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Hubble Space Telescope
Wide Field Camera 3

The Horsehead Nebula in Infrared


Source: Hubblesite.org

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

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

News Archive

Documents added in the last 45 days

ISR 2014-19: Sink Pixels and CTE in the WFC3/UVIS Detector
Jay Anderson and Sylvia Baggett 14 Aug 2014

ISR 2014-18: Pixel-to-Pixel Flat Field Changes in WFC3/UVIS
H.Gunning, S. Baggett, J. MacKenty 08 Aug 2014

ISR 2014-17: Updated non-linearity calibration method for WFC3/IR
B. Hilbert 18 Jul 2014

ISR 2014-16: WFC3/UVIS Photometric Transformations
Kailash Sahu, Susana Deustua and Elena Sabbi 11 Jul 2014

Document Archive

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