1 Time-Delayed Integration/ Drift scanning William van Altena Yale University Basic Astrometric Methods Yale University July 18-22, 2005
2 The Bucket Brigade
3 Observed strip of the sky
4 RA Sample Drift Scan
5 Geometry of Scan Across CCD
6 Coordinates on the CCD
7 The Celestial Sphere
8 Declination Degradation
9 Normal Declination Limits
10 Going to Higher Dec. Limits
11 star track star trail North South West East 25.0 cm 19.3 cm Drift-scanning
12 Relative Reductions
13 Aberration of Starlight
14 Declination Overlap Errors
15 RA Overlap Errors
16 Precision of scan to scan registration
17 Sources of Errors
18 Reference Star Catalog Errors
19 Schmidt Telescope Errors
20 Dynamic Range
21 Error versus Magnitude
22 Error versus Zenith Distance
23 Precision Limits
24 Accuracy Limits & the Atmosphere
25 Precision Limits & the Atmosphere
26 Precision versus Aperture
27 World’s Largest CCD Cameras Palomar-Quest x2400 Sloan x2048 Megacam x4612 SuprimeCam x cm
28 The Sloan Camera (SDSS)
29 Palomar/Quest Camera
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31 Orion Nebula Driftscan: BRI-composite, 140-sec exposure Palomar Quest
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