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A1260881171qOxil

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Gravitational Lensing. Light from a distant galaxy is bent around a mass ... Gravitational Lensing. Galaxies seen through dark matter distribution analogous to ... – PowerPoint PPT presentation

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Title: A1260881171qOxil


1
PASCAL Workshop, Bled 28 Jan 2008 Sarah Bridle
(UCL) on behalf of the GREAT08 Team
PASCAL Challenge
2
Contents of our Universe
70 Dark Energy
5 Baryonic Matter
25 Dark Matter
3
Gravitational Lensing
Light from a distant galaxy is bent around a mass
4
Gravitational Lensing
Galaxies seen through dark matter distribution
analogous to Streetlamps seen through your
bathroom window
5
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6
Cosmic Lensing
gi0.2
Real data gi0.03
7
Atmosphere and Telescope
Convolution with kernel
Real data Kernel size Galaxy size
8
Pixelisation
Sum light in each square
Real data Pixel size Kernel size /2
9
Noise
Mostly Poisson. Some Gaussian and bad
pixels. Uncertainty on total light 5 per cent
10
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11
Typical galaxy used for cosmic shear analysis
Typical star Used for finding Convolution kernel
12
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13
GREAT08 Data
  • 10 000 images
  • divided into 10 sets

One galaxy per image Kernel is given One shear
per set Noise is Poisson
100 000 000 images Divided into 1000 sets
14
GREAT08 Results
You submit g1, g2 for each set of images
15
GREAT09 and Beyond
  • Kernel is not given (just kernel images)
  • Galaxies with more complicated shapes
  • Kernel is more realistic
  • Many objects in each image
  • Correlated noise
  • Poisson Gaussian noise bad pixels
  • Shear is different for each galaxy
  • Kernel is not the same for every galaxy
  • Cosmic rays, satellite tracks, saturated stars
  • Multiple exposures
  • Pixels not exactly square or on a grid

16
GREAT08 Timeline
  • 8 Feb 2008 GREAT08 Handbook public
  • Feb 2008 Produce simulations
  • Mar 2008 Internal analysis of simulations
  • May 2008 Release simulations
  • Leaderboard starts containing best internal
    results
  • Nov 2008 Competition deadline
  • Dec 2008 Workshop Release final report
  • Input shears public

www.great08challenge.info
17
GREAT08 Summary
  • 100 million images
  • 1 galaxy per image
  • De-noise, de-convolve, average ? shear
  • gi 0.03 to accuracy 0.0003 ? Q1000 ? Win!

18
cosmocoffee.info
19
GREAT08
20
Understanding Cosmology
21
GREAT08 Summary
  • 100 million images
  • 1 galaxy per image
  • De-noise, de-convolve, average ? shear
  • gi 0.03 to accuracy 0.0003 ? Q1000 ? Win!

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22
Questions for you
  • Is there too much astronomy to learn?
  • Yes
  • No
  • Is timeline (6 months) right?
  • Too short
  • Fine
  • Too long
  • Is this potentially on your research agenda?
  • No
  • Maybe
  • Yes

23
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