4-PARAMETER TRANSFORMATION OF DIGITIZED ASTRONOMICAL IMAGES Yavor Chapanov 1 1 – National...
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Transcript of 4-PARAMETER TRANSFORMATION OF DIGITIZED ASTRONOMICAL IMAGES Yavor Chapanov 1 1 – National...
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4-PARAMETER TRANSFORMATION OF DIGITIZED ASTRONOMICAL IMAGES
Yavor Chapanov1
1 – National Institute of Geophysics, Geodesy and Geography, Bulgarian Academy of Sciences
VIII Serbian-Bulgarian Astronomical Conference: 8-12 May 2012, Leskovac, Serbia
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VIII Serbian-Bulgarian Astronomical Conference: 8-12 May 2012, Leskovac, Serbia
4-, 3- parameter transformation – Z, Cz, Rx and Ry are zeroes
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DATA SIMULATIONPLATE SCALE <100"/mm
SCAN RESOLUTION 2400dpi IDENTICAL STAR SETS PRELIMINARY UNIFIED DATA REFRACTION AND DISTORTION CORRECTIONS
ACCURACY: (I) 0”.5 – the best case, (II) 1”.0 – middle precision, (III) 5”.0 – poor accuracy
Systematic errors:Image rotation 2 arcmin; Center shift 5 Scales 1*10-4; 1*106 (=2)
VIII Serbian-Bulgarian Astronomical Conference: 8-12 May 2012, Leskovac, Serbia
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VIII Serbian-Bulgarian Astronomical Conference: 8-12 May 2012, Leskovac, Serbia
Field Width: 02Ê00' Center RA: 02h 00m 00s, Center DE: 42Ê00'00ºEquinox: J2000North is Up, East is LeftSource catalog: GSC-ACTCreated by StarGazer version 1.3.0-dev(C)2001-2005by Rumen G.Bogdanovski
STAR POSITIONS
317 stars
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Ðàçïðåäåëåíèå íà ãðåøêàòà íà ñèìóëèðàíèòå íàáëþäåíèÿ
Ôèò y = 10000 * 0.01769 * normal (x, 0.001654, 0.141115)
[arcsec]
Áðîé
íà íàáëþäåíè
ÿòà
0
50
100
150
200
250
300
350
400
450
500
550
600
650
-0.8 -0.7 -0.6 -0.5 -0.4 -0.3 -0.2 -0.1 0.0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8
A MODEL OF TIPICAL ASTROMETRIC ERRORS 10000 Normally distributed numbers N (0, 0.1)
Replaced by:1% evenly distributed numbers from intervals (0.8, 0.4], [0.4, 0.8);6% evenly distributed numbers from intervals (0.4, 0.1], [0.1, 0.4);6% evenly distributed numbers from intervals (0.06, 0.06).
Resulting =0.14
Re-scaling as:0”.5; 1”.0; 5”.0
VIII Serbian-Bulgarian Astronomical Conference: 8-12 May 2012, Leskovac, Serbia
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ERROR MODEL – IStandard 0.5 arcsec
VIII Serbian-Bulgarian Astronomical Conference: 8-12 May 2012, Leskovac, Serbia
Coordinate Frame Rotation2 translations, 1 rotation, scale correction 180.03 X vector [arcsec] 240.02 Y vector [arcsec] -119.48 Z angle [arcsec] 92.96 Scale [ppm]
Quality criteria2.75 Maximum spatial residual [arcsec]0.60 Average spatial residual [arcsec]0.41 Root mean Square (RMS) of residuals [arcsec]
X=180as, Y=240as, Rz=-120as, S=100ppm
Max. errors <0”.05
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ERROR MODEL – IIStandard 1.0 arcsec
VIII Serbian-Bulgarian Astronomical Conference: 8-12 May 2012, Leskovac, Serbia
Coordinate Frame Rotation2 translations, 1 rotation, scale correction 180.03 X vector [arcsec] 240.01 Y vector [arcsec]-121.28 Z angle [arcsec] 99.20 Scale [ppm]
Quality criteria5.23 Maximum spatial residual [arcsec]0.86 Average spatial residual [arcsec]0.66 Root mean Square (RMS) of residuals [arcsec]
X=180as, Y=240as, Rz=-120as, S=100ppm
Max. errors <0”.05
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ERROR MODEL – IIIStandard 5.0 arcsec
VIII Serbian-Bulgarian Astronomical Conference: 8-12 May 2012, Leskovac, Serbia
Coordinate Frame Rotation2 translations, 1 rotation, scale correction 180.24 X vector [arcsec] 240.15 Y vector [arcsec] -112.12 Z angle [arcsec] 87.20 Scale [ppm]
Quality criteria28.29 Maximum spatial residual [arcsec] 6.07 Average spatial residual [arcsec] 4.31 Root mean Square (RMS) of residuals [arcsec]
X=180as, Y=240as, Rz=-120as, S=100ppm
Max. errors <0”.4
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VII BSAC "ASTROINFORMATICS" – Chepelare, 1-4 June 2010
Position errors 0”.5 + PM errors 0”.5/a*10a
Coordinate Frame Rotation2 translations, 1 rotation, scale correction 180.22 X vector [arcsec] 240.15 Y vector [arcsec] -112.78 Z angle [arcsec] 143.54 Scale [ppm]
Quality criteria39.46 Maximum spatial residual [arcsec] 5.55 Average spatial residual [arcsec] 4.46 Root mean Square (RMS) of residuals [arcsec]
X=180as, Y=240as, Rz=-120as, S=100ppm
Max. errors <0”.5
PROPER MOTION ERRORS
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VII BSAC "ASTROINFORMATICS" – Chepelare, 1-4 June 2010
Standard 1.0 arcsec
Coordinate Frame Rotation2 translations, 1 rotation, scale correction 360.03 X vector [arcsec] 480.03 Y vector [arcsec] -119.47 Z angle [arcsec] 1000085.93 Scale [ppm]
Quality criteria5.5 Maximum spatial residual [arcsec] 1.2 Average spatial residual [arcsec] 0.8 Root mean Square (RMS) of residuals [arcsec]
X=360as, Y=480as, Rz=-120as, S=1, =2
Max. errors <0”.6
A CASE OF LARGE SCALE
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CONCLUSIONS
It is possible to estimate the rotation and image center of digitized astronomical plates by the 4-parameter Helmert transformation if the number of identical stars is more than 100. The estimation accuracy is better than 0.4as for plates with 100”/mm scale, scan resolution 2400dpi and total rms errors of star positions below 5as.
The necessary preprocessing of digitized astronomical images are image convert to small scale, determination of identical stars from the image and star catalog and correction of the atmosphere refraction and distortions due to telescope optics and projection of celestial sphere over the focal plane.
VIII Serbian-Bulgarian Astronomical Conference: 8-12 May 2012, Leskovac, Serbia
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VIII Serbian-Bulgarian Astronomical Conference: 8-12 May 2012, Leskovac, Serbia