5.8 References

S. Baggett, 2009, WFC3 TV3 Testing: UVIS-1 Crosstalk, WFC3 ISR 2009-03.

S. Baggett, 2009, Performance of WFC3 Replacement UVIS filters, WFC3 ISR 2007-01.

S. Baggett, E. Sabbi, P. McCullough, 2009, WFC3 SMOV Proposal 11422/ 11529: UVIS SOFA and Lamp Checks, WFC3 ISR 2009-27.

T. Borders, S. Baggett, 2009, WFC3 SMOV Proposals 11419, 11426, 11431, and 11448: On-Orbit Biases, WFC3 ISR 2009-26.

M. Bourque, S. Baggett, 2016, WFC3/UVIS Dark Calibration: Monitoring Results and Improvements to Dark Reference Files, WFC3 ISR 2016-08.

M. Bourque, D. Borncamp, S. Baggett, T. Desjardins, & N. Grogin, 2018, Using Dark Images to Characterize Pixel Stability in the WFC3/UVIS Detector, WFC3 ISR 2018-15.

T. M. Brown & O. Lupie, 2004, Filter Ghosts in the WFC3 UVIS Channel, WFC3 ISR 2004-04.

T. Brown, 2007, UVIS Channel Filter Ghosts after Filter Replacement, WFC3 ISR 2007-09.

T. Brown, 2007, WFC3 TV2 Testing: UVIS Channel Glint, WFC3 ISR 2007-21.

T. Brown, G. Hartig, S. Baggett, 2008, WFC3 TV3 Testing: UVIS Window Contamination, WFC3 ISR 2008-10.

S. E. Deustua et al., 2016, UVIS 2.0 Chip-dependent Inverse Sensitivity Values, WFC3 ISR 2016-03.

J. Fowler, L. Markwardt, M. Bourque, J. Anderson, 2017, Analysis of Dragon’s Breath and Scattered Light Detector Anomalies on WFC3/UVIS, WFC3 ISR 2017-02.

J. Fowler, 2018, WFC3/UVIS Gain Stability Results for Cycles 24 and 25, WFC3 ISR 2018-17.

R. L. Gilliland, 1994, Stellar Photometry Including Saturated Images: Results on M67 with WFPC2, ApJ, 435, L63-66.

R. L. Gilliland, P. Goudfrooij, and R. A. Kimble, 1999, Linearity and High Signal‐to‐Noise Performance of the STIS CCD, PASP, 111, 1009-1020.

R. L. Gilliland, 2004, ACS CCD Gains, Full Well Depths, and Linearity up to and Beyond Saturation, ACS ISR 2004-01.

R. L. Gilliland, A. Rajan and S. E. Deustua, 2010, WFC3 UVIS Full Well Depths, and Linearity Near and Beyond Saturation, WFC3 ISR 2010-10.

C.M. Gosmeyer & the Quicklook Team, WFC3 Anomalies Flagged by the Quicklook Team, WFC3 ISR 2017-22.

H. Gunning, C. Pavlovsky, S. Baggett, 2013, WFC3 Cycle 19 Proposal 12690: UVIS Gain, WFC3 ISR 2013-02.

H. Gunning, 2015, WFC3 Cycle 21 Proposal 13561: UVIS Gain, WFC3 ISR 2015-05.

B. Hilbert, 2009, UVIS Channel Shutter Shading, WFC3 ISR 2009-05.

B. Hilbert, 2010, WFC3 SMOV Program 11427: UVIS Channel Shutter Shading, WFC3 ISR 2009-25.

K. Huynh and B. Kuhn, WFC3/UVIS Gain Stability Results for Cycles 26-29, WFC3 ISR 2022-08.

K. Huynh and P. R. McCullough, UVIS Shutter Timing Jitter, WFC3 ISR 2023-04.

J. Janesick, 2001, Scientific charge-coupled devices, SPIE Optical Engineering Press, (Bellingham, WA).

H. Khandrika and S. Baggett, 2015, WFC3 UVIS Read Noise, WFC3 ISR 2015-13.

H. Khandrika, 2017, WFC3/UVIS Read Noise Aug 2009 - Apr 2017, WFC3 ISR 2017-17.

B. Kuhn and H. Khandrika, 2018 Superbias Reference File, WFC3 ISR 2019-11.

J. Mack, E. Sabbi, & T. Dahlen, 2013, In-flight Corrections to the WFC3 UVIS Flat Fields, WFC3 ISR 2013-10.

J. Mack, A. Rajan, & A.S. Bowers, 2015, Spatial Accuracy of the UVIS Flat Fields, WFC3 ISR 2015-18.

J. Mack, T. Dahlen, E. Sabbi, and A. S. Bowers, 2016, UVIS 2.0: Chip-Dependent Flats, WFC3 ISR 2016-04.

J. Mack, 2016, UVIS 2.0: Ultraviolet Flats, WFC3 ISR 2016-05.

R. van der Marel, 2003, Determination of Low-Frequency Flat-Field Structure from Photometry of Stellar Fields, ACS ISR 2003-10.

C. Martlin, 2016, WFC3 Cycle 23 Proposal 14373: UVIS Gain, WFC3 ISR 2016-13.

P. McCullough, 2011, Geometric model of UVIS window ghosts in WFC3, WFC3 ISR 2011-16.

J. V. Medina, 2021, UVIS Pixel Stability: Updates to The UVIS Bad Pixel Table Pipeline, WFC3 ISR 2021-14.

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M. V. Newberry, 1999, Increasing Precision and Accuracy in Photometric Measurements in Precision CCD Photometry, ASP Conference Series, Vol. 189, Edited by E. R. Craine, D. L. Crawford, and R. A. Tucker. ISBN: 1-58381-015-3 (1999), p.74.

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I. Rivera, M. Marinelli, J. Mack, WFC3/UVIS: New Full-Well Saturation Map Reference File, WFC3 ISR 2023-08.

M. Robberto & B. Hilbert, 2005, The Behaviour of the WFC3 UVIS and IR Analog-to-Digital Converters, WFC3 ISR 2005-27.

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E. Sabbi et al., 2009, WFC3 Calibration Using Galactic Clusters, WFC3 ISR 2009-06.

E. Sabbi, 2009, WFC3 SMOV PROGRAM 11452: UVIS Flat Field Uniformity, WFC3 ISR 2009-19.

Sabbi, E. and Bellini, A., 2013, UVIS PSF Spatial & Temporal Variations, WFC3 ISR 2013-11.

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K. Sahu, C.M. Gosmeyer, S. Baggett, 2015, WFC3/UVIS Shutter Characterization, WFC3 ISR 2015-12.

M. Stiavelli, J. Sullivan, and C. Hanley, 2001, Modeling the Impact of Ghosts in WFC3/UVIS, WFC3 ISR 2001-17.

A. Suchkov & S. Baggett, 2012, WFC3/UVIS Crosstalk and Crosstalk Correction, WFC3 ISR 2012-02.

M. H. Wong, 2010, WFC3/UVIS Fringing: Ground test data and analysis codes, WFC3 TIR 2010-01, Available by request from http://hsthelp.stsci.edu.

M. H. Wong, 2010, Amplitude of fringing in WFC3/UVIS narrowband red filters, WFC3 ISR 2010-04.

«Previous Next»

WFC3 Data Handbook
- • Acknowledgments
- • What's New in This Revision
- Preface
  - • Handbook Structure
  - • Typographic Conventions
- Chapter 1: WFC3 Instruments
  - • 1.1 Instrument Overview
  - • 1.2 The UVIS Channel
  - • 1.3 The IR Channel
- Chapter 2: WFC3 Data Structure
  - • 2.1 Types of WFC3 Files
  - • 2.2 WFC3 File Structure
  - • 2.3 Data Storage Requirements
  - • 2.4 Headers and Keywords
- Chapter 3: WFC3 Data Calibration
  - • 3.1 The calwf3 Data Processing Pipeline
  - • 3.2 UVIS Data Calibration Steps
  - • 3.3 IR Data Calibration Steps
  - • 3.4 Pipeline Tasks
  - • 3.5 Manual Recalibration of WFC3 Data
- Chapter 4: WFC3 Images: Distortion Correction and AstroDrizzle
- Chapter 5: WFC3 UVIS Sources of Error
  - • 5.1 Gain and Read Noise
  - • 5.2 Bias Subtraction
  - • 5.3 Dark Current and Hot Pixels
  - • 5.4 UVIS Flat Fields
  - • 5.5 Image Anomalies
  - • 5.6 Generic Detector and Camera Properties
  - • 5.7 UVIS Photometry Errors
  - • 5.8 References
- Chapter 6: WFC3 UVIS Charge Transfer Efficiency - CTE
  - • 6.1 Overview
  - • 6.2 CTE Losses And Background
  - • 6.3 The Nature Of CTE Losses
  - • 6.4 The Pixel-Based Model
  - • 6.5 Empirical Corrections
  - • 6.6 Dealing With CTE Losses in WFC3 UVIS Images
  - • 6.7 Sink Pixels
  - • 6.8 References
- 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
  - • 7.11 IR Photometry Errors
  - • 7.12 References
- Chapter 8: Persistence in WFC3 IR
- Chapter 9: WFC3 Data Analysis
  - • 9.1 Photometry
  - • 9.2 Astrometry
  - • 9.3 Spectroscopy
  - • 9.4 STSDAS, STSCI_PYTHON and Astropy
  - • 9.5 Specific Tools for the Analysis of WFC3
  - • 9.6 References
- Chapter 10: WFC3 Spatial Scan Data
  - • 10.1 Analysis of Scanned Data
  - • 10.2 IR Scanned Data
  - • 10.3 UVIS Scanned Data
  - • 10.4 References

5.8 References

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