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Hubble Space Telescope
Wide Field Camera 3

The Horsehead Nebula in Infrared


The Wide Field Camera 3 (WFC3) is a fourth-generation UVIS/IR imager aboard the Hubble Space Telescope (HST). WFC3 was installed in May 2009 during HST servicing mission 4, and replaces the Wide Field Planetary Camera 2 (WFPC2).

WFC3 Status

The UVIS and IR Channels are operating nominally.

WFC3 STAN Archive
All Telescopes documents of interest to WFC3 users

Late Breaking News from the Last 45 Days

PandExo: A community tool for transiting exoplanet science with JWST & HST

Please note that the default aperture radius for WFC3/UVIS is 0.4 arcsec (90% of encircled energy). For 80% of encircled energy, use an aperture with radius 0.2 arcsec, comparable to the ACS default.

Quick-Start Advice to Run Reverse Correction for CTE now available here: CTE Tools

WFC3 Throughput are now available as text files: Throughput Tables

The color tool has been updated to include a new version of the NICMOS unit conversion form.

News Archive

Documents added in the last 45 days

ISR 2017-09: WFC3/UVIS External CTE Monitor: 2016 Updates on Coefficients and Analysis Pipeline
C.M. Gosmeyer & S. Baggett 15 Mar 2017

ISR 2017-08: Monitoring the WFC3/UVIS Relative Gain with Internal Flatfields
J. Fowler & S. Baggett 15 Mar 2017

ISR 2016-05: UVIS 2.0: Ultraviolet Flats
J. Mack 06 Mar 2017

ISR 2017-06: Trajectories of Multi-lined Spatial Scans
P. McCullough 02 Mar 2017

ISR 2017-05: Variable He I emission in grism data
N. Pirzkal & R. Ryan 20 Feb 2017

ISR 2017-04: An Exploration of WFC3/IR Dark Current Variation
B. Sunnquist, S. Baggett & K. S. Long 15 Feb 2017

ISR 2017-03: Long-term Stability of the Post-Flash LED Lamp
C. Martlin S. Baggett 13 Feb 2017

Document Archive

If you need assistance with anything related to WFC3, please see the Help page.