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1 Preliminary Design Review • Tucson, Arizona • August 29 th – September 2 nd , 2011 Preliminary Design Review • Tucson, Arizona • August 29 th – September 2 nd , 2011 Data Management: Input Data Prepared by: Simon Krughoff ImSim Project: University of Washington LSST Preliminary Design Review August 29-September 2, 2011

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Data Management: Input Data Prepared by: Simon Krughoff ImSim Project: University of Washington LSST Preliminary Design Review August 29-September 2, 2011. Input Data. Summary Simulated Imagery Simulated operations Simulated time variable sky Atmosphere/Optics model CFHT Imagery - PowerPoint PPT Presentation

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Page 1: Input Data

1Preliminary Design Review • Tucson, Arizona • August 29th – September 2nd, 2011Preliminary Design Review • Tucson, Arizona • August 29th – September 2nd, 2011

Data Management: Input Data

Prepared by: Simon KrughoffImSim Project: University of Washington

LSST Preliminary Design ReviewAugust 29-September 2, 2011

Page 2: Input Data

2Preliminary Design Review • Tucson, Arizona • August 29th – September 2nd, 2011

Input Data

Summary – Simulated Imagery

– Simulated operations– Simulated time variable sky– Atmosphere/Optics model

– CFHT Imagery– Camera design

– Focal plane layout– Electronic properties

– Calibration Products

Page 3: Input Data

3Preliminary Design Review • Tucson, Arizona • August 29th – September 2nd, 2011

Input Data: Simulated Imagery

− Simulated Observations– 10 years – ~3 Million

observations– Historical weather and

downtime– Filter and location

chosen to satisfy science programs

– Realistic slew, exposure, and shutter times

Page 4: Input Data

4Preliminary Design Review • Tucson, Arizona • August 29th – September 2nd, 2011

Input Data: Simulated Imagery

− Simulated Sky– Galactic structure model from

Juric et al. (2008), Amores & Lepine (2005), Schlegel, Finkbeiner, & Davis (1998)

– Solar system model from Grav et al. (2010)

– Extragalactic positions from White with semi-analytic properties from De Lucia

– Variable AGN/QSOs, Cepheids, RRLy, eclipsing binaries, AM CVn, microlensing events, M-dwarf flare

Page 5: Input Data

5Preliminary Design Review • Tucson, Arizona • August 29th – September 2nd, 2011

Input Data: Simulated Imagery

− Atmosphere/Optics Model – 6 moving screen model

normalized to seeing from OpSim with historical wind velocity

– Kolmogorov spectrum cloud model informed by historical cloud coverage data

– Full optical system model

Page 6: Input Data

6Preliminary Design Review • Tucson, Arizona • August 29th – September 2nd, 2011

Input Data: Simulated Imagery

Page 7: Input Data

7Preliminary Design Review • Tucson, Arizona • August 29th – September 2nd, 2011

CFHT Data

− ~19,000 MegaCam images– 23 May 2003 to 16 Feb

2008− 36 two amp CCDs in

rectangular grid− 1deg x 1deg fov− u*,g,r,i,z filters (note the u*

is broader than the LSST u)− Bias Frames− Flat Frames− Fringe Frames for i and z

images.

Page 8: Input Data

8Preliminary Design Review • Tucson, Arizona • August 29th – September 2nd, 2011

Camera and Electronics Model

− Focal plane layout– 189 imaging chips:

2000x2072 pix– 4 wavefront sensors– 21 3x3 rafts

− Electronic design– 8x2 Amps per chip– 509x1000 pix per amp

Page 9: Input Data

9Preliminary Design Review • Tucson, Arizona • August 29th – September 2nd, 2011

Calibration Products

− 10 realizations with 2 exposures per realization

− Reduced using DM stack to produce master calibration frames.

− Bias frames– zero length exposures

− Dark frames– 180 sec exposures with

shutter closed− Per filter flats

– Analytic fit to vignetting function sampled to place photons.