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Variable-Step Frequency Integration in the Decade/Century-Band Imaging. 2010 Nov 4-5 SKA Japan Workshop @ Mitaka Tomoharu Kurayama (Kagoshima Univ.). Abstract. In decade/century-band imaging, we have a problem in the frequency integration. - PowerPoint PPT Presentation
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SKA Japan Workshop 12010/11/04-05
Variable-Step Frequency Integration in the
Decade/Century-Band Imaging
2010 Nov 4-5SKA Japan Workshop @ Mitaka
Tomoharu Kurayama(Kagoshima Univ.)
SKA Japan Workshop 2
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 3
Synthesis Imaging►Synthesized images are Fourier
transforms of visibilities on (u, v) planes.
2010/11/04-05
Fourier Transform
ImageVisibilities
(Observables)
RA
lmdec
uv
(Taylor, Carilli & Perley ed. 1999)
I(l,m) V(u,v)
)(2),(),( vmulievuVdvdumlI
SKA Japan Workshop 4
Integration for Weak Sources►We can detect low-flux sources by
integrating frequency points.
2010/11/04-05
Integration of images
Integration of visibilities
)(221
)(22
)(21 )( mulimulimuli eVVddueVddueVddu
N11
RA lmdec I1(l,m)
I3(l,m)I2(l,m)
sensitivity
uv
V1(u,v)V2(u,v)
V3(u,v)
frequency frequen
cy
SKA Japan Workshop 5
Current Data AnalysisIntegrating frequency points of visibilities
2010/11/04-05
Making images with Fourier transform
frequency
Frequency-integrated visibilities
Images
RAlm
dec I(l,m)
uv
V(u,v)
uv
V1(u,v)V2(u,v)
V3(u,v)
SKA Japan Workshop 6
What is (u, v)?►(u, v) : Projected baseline lengths in
the unit of wavelengths
2010/11/04-05
►(u, v)s depend on frequencies!
earthu-direction
v-direction
w-direction
Lx
Ly
cLLcLLu
yy
xx
observing source
SKA Japan Workshop 7
Problem in Decade/Century Bands
►e.g.) VERA
2010/11/04-05
►Decade band
cLL yy
cLLu xx
cLL yy
cLLu xx
22 GHz Bandwidt
h ~ 0.25 GHz
1 GHz
10 GHz
► We can NOT ignore the effect of bandwidth in the case of decade/century band.
integrating area
SKA Japan Workshop 8
Visibility Gridding► Requirement of FFT :
Data points are on rectangular grids► We need ‘gridding’ before Fourier transform
2010/11/04-05
cLL yy
cLLu xx
cLL yy
cLLu xx
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.
SKA Japan Workshop 9
(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
cLL yy
cLLu xx
length
area2
1
Frequency :
Frequency : 1
222
11
► The numbers of points are same for both loci.
► The point distribution is more uniform whenconstant
: :
SKA Japan Workshop 10
Simple Simulation►Considering SKA…
Band : 1 – 10 GHz 10-hour observation Time step : 48 s 48 stations
2010/11/04-05
~ 5 km
~ 180 km12 stations
~ 500 km12 stations
24 stations
30o S nort
h
► uv loci of one baseline, one frequency point
SKA Japan Workshop 11
(u, v) Loci of One Baseline
2010/11/04-05
constant constant
SKA Japan Workshop 12
(u, v) Loci of All Baselines
2010/11/04-05
constant constant
SKA Japan Workshop 13
Sampled Grids
2010/11/04-05
constant
constant
462382 grids
1024 grids
1024
gr
ids
Total : 1048576 grids
758383 grids
SKA Japan Workshop 14
Synthesized Beam
2010/11/04-05
constant constant
0.109
0.122
0.235
0.371
►Width of main beam is smaller.
►First sidelobe is slightly higher.
~ 14 pixels
~ 14 pixels
SKA Japan Workshop 15
Imaging Simulation : Method►Making model visibilities with Fourier
transform►Picking up the grids covered by (u, v) loci►Getting simulated images with inverse
transform
2010/11/04-05
model image
model visibilities
FTinverse Fourier transformobserve
d image
0 0
0
0
0
0
0 0 00 0 0
0
0
SKA Japan Workshop 16
Imaging Simulation : Result (1)
2010/11/04-05
model image
constant constant
1024 pixels
1024 pixels
1024 pixels
SKA Japan Workshop 17
Imaging Simulation : Result (2)
2010/11/04-05
model image
constant constant
100 pixels
SKA Japan Workshop 18
Imaging Simulation : Result (3)
2010/11/04-05
model image
constant constant
25 pixels
SKA Japan Workshop 19
Summary►We have proposed a new type of
frequency integration for decade/century-band imaging. Setting the frequency step as
►From a simple simulation, we have found The sampled points distribute more
uniformly on (u, v) plane Synthesized beams and images become
more sharp2010/11/04-05
constant
SKA Japan Workshop 20
Thank you!
2010/11/04-05
2010 Oct 24 Triathlon in Tokunoshima(swim 2 km / bike 75 km / run 21 km)