SITCOMTN-161: PSF assessment in the field of Abell 360 and shapeHSM shear profile using LSSTComCam data
Abstract
The Rubin LSSTComCam on-sky campaign performed at the end of 2024 provided observations of the Abell 360 galaxy cluster; these data allow a preliminary study of cluster weak lensing analysis using Rubin Data Preview 1 (DP1) data. Among all the steps required for such analyses, accurate modeling of the PSF is essential. This work uses several diagnostics, mostly based on the residuals between the second moments of stars and the PSF model, to characterize the accuracy of the PSF modeling in the A360 field. We find the level of the residuals to be sufficiently low not to hinder the measurement of the tangential shear profile around A360. With a simple source selection process, we demonstrate that outputs of the LSST Science Pipelines can be used to detect the tangential shear profile in Abell 360 at the 3.6σ level, and our analysis indicates that contamination from PSF modeling systematics is negligible.
- Authors:
-
- Université Grenoble Alpes, CNRS/IN2P3, LPSC
- SLAC National Accelerator Laboratory; Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory
- Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory
- Department of Physics and Astronomy, Stony Brook University
- Department of Physics, Brown University
- Department of Physics, University of Wisconsin-Madison
- Center for Cosmology and Astro-Particle Physics, The Ohio State University
- Department of Astrophysical Sciences, Princeton University
- Université Savoie Mont-Blanc, CNRS/IN2P3, LAPP
- McWilliams Center for Cosmology & Astrophysics, Department of Physics, Carnegie Mellon University
- Department of Physics, Harvard University
- NSF NOIRLab
- Publication Date:
- Other Number(s):
- Vera C. Rubin Observatory Commissioning Technical Note SITCOMTN-161
- DOE Contract Number:
- AC02-76SF00515
- Research Org.:
- NSF-DOE Vera C. Rubin Observatory
- Sponsoring Org.:
- U.S. National Science Foundation; U.S. Department of Energy Office of Science
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS
- OSTI Identifier:
- 2572986
- DOI:
- https://doi.org/10.71929/rubin/2572986
Citation Formats
Combet, Céline, Plazas Malagón, Andrés A., Fu, Shenming, Adari, Prakruth, Dell'Antonio, Ian, Englert, Anthony, Gorsuch, Miranda R., Laliotis, Katherine, Léget, Pierre-François, Lorenzo Martinez, Narei, Mandelbaum, Rachel, Pedersen, Eske M., von der Linden, Anja, and Zhang, Yuanyuan. SITCOMTN-161: PSF assessment in the field of Abell 360 and shapeHSM shear profile using LSSTComCam data. United States: N. p., 2025.
Web. doi:10.71929/rubin/2572986.
Combet, Céline, Plazas Malagón, Andrés A., Fu, Shenming, Adari, Prakruth, Dell'Antonio, Ian, Englert, Anthony, Gorsuch, Miranda R., Laliotis, Katherine, Léget, Pierre-François, Lorenzo Martinez, Narei, Mandelbaum, Rachel, Pedersen, Eske M., von der Linden, Anja, & Zhang, Yuanyuan. SITCOMTN-161: PSF assessment in the field of Abell 360 and shapeHSM shear profile using LSSTComCam data. United States. doi:https://doi.org/10.71929/rubin/2572986
Combet, Céline, Plazas Malagón, Andrés A., Fu, Shenming, Adari, Prakruth, Dell'Antonio, Ian, Englert, Anthony, Gorsuch, Miranda R., Laliotis, Katherine, Léget, Pierre-François, Lorenzo Martinez, Narei, Mandelbaum, Rachel, Pedersen, Eske M., von der Linden, Anja, and Zhang, Yuanyuan. 2025.
"SITCOMTN-161: PSF assessment in the field of Abell 360 and shapeHSM shear profile using LSSTComCam data". United States. doi:https://doi.org/10.71929/rubin/2572986. https://www.osti.gov/servlets/purl/2572986. Pub date:Fri Jun 20 04:00:00 UTC 2025
@article{osti_2572986,
title = {SITCOMTN-161: PSF assessment in the field of Abell 360 and shapeHSM shear profile using LSSTComCam data},
author = {Combet, Céline and Plazas Malagón, Andrés A. and Fu, Shenming and Adari, Prakruth and Dell'Antonio, Ian and Englert, Anthony and Gorsuch, Miranda R. and Laliotis, Katherine and Léget, Pierre-François and Lorenzo Martinez, Narei and Mandelbaum, Rachel and Pedersen, Eske M. and von der Linden, Anja and Zhang, Yuanyuan},
abstractNote = {The Rubin LSSTComCam on-sky campaign performed at the end of 2024 provided observations of the Abell 360 galaxy cluster; these data allow a preliminary study of cluster weak lensing analysis using Rubin Data Preview 1 (DP1) data. Among all the steps required for such analyses, accurate modeling of the PSF is essential. This work uses several diagnostics, mostly based on the residuals between the second moments of stars and the PSF model, to characterize the accuracy of the PSF modeling in the A360 field. We find the level of the residuals to be sufficiently low not to hinder the measurement of the tangential shear profile around A360. With a simple source selection process, we demonstrate that outputs of the LSST Science Pipelines can be used to detect the tangential shear profile in Abell 360 at the 3.6σ level, and our analysis indicates that contamination from PSF modeling systematics is negligible.},
doi = {10.71929/rubin/2572986},
journal = {},
number = ,
volume = ,
place = {United States},
year = {Fri Jun 20 04:00:00 UTC 2025},
month = {Fri Jun 20 04:00:00 UTC 2025}
}
