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Searching for Satellites Around Galactic AnalogsThe SAGA Project
Risa Wechsler, Ben Weiner, Erik Tollerud, Yao-Yuan Mao, Ben Hoyleand the SAGA team
Marla Geha
The Milky Way’s Satellite Population ~1000 satellite galaxies predicted 2005: 11 satellite galaxies
Dwarf Galaxies (pre-2005)
The “Missing Satellite Problem”
2014: 25 satellite galaxies2015: 41 satellite galaxies
Via Lactea
5020
Small Scale Problems: Missing Satellites
Observations
Predictions
Mass of Satellite Galaxy
Num
ber o
f Sat
ellit
e G
alax
ies
5020
Observations
Predictions
new satellites
Num
ber o
f Sat
ellit
e G
alax
ies
Mass of Satellite Galaxy
Small Scale Problems: Missing Satellites
SDSS suggests LMC/SMC are unusual for a MW-mass halo,
but not uncomfortably so.
Velocity Dispersion (km/s)1006020 1006020
Velocity Dispersion (km/s)
Milky Way: Observed Milky Way: Predicted
Small Scale Problems: TBTF
MV
-16
-12
-8
-20
N (MV< -13) = 4 N (MV< -13) = 12
Many papers written comparing one observation (Milky Way) to one simulation!
The SAGA Project
Need a statistical sample (~100) of MWs,requires a volume out to 50 Mpc.
The properties of satellites observed around our Milky Way Galaxy disagree with model predictions.
Are models incorrect? Or is our Milky Way galaxy an outlier?
@ 30 Mpc, Rvir ~1 deg
Photometric redshifts for z < 0.05 are useless!
@ 30 Mpc, MV = -13 => mv = 21
The SAGA Project
Confirmed Satellites
Confirmed Background Galaxies
To move forward, need a training set of galaxies
w/spectra down to r < 21
NGC 6181 field: >3000 spectra to r=21.Most are background galaxies or stars. There are 8 satellites in here at z=0.008!
Building a Spectroscopic Training Set
Slide from B. Weiner
The SAGA Project
Candidate Satellites w/in virial radius:
-- All galaxies: ~10,000-- Basic Color cuts: ~1000-- Aggressive cuts: ~500
B. Hoyle: Machine learning using all photometric properties from SDSS has improved selection significantly
-- Machine Learning: ~150
Confirmed Satellites
Confirmed Background Galaxies