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Project & Community Workshop 2023
7-11, August 2023 | Marriott University Park Tucson | Tucson, AZ
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Rubin Science Medley (Contributed Talks)
All are welcome to join this session, which will include an assortment of contributed talks on Rubin-related research.
Agenda
Welcome (5 min)
Simonyi/NSF Scholars Lightning Talks (each 7 min +3 min for questions; abstracts below)
Colin Burke -- Intermediate-mass black hole demographics with the Rubin Observatory
Gautham Narayan -- Building the Time-Domain Ecosystem with Rubin
Darryl Zachary Seligman -- Prospects for Interstellar Interlopers and Dark Comets with the Rubin Observatory
Contributed Talks (each 7 min +3 min for questions; abstracts linked)
Adam McMaster -- Black Hole Hunters: A Future Microlensing Search for Quiescent Black Holes With LSST?
Oleksandra Razim -- Synthetic LSST magnitudes derived from Gaia XP spectra
Roohi Dalal -- New Cosmology Constraints from Hyper Suprime-Cam Year 3 Data and Lessons Learned for Rubin
Abstracts
Colin Burke -- Intermediate-mass black hole demographics with the Rubin Observatory
Optical variability is a powerful probe of the population of accreting black holes. Thanks to its superb cadence and depth, Rubin light curves will open a new window onto the population of accreting intermediate-mass black holes (IMBHs). In this talk, I will describe plans to develop and apply Bayesian modeling techniques to constrain the number density of IMBHs with early Rubin data. With Rubin light curves, IMBHs will also be laboratories for studying the physics of black hole accretion on human timescales.
Darryl Zachary Seligman -- Prospects for Interstellar Interlopers and Dark Comets with the Rubin Observatory
In recent years, two entirely new classes of planetesimals have been discovered in the solar system: interstellar interlopers and dark comets. These still-enigmatic objects are challenging our understanding of the behavior and properties of comets and asteroids. In this talk, I will review what has been learned to date from the known interstellar objects and dark comets, highlighting the attributes that are difficult to reconcile with previous models of planetesimal behavior. The forthcoming Rubin Observatory Legacy Survey of Space and Time (LSST) is poised to further transform our understanding of these classes of objects, and I will discuss the feasibility of future discoveries via ground-based observations as well as possible intercept missions.
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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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Slides
mgraham
Thu, 08/03/2023 - 18:41
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Graham (Intro)
colinburke
Sat, 08/05/2023 - 13:46
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Burke IMBH (PCW 2023)
gnarayan
Sun, 08/06/2023 - 16:45
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Building the Time Domain Ecosystem with Rubin
adammcmaster
Mon, 08/07/2023 - 09:37
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Black Hole hunters
roohidalal
Mon, 08/07/2023 - 09:59
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New Cosmology Constraints from Hyper Suprime-Cam Year 3 Data
ShrRa
Tue, 08/08/2023 - 07:30
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Synthetic LSST magnitudes derived from Gaia XP spectra
darrylseligman
Tue, 08/08/2023 - 09:29
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Seligman Prospects for Interstellar Interlopers and Dark Comets
bbolin
Tue, 08/08/2023 - 14:58
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Palomar twilight discovery of Aylos and comets