10.4 References
Deming, D., et al., Infrared Transmission Spectroscopy of the Exoplanets HD209458b and XO-1b Using the Wide Field Camera-3 on the Hubble Space Telescope, 2013, ApJ, 774, 95.
van Dokkum, P., 2001. L.A. Cosmic., Laplacian Cosmic Ray Identification.
McCullough, P. & MacKenty, J., WFC3 ISR 2012-08, Considerations for using Spatial Scans with WFC3.
Petro, L. & Wheeler, T., WFC3 ISR 2006-06 New IR Detector Sample Times.
Reiss, A., Casertano, S., et al., Parallax beyond a kiloparsec from spatially scanning the Wide Field Camera 3 on the Hubble Space Telescope, 2014, ApJ, 785, 2.
Casertano, S., et al., Parallax of galatic Cephids from spatially scanning the Wide Field Camera 3 on the Hubble Space Telescope: the Case of SS Canis Majoris, 2016, ApJ, 825, 1.
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WFC3 Data Handbook
- • Acknowledgments
- Preface
- Chapter 1: WFC3 Instruments
- Chapter 2: WFC3 Data Structure
- Chapter 3: WFC3 Data Calibration
- Chapter 4: WFC3 Images: Distortion Correction and AstroDrizzle
- Chapter 5: WFC3-UVIS Sources of Error
- Chapter 6: WFC3 UVIS Charge Transfer Efficiency - CTE
-
Chapter 7: WFC3 IR Sources of Error
- • 7.1 WFC3 IR Error Source Overview
- • 7.2 Gain
- • 7.3 WFC3 IR Bias Correction
- • 7.4 WFC3 Dark Current and Banding
- • 7.5 Blobs
- • 7.6 Detector Nonlinearity Issues
- • 7.7 Count Rate Non-Linearity
- • 7.8 IR Flat Fields
- • 7.9 Pixel Defects and Bad Imaging Regions
- • 7.10 Time Variable Background Contamination
- • 7.11 IR Photometry Errors
- • 7.12 References
- Chapter 8: Persistence in WFC3 IR
- Chapter 9: WFC3 Data Analysis
- Chapter 10: WFC3 Spatial Scan Data