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Possible non-standard halo models:
“Messy” VDFs from simulation
G. Lawrence in prep (+ MJZ and GL already working on related project)
Gaia sausage (two gaussian distributions)
S1 stream (counter-rotating/retrograde stream)
Nyx (co-rotating/prograde stream)
Hemli stream (stream from merger event)
Koppelman 1 and 2 (also called group 1 and 2, pair of streams from recent accretion)
EFTs with strong dependence on velocity or that allow for strong limits from NaI
Milestones
- Compute model spectrums in SABRE (if in a pinch, just do the last two)
- SI
- SD
- V dep
- Low mass
- High mass
- Influence of velocity dist on exclusion plots for SI (O1)
- SHM
- SHM++
- Helmi
- Sausage
- Sequoia
- Shards
- Messy
- Influence of velocity dist on exclusion plots for SD (O4)
- SHM
- SHM++
- Helmi
- Sausage
- Sequoia
- Shards
- Messy
- Comparison of modulation fraction for different targets
- Modulation amplitude vs peak day/phase
Meetings
Resources
Halo substructures of interest (Ciaran’s work): https://arxiv.org/pdf/1909.04684.pdf
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