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).
The UVIS and IR Channels are operating nominally.
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
Documents added in the last 45 days
C.M. Gosmeyer & S. Baggett 15 Mar 2017
J. Fowler & S. Baggett 15 Mar 2017
J. Mack 06 Mar 2017
P. McCullough 02 Mar 2017
N. Pirzkal & R. Ryan 20 Feb 2017
B. Sunnquist, S. Baggett & K. S. Long 15 Feb 2017
C. Martlin S. Baggett 13 Feb 2017
If you need assistance with anything related to WFC3, please see the Help page.