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2010/11/04-05 SKA Japan Workshop 2010/11/04-05 SKA Japan Workshop

2010/11/04-05 SKA Japan Workshop - PowerPoint Presentation

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2010/11/04-05 SKA Japan Workshop - PPT Presentation

1 VariableStep Frequency Integration in the DecadeCenturyBand Imaging 2010 Nov 45 SKA Japan Workshop Mitaka Tomoharu Kurayama Kagoshima Univ Abstract In decadecenturyband imaging we have a problem in the frequency integration ID: 657217

japan ska 2010 workshop ska japan workshop 2010 frequency integration imaging grids simulation visibilities image pixels images transform loci

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Slide1

2010/11/04-05

SKA Japan Workshop

1

Variable-Step Frequency Integration in the Decade/Century-Band Imaging

2010 Nov 4-5

SKA Japan Workshop @

Mitaka

Tomoharu Kurayama

(Kagoshima Univ.)Slide2

Abstract

In decade/century-band

imaging, we have a problem in the frequency integration.We propose the variable-step frequency integration in order to minimize this problem.From the simple

simulation, synthesized beams and images become more sharp in the variable-step frequency integration.

2010/11/04-05

SKA Japan Workshop

2Slide3

Synthesis Imaging

Synthesized images are Fourier transforms of visibilities on (u, v) planes.

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SKA Japan Workshop

3

Fourier Transform

Image

Visibilities

(Observables)

RA

l

m

dec

u

v

(Taylor,

Carilli

&

Perley

ed

. 1999

)

I(

l,m

)

V(

u,v

)Slide4

Integration for Weak Sources

We can detect low-flux sources by integrating frequency points.

2010/11/04-05

SKA Japan Workshop

4

Integration

of images

Integration

of visibilities

RA

l

m

dec

I

1

(

l,m

)

I

3

(

l,m

)

I

2

(

l,m

)

sensitivity

u

v

V

1

(

u,v

)

V

2

(

u,v

)

V

3

(

u,v

)

frequency

frequencySlide5

Current Data Analysis

Integrating frequency points of visibilities

2010/11/04-05

SKA Japan Workshop

5

Making images with Fourier transform

frequency

Frequency-integrated visibilities

Images

RA

l

m

dec

I(

l,m

)

u

v

V(

u,v

)

u

v

V

1

(

u,v

)

V

2

(

u,v

)

V

3

(

u,v

)Slide6

What is (u, v)?

(u, v) : Projected baseline lengths in the unit of

wavelengths

2010/11/04-05

SKA Japan Workshop

6

(u, v)s depend on

frequencie

s!

earth

u-direction

v-direction

w-direction

L

x

L

y

observing sourceSlide7

Problem in Decade/Century Bands

e.g.) VERA

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SKA Japan Workshop

7

Decade band

22 GHz

Bandwidth ~ 0.25 GHz

1 GHz

10 GHz

We can NOT ignore

the effect of bandwidth in the case of decade/century band.

integrating areaSlide8

Visibility Gridding

Requirement of FFT :

Data points are on rectangular gridsWe need ‘gridding’ before Fourier transform

2010/11/04-05

SKA Japan Workshop

8

gridding

When

the point distribution is more uniform,

We can get more points in the process of gridding, and

The quality

of image becomes more sharp.Slide9

(u, v) Loci and Frequency Step

(u, v) change with the earth’s spin.

The loci are ellipse if we can observe 24 hours.

2010/11/04-05

SKA Japan Workshop

9

length

area

Frequency :

Frequency :

The numbers of points are same for

both loci

.

The point distribution is more uniform when

:

: Slide10

Simple Simulation

Considering SKA…

Band : 1 – 10 GHz10-hour observationTime step : 48 s

48 stations2010/11/04-05

SKA Japan Workshop

10

~ 5 km

~ 180 km

12 stations

~ 500 km

12 stations

24

stations

30

o

S

north

uv

loci of one baseline, one frequency pointSlide11

(u, v) Loci of One Baseline

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SKA Japan Workshop

11Slide12

(u, v) Loci of All Baselines

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SKA Japan Workshop

12Slide13

Sampled Grids

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SKA Japan Workshop

13

462382 grids

1024 grids

1024 grids

Total : 1048576 grids

758383 gridsSlide14

Synthesized Beam

2010/11/04-05

SKA Japan Workshop

14

0.109

0.122

0.235

0.371

Width of main beam is smaller.

First

sidelobe

is slightly higher.

~ 14 pixels

~ 14 pixelsSlide15

Imaging Simulation : Method

Making model visibilities with Fourier transform

Picking up the grids covered by (u, v) lociGetting simulated images with inverse transform

2010/11/04-05

SKA Japan Workshop

15

model image

model visibilities

FT

inverse Fourier transform

observed image

0

0

0

0

0

0

0

0

0

0

0

0

0

0Slide16

Imaging Simulation : Result (1)

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16

model image

1024 pixels

1024 pixels

1024 pixelsSlide17

Imaging Simulation : Result (2)

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17

model image

100 pixelsSlide18

Imaging Simulation : Result (3)

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SKA Japan Workshop

18

model image

25

pixelsSlide19

Summary

We have proposed a new type of frequency integration for decade/century-band imaging.

Setting the frequency step asFrom a simple simulation, we have found

The sampled points distribute more uniformly on (u, v) planeSynthesized beams and images become more sharp

2010/11/04-05

SKA Japan Workshop

19Slide20

Thank you!

2010/11/04-05

SKA Japan Workshop

20

2010 Oct 24 Triathlon in

Tokunoshima

(swim 2 km / bike 75 km / run 21 km)