ACS/WFC
Geometric Distortion and CTE
V. Kozhurina-Platais & ACS team
ACS/WFC geometric distortion is changing linearly with timeAnderson J., ISR-ACS/WFC , August 2006 a) Standard astrometric reference field (47Tuc) ~ 53,000 stars b) User friendly software - XYM2MAT
Our plan was to: a) Check the time-dependency on FLT images; b) Implement the time dependency in MultiDrizzle c) Verify the implementation
The observations of 47Tuc
• F606W filter • 2002-2006 (PIP-9018-10771)• different orientations• different postargs• different exposures: 22 - 1200s
The reductions:
• effective PSF fitting on FLT - X,Y mag; • standard frame: 2002 March, 690s, F606W,=-163
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tgθ =B
D
tg(θ + γ ) = −A
C
tgγ = −A ⋅B + C ⋅DA ⋅D − C ⋅B
Ouv - standard orthogonal system MXY - measured system
Kiselev A.A, 1989, pub.,”Nauka”, St.Petersburg, Russia
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u
v
⎛
⎝ ⎜
⎞
⎠ ⎟=
AB
CD
⎡
⎣ ⎢
⎤
⎦ ⎥X − Xo
Y −Yo
⎛
⎝ ⎜
⎞
⎠ ⎟+
uo
vo
⎛
⎝ ⎜
⎞
⎠ ⎟
X
Y
Xo
YoO
M
90+
u
v
Y
X
uo
vo
720 s , =-163.2 2002.4
22 s , =- -23.9 2004.7
22 s, = 51.9 2005.9
22 s , = -117.9 2002.4
22 s , = -67.82005.0
22 s , = -122.92004.5
The skew term as
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=arctan −A ⋅B + C ⋅DA ⋅D − C ⋅B
⎛ ⎝ ⎜
⎞ ⎠ ⎟
€
α = 0.095 + 0.090 ⋅(date − 2004.5)/2.5
β = −0.029 − 0.030 ⋅(date − 2004.5)/2.5
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fx = (Xc − 2048) 2048
fy = (Yc − 2048) 2048
Xo = fx + β ⋅ fx + α ⋅ fy
Yo = fy + β ⋅ fy + α ⋅ fx
Many variables: PID - 10368:• The same pointing
• Exposures - 400s, 30s
• Two orientations : +154.8, -29.4
exposure
pointing
orientation
epoch
LAMP=OFF/OFF
400sec--> 400sec, 154.7-> 154.7
400sec--> 400sec, 154.7-> -29.4
30sec--> 400sec, 154.7-> 154.7
30sec--> 400sec, 154.7-> 154.7
30sec--> 400sec, 154.7-> 154.7
30sec--> 400sec, -29.4->-29.4
LAMP=OFF/OFF
LAMP=OFF/OFF
LAMP=MED/OFF
LAMP=HIGH/OFF
LAMP=LOW/OFF
Schematic illustration of the WFC1 and WFC2 plane:- Red arrows show the readout direction- Green color shows the PSF profile affected by CTE
Conclusions The CTE-induced centroid shift depends on: magnitude of a star position on a CCD chip sky background The amplitude of CTE-induced centroid shift is ~ 0.1 pix CTE effect leads to a discontinuity in the reference frame Accounting for CTE effect is critical to reach a 1 mas accuracy requirement for JWST standard astrometric field