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Posters (Monday)

Undergraduate students funded by the LSSTC will have their posters displayed all day on Monday and Tuesday.

These undergraduates will be giving flash talks during the Monday and Tuesday plenary sessions.

The dedicated "poster session" times for students to stand at their posters are the 30 minutes after each plenary.

Posters

Denvir Higgin - Exploring the mass to light ratio of massive galaxies with the Rubin Observatory data preview
Rodiat Ayinde - From MetaAI insight to the detection of rare echoes of stellar explosions
Andrew Eden - The outer halo observed by the Vera Rubin Observatory: Mock catalogs of the outer halo using FIRE and ANANKE
Ved Shah - Finding EM counterparts for kilonovae with LSST using machine learning
Mathilda Nillson - Using Nearby Type Ia Supernovae to Measure Cosmological Distances
Joseph Santos - Characterizing the impact of photometric redshift uncertainties on dark energy constraints from LSST using analytic nuisance parameter marginalization
Aiden Cloud - Connecting Stellar Streams - a Precursor Study for LSST
David Gonzalez - Mapping the Outer Edge of the Milky Way’s Dark Matter Halo Using LSST
Heloisa Mengisztki - Optimizing software infrastructure to compute photo-zs in the LSST scale: preparing for DR1
Giovanni Gollotti - Strategies for Incremental Template Generation in the Early LSST Survey
Sam Scott - Transient Science with DP0.2: Photometric history of a star
Alice Crafford - Assessing RAIL’s Estimation of Photometric Redshifts
Alessandro Salvatore Tramuto - Photometric Analysis and Classification of Young stars (PACY)
Nathan Cristello - Investigating the star formation rates of AGNs in three LSST Deep-Drilling Fields relative to the star-forming main sequence
Kevin Hong - Impact of scalar spectral index on weak lensing cosmology
Peter Kiernan - Modeling correlations in the atmospheric point spread function
Keyi Ding - Accurate and Precise Photospheric Stellar Parameters from Rubin ugriz Photometry
Ella Roselli - Testing the Consistency of Age Indicators in Understudied Open Clusters
Zoryanna Alvarez - Impact of residual errors in the atmospheric point spread function on cosmic shear measurements

Lead or Chair for this Session:

Beth Willman, Ryan Oelkers

Suggested Audience:

All

Category:

Science

Applicable to:

Project

Community

Day:

Monday 08/07

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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