7.2 Gain
Gain, a fundamental scaling parameter of the IR detector, relates the registered number of analog-to-digital units (ADUs) or equivalently, data numbers (DNs), to the number of accumulated photoelectrons. Like the UVIS channel, the Analog to Digital Converter (ADC) outputs a 16-bit number, allowing output signal values ranging from 0 to 65535 (i.e 216 -1) for each pixel.
The WFC3 IR detector has a nominal gain setting of 2.5 e¯/DN in order to provide complete sampling of the full-well of the IR detector (~80,000 electrons, which is ~32,000 DN at the nominal gain). Due to slight hardware differences, effective gain values in each quadrant of the detector deviate slightly from the nominal gain. Twice yearly, the effective gain is measured via the mean-variance technique on pairs of internal flat fields: the mean signal level is plotted against the variance in signal, and the gain is the inverse of the slope. See WFC3 ISR 2015-14 for more information on this method and the status of the IR gain from 2010-2015. Table 7.1 summarizes the current values of the effective gain measured in each quadrant of the IR detector. The WFC3 group will continue to monitor the effective gain of the detector twice yearly to evaluate its stability over time.
Table 7.1: Gain measurements for each quadrant in e-/DN, averaged over all epochs of observations. Quadrants 1, 2, 3, and 4 are the 512 × 512 pixel detector quadrants that are read out independently from the outer corner.
Quadrant. | Gain | Error |
---|---|---|
1 | 2.252 | 0.054 |
2 | 2.203 | 0.039 |
3 | 2.188 | 0.036 |
4 | 2.265 | 0.053 |
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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
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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