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Project & Community Workshop 2023
7-11, August 2023 | Marriott University Park Tucson | Tucson, AZ
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The outer halo observed by the Vera Rubin Observatory: Mock catalogs of the outer halo using FIRE and ANANKE
Andrew Eden
Mock catalogs are a powerful tool to predict observables of future surveys and to compare data sets with simulations. We present mock catalogs of the Vera Rubin Observatory using the simulated Milky Way (MW) stellar halos from the Feedback In Realistic Environments (FIRE) simulations along with the ANANKE library. These catalogs provide generated observational data for the Vera Rubin Observatory telescope from seven selected Milky Way-like galaxies. We chose the galaxies and their respective snapshots to feature satellite galaxies such as the Large Magellanic Cloud (LMC) in the galactic halo at their pericentric passage around their host. We generated all-sky density maps for stellar and dark matter overdensities in the halos from the FIRE data and the ANANKE catalog. By comparing the overdensities between the original simulated data and the generated mock catalogs, we can establish how the Vera Rubin Observatory will be able to characterize the perturbations induced by the LMC on the MW’s halo.
This poster will be displayed on Monday and Tuesday.
The National Science Foundation (NSF) and the US Department of Energy (DOE) will support Rubin Observatory in its operations phase to carry out the Legacy Survey of Space and Time. They will also provide support for scientific research with the data. During operations, NSF funding is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with NSF, and DOE funding is managed by SLAC National Accelerator Laboratory (SLAC), under contract by DOE. Rubin Observatory is operated by NSF's National Optical-Infrared Astronomy Research Laboratory (NOIRLab) and SLAC.
NSF is an independent federal agency created by Congress in 1950 to promote the progress of science. NSF supports basic research and people to create knowledge that transforms the future.
We are privileged to conduct research on Cerro Pachón in Chile, and acknowledge the Indigenous communities in Chile as the natural protectors of these lands.
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