Probe | Constraint | LSST Impact | Complementary Instruments | Complications | References |
---|---|---|---|---|---|
Gaps in Streams | Power at small scale | Increasing number of streams; large distances less suceptible to disk baryons | Gaia; spec. follow-up; w-first | subhalo disruption by disk; gaps from baryons | |
Potential from Streams | Halo shape | Increasing number of streams | spectroscopy; Gaia; wfirst | perturbation from large accretion events (MW history); non-equilibrium dynamics | |
Colliding Clusters | self-interaction cross section | Finding colliding clusters; weak-lensing mass mapping; galaxy centroids; gas distribution and mass | chandra/xmm/erosita; w-first; SPT/ACT | ||
Cluster weak lensing mass | decay/annihilation | finding clusters; weak lensing mass profiles | x-rays | agn feedback; mergers (non-equilibrium); Baryon emission lines | |
Cluster galaxy and weak lensing mass profiles | halo shape | finding clusters; deep |
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#!/usr/bin/env python | |
# | |
# LSST Data Management System | |
# Copyright 2015 AURA/LSST | |
# | |
# This product includes software developed by the | |
# LSST Project (http://www.lsst.org/). | |
# | |
# This program is free software: you can redistribute it and/or modify | |
# it under the terms of the GNU General Public License as published by |
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