18 th Conference on Gravitational Microlensing Microlensing Planetary and Binary Statistics from...
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18th Conference on Gravitational Microlensing
Microlensing Planetary and Binary Statistics from 2011-2013
Generation-II OGLE-MOA-Wise
Yossi Shvartzvald Tel-Aviv University with Dan Maoz, Matan Friedmann (TAU)in collaboration with OGLE, MOA, µFUN
18th Conference on Gravitational Microlensing
Microlensing statistics – snowline planet frequency
Gould et al. 2010 (6 planets):
~1/3 of stars have snowline-region giant planets
~1/6 of stars have solar-like planetary systems
Sumi et al. 2010 (10 planets):
Neptunes are at least 3 times more common than Jupiters
Cassan et al. 2012 (3 planets+Gould10+Sumi10):
~1/6 host Jupiters
~1/2 host Neptunes
~2/3 host super-Earths
18th Conference on Gravitational Microlensing
Second generation survey
A different approach:
1. Controlled experiment:
Untargeted survey, specific field (high mag + low mag)
Continuous coverage
2. Forward modeling for planet abundance:
Simulate the experiment
Define planetary anomaly detection threshold (not necessarily perfectly modeled events)
Compare data to simulation
18th Conference on Gravitational Microlensing
The generation-II network
OGLE, Chile, 1.3m MOA, NZ, 1.8m
Wise Obs., Israel, 1m
18th Conference on Gravitational Microlensing
Second generation microlensing survey
• 8 deg2 of bulge with highest lensing rate• covered quasi-continuously by all 3 telescopes• cadences 20-40 min
18th Conference on Gravitational Microlensing
What to expect from Generation II?a simulation:
Monte-Carlo of many Solar-System-like planetary systems, host star properties matching those of bulge microlensing population, random inclinations.
Shvartzvald & Maoz 2012
Simulating the experiment
18th Conference on Gravitational Microlensing
Simulating the experiment
Ray trace through systems……
…search for planetary-type anomalies with same detection criteria as real data
…add real sampling sequences, photometry errors…
18th Conference on Gravitational Microlensing
Shvartzvald & Maoz 2012
S
Simulation results:
can detect ~15-20% of planets around microlensed stars;
Simulating the experiment
18th Conference on Gravitational Microlensing
2011-2013 sample
Sample Criteria:
• u0<=1
• t0 within Wise season
• Data from all 3 groups
18th Conference on Gravitational Microlensing
2011-2013 sample
Sample Criteria:
• u0<=1
• t0 within Wise season
• Data from all 3 groups
Events
245 Sample
18th Conference on Gravitational Microlensing
Comparison to simulation - u0
Shvartzvald & Maoz 2012
Simulation 2011-2013 sample
18th Conference on Gravitational Microlensing
Comparison to simulation - tE
Shvartzvald & Maoz 2012
Simulation 2011-2013 sample
18th Conference on Gravitational Microlensing
tE distribution
Sumi et al. 2011
MOA-II 2006-2007 2011-2013 sample
18th Conference on Gravitational Microlensing
Anomalous events
Events
245 Sample
29) 11.8%( Anomalous
8) 3.3%( Planetary
Mass ratio
18th Conference on Gravitational Microlensing
Anomalous events
Events
245 Sample
29) 11.8%( Anomalous
8) 3.3%( Planetary
Mass ratio
Accounting for detection efficiency,>17% planetary system frequency
18th Conference on Gravitational Microlensing
Gen-II planets
???
From the 16th microlensing conference in Pasadena
18th Conference on Gravitational Microlensing
Gen-II planets
• MOA-11-322
Shvartzvald et al. 2014
13.45.6
1.51.2
0.450.19
11.6
4.3 AU
0.39
P J
L
M M
a
M M
Super-Jupiter around M dwarf
18th Conference on Gravitational Microlensing
Gen-II planets
• MOA-11-322
• MOA-11-293
I-ba
nd (
mag
)I-
band
(m
ag)
HJD-2450000
Yee et al. 2012
OGLEMOAWise
Survey data only:
All data:
18th Conference on Gravitational Microlensing
Gen-II planets
• MOA-11-322
• MOA-11-293
I-ba
nd (
mag
)I-
band
(m
ag)
HJD-2450000
Yee et al. 2012
OGLEMOAWise
Survey data only:
All data:
4.8 0.3
1.1 0.1 AU
0.86 0.06
P J
L
M M
a
M M
Batista et al. 2013
First ML planet in the habitable zone
18th Conference on Gravitational Microlensing
Gen-II planets
• MOA-11-322
• MOA-11-293
• OGLE-11-265
0.38 0.05
1.15 0.13AU
0.085 0.013
P J
L
M M
a
M M
Saturn around M dwarf
modeled by C. Han
18th Conference on Gravitational Microlensing
Gen-II planets
• MOA-11-322
• MOA-11-293
• OGLE-11-265
• OGLE-12-406
Poleski et al. 2013, Tsapras et al. 2013
2.73 0.43
3.45 0.26 AU
0.44 0.07
P J
L
M M
a
M M
Super-Jupiter around M dwarf
18th Conference on Gravitational Microlensing
Gen-II planets
• MOA-11-322
• MOA-11-293
• OGLE-11-265
• OGLE-12-406
Poleski et al. 2013, Tsapras et al. 2013
2.73 0.43
3.45 0.26 AU
0.44 0.07
P J
L
M M
a
M M
Super-Jupiter around M dwarf
Super-Jupiters around low-mass stars are common?
18th Conference on Gravitational Microlensing
Galactic model from higher order statistics
Events
216 Sample
30% Parallax
>1% Finite source
18th Conference on Gravitational Microlensing
C28 telescope
A new telescope at Wise observatory:
• 0.71m telescope
• Fully robotic
• FOV: 1 degree2
• Together with 1m telescope,
higher cadence / more fields