Paper
Lensing in the Blue III: Weak Lensing Shape Catalogs of 30 Merging Galaxy Clusters
Authors
Sayan Saha, Jacqueline E. McCleary, Spencer W. Everett, Maya Amit, Georgios N. Vassilakis, Emaad Paracha, Leo W. H. Fung, Steven J. Benton, William C. Jones, Gavin Leroy, Eric M. Huff, Richard Massey, Thuy Vy T. Luu, Ajay S. Gill, Mohamed M. Shaaban, Philippe Voyer, Anthony M. Brown, Giulia Cerini, Paul Clark, Matthew Craigie, Christopher J. Damaren, Tim Eifler, David Harvey, Eric Habjan, John W. Hartley, Bradley Holder, Mathilde Jauzac, David Lagattuta, Jason S. -Y. Leung, Lun Li, Johanna M. Nagy, C. Barth Netterfield, Susan F. Redmond, Jason D. Rhodes, Andrew Robertson, L. Javier Romualdez, Jurgen Schmoll, Ellen Sirks, Sut Ieng Tam, André Z. Vitorelli, Alfredo Zenteno
Abstract
We present the weak gravitational lensing dataset from the Super-pressure Balloon-Borne Imaging Telescope (SuperBIT), which imaged 30 galaxy clusters during its 45 night flight in April to May 2023. SuperBIT is a first-of-its-kind balloon-borne imaging telescope that achieved near diffraction-limited observations in near-space conditions above 98% of the Earth's atmosphere. We use the metacalibration algorithm to obtain calibrated galaxy shapes for our target clusters and several calibration fields, enabling unbiased reconstruction of the weak-lensing signal. We employ several diagnostics throughout the pipeline, including assessments of point-spread function (PSF) modeling residuals and their impact on weak-lensing measurements, as well as tests for correlations between galaxy shapes and measured galaxy and PSF properties. To assess the multiplicative shear bias of the pipeline, we analyze a parallel set of simulated images that incorporate the real observing conditions from the flight, including measured SuperBIT PSFs, observed sky backgrounds, and detector noise, yielding a bias of $(1.1 \pm 7.8)$~per~cent.
Metadata
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Raw Data (Debug)
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"raw_xml": "<entry>\n <id>http://arxiv.org/abs/2603.18376v1</id>\n <title>Lensing in the Blue III: Weak Lensing Shape Catalogs of 30 Merging Galaxy Clusters</title>\n <updated>2026-03-19T00:28:59Z</updated>\n <link href='https://arxiv.org/abs/2603.18376v1' rel='alternate' type='text/html'/>\n <link href='https://arxiv.org/pdf/2603.18376v1' rel='related' title='pdf' type='application/pdf'/>\n <summary>We present the weak gravitational lensing dataset from the Super-pressure Balloon-Borne Imaging Telescope (SuperBIT), which imaged 30 galaxy clusters during its 45 night flight in April to May 2023. SuperBIT is a first-of-its-kind balloon-borne imaging telescope that achieved near diffraction-limited observations in near-space conditions above 98% of the Earth's atmosphere. We use the metacalibration algorithm to obtain calibrated galaxy shapes for our target clusters and several calibration fields, enabling unbiased reconstruction of the weak-lensing signal. We employ several diagnostics throughout the pipeline, including assessments of point-spread function (PSF) modeling residuals and their impact on weak-lensing measurements, as well as tests for correlations between galaxy shapes and measured galaxy and PSF properties. To assess the multiplicative shear bias of the pipeline, we analyze a parallel set of simulated images that incorporate the real observing conditions from the flight, including measured SuperBIT PSFs, observed sky backgrounds, and detector noise, yielding a bias of $(1.1 \\pm 7.8)$~per~cent.</summary>\n <category scheme='http://arxiv.org/schemas/atom' term='astro-ph.CO'/>\n <category scheme='http://arxiv.org/schemas/atom' term='astro-ph.IM'/>\n <published>2026-03-19T00:28:59Z</published>\n <arxiv:comment>29 pages, 22 figures, 2 table</arxiv:comment>\n <arxiv:primary_category term='astro-ph.CO'/>\n <author>\n <name>Sayan Saha</name>\n </author>\n <author>\n <name>Jacqueline E. McCleary</name>\n </author>\n <author>\n <name>Spencer W. Everett</name>\n </author>\n <author>\n <name>Maya Amit</name>\n </author>\n <author>\n <name>Georgios N. Vassilakis</name>\n </author>\n <author>\n <name>Emaad Paracha</name>\n </author>\n <author>\n <name>Leo W. H. Fung</name>\n </author>\n <author>\n <name>Steven J. Benton</name>\n </author>\n <author>\n <name>William C. Jones</name>\n </author>\n <author>\n <name>Gavin Leroy</name>\n </author>\n <author>\n <name>Eric M. Huff</name>\n </author>\n <author>\n <name>Richard Massey</name>\n </author>\n <author>\n <name>Thuy Vy T. Luu</name>\n </author>\n <author>\n <name>Ajay S. Gill</name>\n </author>\n <author>\n <name>Mohamed M. Shaaban</name>\n </author>\n <author>\n <name>Philippe Voyer</name>\n </author>\n <author>\n <name>Anthony M. Brown</name>\n </author>\n <author>\n <name>Giulia Cerini</name>\n </author>\n <author>\n <name>Paul Clark</name>\n </author>\n <author>\n <name>Matthew Craigie</name>\n </author>\n <author>\n <name>Christopher J. Damaren</name>\n </author>\n <author>\n <name>Tim Eifler</name>\n </author>\n <author>\n <name>David Harvey</name>\n </author>\n <author>\n <name>Eric Habjan</name>\n </author>\n <author>\n <name>John W. Hartley</name>\n </author>\n <author>\n <name>Bradley Holder</name>\n </author>\n <author>\n <name>Mathilde Jauzac</name>\n </author>\n <author>\n <name>David Lagattuta</name>\n </author>\n <author>\n <name>Jason S. -Y. Leung</name>\n </author>\n <author>\n <name>Lun Li</name>\n </author>\n <author>\n <name>Johanna M. Nagy</name>\n </author>\n <author>\n <name>C. Barth Netterfield</name>\n </author>\n <author>\n <name>Susan F. Redmond</name>\n </author>\n <author>\n <name>Jason D. Rhodes</name>\n </author>\n <author>\n <name>Andrew Robertson</name>\n </author>\n <author>\n <name>L. Javier Romualdez</name>\n </author>\n <author>\n <name>Jurgen Schmoll</name>\n </author>\n <author>\n <name>Ellen Sirks</name>\n </author>\n <author>\n <name>Sut Ieng Tam</name>\n </author>\n <author>\n <name>André Z. Vitorelli</name>\n </author>\n <author>\n <name>Alfredo Zenteno</name>\n </author>\n </entry>"
}