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
Workaround for aXe issues on astroconda: Click Here
On June 15, 2017, 18 bias files, 4 post-flash files, and 1 image photometry table for WFC3/UVIS were delivered to the Calibration Reference Data System (CRDS) and went live in the 2017.2 release of the MAST processing pipeline for WFC3. These files will be used for processing all WFC3/UVIS data. Please check the [WFC3 reference file pages] and the [WFC3 Photometry website] for more information.
Documents added in the last 45 days
ISR 2017-22: WFC3 Anomalies Flagged by the Quicklook Team
C.M. Gosmeyer & The Quicklook Team 08 Sept 2017
M. Gennaro, V. Bajaj, K. Long 17 May 2018
Knox S. Long, & Sylvia M. Baggett 01 May 2018
If you need assistance with anything related to WFC3, please see the Help page.