps for the six clusters with independent tracers, including X-ray emission and red-sequence cluster-member number-density maps. These results demonstrate the first successful weak-lensing mass mapping with imaging from a sub-orbital astronomical observatory.
Sources
- Lensing-Reconstructed Dark Matter-Intracluster Medium Coherence as a Probe of Cluster Dynamical State: Application to HSTFF, RELICS, and CLASH Clusters
- Metacalibration: Direct Self-Calibration of Biases in Shear Measurement
- Large-Scale Cosmic Shear Measurements
- Lensing in the Blue III: Weak Lensing Shape Catalogs of 30 Merging Galaxy Clusters
- Cluster Weak Gravitational Lensing
- Detection of correlated galaxy ellipticities on CFHT data: first evidence for gravitational lensing by large-scale structures
- From SuperBIT to GigaBIT: Informing next-generation balloon-borne telescope design with Fine Guidance System flight data
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